The following information is also available:
Time column is TIME ORDERED-> Determining observation start and end
Offset of 172474373.967600 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1998-06-20 05:32:49.96759 Modified Julian Day = 50984.231133884255541-> leapsec.fits already present in current directory
Offset of 172504837.870200 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1998-06-20 14:00:33.87020 Modified Julian Day = 50984.583725349541055-> Observation begins 172474373.9676 1998-06-20 05:32:49
ATTITUDE_V0.9j reading attitude file:./merged.tmp open asc output file:out.tmp AVERAGE ASPECT AND OFFSET FOR THIS ATTITUDE FILE: Attitude file start and stop ascatime : 172474373.967400 172504849.870300 Data file start and stop ascatime : 172474373.967400 172504849.870300 Aspecting run start and stop ascatime : 172474373.967500 172504849.870192 Time interval averaged over (seconds) : 30475.902691 Total pointing and manuver time (sec) : 19347.984375 11127.985352 Mean boresight Euler angles : 188.268099 81.917068 142.337604 RA DEC SUN ANGLE Mean solar position (deg) : 87.73 23.42 Mean aberration (arcsec) : 3.66 2.54 Mean sat X-axis (deg) : 288.592486 51.606174 102.77 Mean sat Y-axis (deg) : 92.074283 37.224353 14.30 Mean sat Z-axis (deg) : 188.268099 8.082932 96.33 RA DEC ROLL OFFSET (deg) (deg) (deg) (arcmin) Average 187.985245 8.131683 52.377583 0.152325 Minimum 187.983734 8.109540 52.357903 0.000000 Maximum 188.104111 8.248934 52.759361 92.595970 Sigma (RMS) 0.000631 0.000578 0.003727 0.603806 Number of ASPECT records processed = 26552 Aspecting to RA/DEC : 187.98524475 8.13168335 closing output file... closing attitude file...-> Standard Output From STOOL checkatt:
Opening file: ./out.tmp ***************** Observation Info ****************** RA (J2000 deg): 187.985 DEC: 8.132 START TIME: SC 172474373.9675 = UT 1998-06-20 05:32:53 ****** Definition of Attitude SENSOR Bit Flags ****** Sensors used in the attitude determination and attitude control mode 1: USED, 0: NOT USED B0:STT-A, B1:STT-B, B2:NSAS, B3:GAS, B4:SSAS-SA, B5:SSAS-SB, B6:IRU-X, B7:IRU-Y, B8:IRU-Z, B9:IRU-S1, B10:IRU-S2, B11: Attitude control mode 1: coarse, 0: fine B12: Sun presence 1: day, 0: night B13: STT-A earth occultation 1: earth occultation, 0: no occultation B14: STT-B earth occultation 1: earth occultation, 0: no occultation B16,17,18: STT-A track stars no.1,2,3, 1: USED, 0: NOT USED B19,20,21: STT-B track stars no.1,2,3, 1: USED, 0: NOT USED B22,23: always 0 ******** Attitude File Reconstruction Summary ******* S S N G S S I I I I I A S S S S S T T S A S S R R R R R C U T T T T T T A S A A U U U U U M N T T T T - - S . A A - - - - - . . - - - - A B . . - - X Y Z S S . . A B A B . . . . S S . . . 1 2 . . O O S S offset_time separation sensor . . . . A B . . . . . . . C C T T (sec) (arcmin) . . . . . . . . . . . . . C C R R BIT: 0 1 2 3 4 5 6 7 8 9 A B C D E 4.000078 1.308 8603 1 1 0 0 0 0 0 0 0 1 1 0 0 0 0 0 0 2587.991455 1.256 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0 3575.988037 0.255 8803 1 1 0 0 0 0 0 0 0 0 0 1 0 0 0 0 0 4811.983887 0.070 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 8321.972656 0.092 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0 10539.965820 0.151 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 14057.954102 0.148 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0 16283.947266 0.042 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 19793.935547 0.054 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0 22027.929688 0.115 9C80C3 1 1 0 0 0 0 1 1 0 0 0 0 0 0 0 4 3 25527.917969 0.180 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0 27787.912109 0.287 9C80C3 1 1 0 0 0 0 1 1 0 0 0 0 0 0 0 4 3 30459.902344 9.966 9603 1 1 0 0 0 0 0 0 0 1 1 0 1 0 0 0 0 30475.902344 92.596 9E03 1 1 0 0 0 0 0 0 0 1 1 1 1 0 0 0 0 Attitude Records: 26552 Attitude Steps: 14 Maneuver ACM time: 11128.0 sec Pointed ACM time: 19348.0 sec-> Calculating aspect point
99 97 count=12992 sum1=2.44598e+06 sum2=1.06424e+06 sum3=1.84926e+06 99 98 count=12786 sum1=2.40721e+06 sum2=1.0474e+06 sum3=1.81993e+06 99 99 count=54 sum1=10166.6 sum2=4424.31 sum3=7685.85 99 100 count=717 sum1=134988 sum2=58749.4 sum3=102045 100 100 count=1 sum1=188.276 sum2=81.937 sum3=142.375 111 86 count=1 sum1=188.387 sum2=81.8 sum3=142.34 1 out of 26552 points outside bin structure-> Euler angles: 188.269, 81.9167, 142.338
Interpolating 16 records in time interval 172504813.87 - 172504833.87 Interpolating 145 records in time interval 172504833.87 - 172504849.87
59.9998 second gap between superframes 332 and 333 Dropping SF 511 with inconsistent datamode 0/31 Dropping SF 512 with corrupted frame indicator Dropping SF 514 with inconsistent datamode 0/31 Dropping SF 711 with corrupted frame indicator Dropping SF 713 with invalid bit rate 7 106 second gap between superframes 2704 and 2705 Warning: GIS2 bit assignment changed between 172487771.92391 and 172487773.9239 Warning: GIS3 bit assignment changed between 172487775.92389 and 172487777.92389 Warning: GIS2 bit assignment changed between 172487785.92386 and 172487787.92386 Warning: GIS3 bit assignment changed between 172487791.92384 and 172487793.92384 Dropping SF 3066 with inconsistent datamode 0/31 Dropping SF 3067 with inconsistent datamode 0/31 Dropping SF 5103 with synch code word 0 = 94 not 250 Dropping SF 5440 with inconsistent datamode 0/31 Dropping SF 5441 with inconsistent datamode 0/31 Dropping SF 6215 with invalid bit rate 7 6647 of 6658 super frames processed-> Removing the following files with NEVENTS=0
ft980620_0532_1400G200970M.fits[0] ft980620_0532_1400G201070L.fits[0] ft980620_0532_1400G201670H.fits[0] ft980620_0532_1400G201770H.fits[0] ft980620_0532_1400G201870M.fits[0] ft980620_0532_1400G201970M.fits[0] ft980620_0532_1400G202070H.fits[0] ft980620_0532_1400G202170H.fits[0] ft980620_0532_1400G202270H.fits[0] ft980620_0532_1400G202370H.fits[0] ft980620_0532_1400G202470H.fits[0] ft980620_0532_1400G202670H.fits[0] ft980620_0532_1400G202970H.fits[0] ft980620_0532_1400G203070H.fits[0] ft980620_0532_1400G203170H.fits[0] ft980620_0532_1400G203270H.fits[0] ft980620_0532_1400G203970M.fits[0] ft980620_0532_1400G204070H.fits[0] ft980620_0532_1400G204170H.fits[0] ft980620_0532_1400G204270H.fits[0] ft980620_0532_1400G204370H.fits[0] ft980620_0532_1400G204470H.fits[0] ft980620_0532_1400G204570H.fits[0] ft980620_0532_1400G205170L.fits[0] ft980620_0532_1400G300970M.fits[0] ft980620_0532_1400G301070L.fits[0] ft980620_0532_1400G301670H.fits[0] ft980620_0532_1400G301770H.fits[0] ft980620_0532_1400G301870M.fits[0] ft980620_0532_1400G301970M.fits[0] ft980620_0532_1400G302070H.fits[0] ft980620_0532_1400G302170H.fits[0] ft980620_0532_1400G302270H.fits[0] ft980620_0532_1400G302370H.fits[0] ft980620_0532_1400G302470H.fits[0] ft980620_0532_1400G303070H.fits[0] ft980620_0532_1400G303170H.fits[0] ft980620_0532_1400G303270H.fits[0] ft980620_0532_1400G303970M.fits[0] ft980620_0532_1400G304070H.fits[0] ft980620_0532_1400G304170H.fits[0] ft980620_0532_1400G304270H.fits[0] ft980620_0532_1400G304370H.fits[0] ft980620_0532_1400G305170L.fits[0] ft980620_0532_1400S001301M.fits[0] ft980620_0532_1400S101301M.fits[0]-> Checking for empty GTI extensions
ft980620_0532_1400S000101M.fits[2] ft980620_0532_1400S000201L.fits[2] ft980620_0532_1400S000301M.fits[2] ft980620_0532_1400S000401L.fits[2] ft980620_0532_1400S000501L.fits[2] ft980620_0532_1400S000601M.fits[2] ft980620_0532_1400S000701H.fits[2] ft980620_0532_1400S000801M.fits[2] ft980620_0532_1400S000901M.fits[2] ft980620_0532_1400S001001M.fits[2] ft980620_0532_1400S001101H.fits[2] ft980620_0532_1400S001201M.fits[2] ft980620_0532_1400S001401M.fits[2] ft980620_0532_1400S001501H.fits[2] ft980620_0532_1400S001601M.fits[2] ft980620_0532_1400S001701L.fits[2] ft980620_0532_1400S001801L.fits[2] ft980620_0532_1400S001901L.fits[2] ft980620_0532_1400S002001M.fits[2] ft980620_0532_1400S002101H.fits[2] ft980620_0532_1400S002201M.fits[2] ft980620_0532_1400S002301L.fits[2] ft980620_0532_1400S002401M.fits[2]-> Merging GTIs from the following files:
ft980620_0532_1400S100101M.fits[2] ft980620_0532_1400S100201L.fits[2] ft980620_0532_1400S100301M.fits[2] ft980620_0532_1400S100401L.fits[2] ft980620_0532_1400S100501L.fits[2] ft980620_0532_1400S100601M.fits[2] ft980620_0532_1400S100701H.fits[2] ft980620_0532_1400S100801M.fits[2] ft980620_0532_1400S100901M.fits[2] ft980620_0532_1400S101001M.fits[2] ft980620_0532_1400S101101H.fits[2] ft980620_0532_1400S101201M.fits[2] ft980620_0532_1400S101401M.fits[2] ft980620_0532_1400S101501H.fits[2] ft980620_0532_1400S101601M.fits[2] ft980620_0532_1400S101701L.fits[2] ft980620_0532_1400S101801L.fits[2] ft980620_0532_1400S101901L.fits[2] ft980620_0532_1400S102001M.fits[2] ft980620_0532_1400S102101H.fits[2] ft980620_0532_1400S102201M.fits[2] ft980620_0532_1400S102301L.fits[2] ft980620_0532_1400S102401M.fits[2]-> Merging GTIs from the following files:
ft980620_0532_1400G200170M.fits[2] ft980620_0532_1400G200270L.fits[2] ft980620_0532_1400G200370L.fits[2] ft980620_0532_1400G200470M.fits[2] ft980620_0532_1400G200570M.fits[2] ft980620_0532_1400G200670M.fits[2] ft980620_0532_1400G200770M.fits[2] ft980620_0532_1400G200870M.fits[2] ft980620_0532_1400G201170L.fits[2] ft980620_0532_1400G201270L.fits[2] ft980620_0532_1400G201370M.fits[2] ft980620_0532_1400G201470H.fits[2] ft980620_0532_1400G201570H.fits[2] ft980620_0532_1400G202570H.fits[2] ft980620_0532_1400G202770H.fits[2] ft980620_0532_1400G202870H.fits[2] ft980620_0532_1400G203370H.fits[2] ft980620_0532_1400G203470H.fits[2] ft980620_0532_1400G203570H.fits[2] ft980620_0532_1400G203670H.fits[2] ft980620_0532_1400G203770M.fits[2] ft980620_0532_1400G203870M.fits[2] ft980620_0532_1400G204670H.fits[2] ft980620_0532_1400G204770H.fits[2] ft980620_0532_1400G204870M.fits[2] ft980620_0532_1400G204970M.fits[2] ft980620_0532_1400G205070L.fits[2] ft980620_0532_1400G205270L.fits[2] ft980620_0532_1400G205370M.fits[2] ft980620_0532_1400G205470M.fits[2] ft980620_0532_1400G205570M.fits[2] ft980620_0532_1400G205670M.fits[2] ft980620_0532_1400G205770H.fits[2] ft980620_0532_1400G205870H.fits[2] ft980620_0532_1400G205970H.fits[2] ft980620_0532_1400G206070H.fits[2] ft980620_0532_1400G206170M.fits[2] ft980620_0532_1400G206270M.fits[2] ft980620_0532_1400G206370L.fits[2] ft980620_0532_1400G206470L.fits[2] ft980620_0532_1400G206570L.fits[2] ft980620_0532_1400G206670L.fits[2] ft980620_0532_1400G206770M.fits[2] ft980620_0532_1400G206870M.fits[2] ft980620_0532_1400G206970M.fits[2] ft980620_0532_1400G207070M.fits[2]-> Merging GTIs from the following files:
ft980620_0532_1400G300170M.fits[2] ft980620_0532_1400G300270L.fits[2] ft980620_0532_1400G300370L.fits[2] ft980620_0532_1400G300470M.fits[2] ft980620_0532_1400G300570M.fits[2] ft980620_0532_1400G300670M.fits[2] ft980620_0532_1400G300770M.fits[2] ft980620_0532_1400G300870M.fits[2] ft980620_0532_1400G301170L.fits[2] ft980620_0532_1400G301270L.fits[2] ft980620_0532_1400G301370M.fits[2] ft980620_0532_1400G301470H.fits[2] ft980620_0532_1400G301570H.fits[2] ft980620_0532_1400G302570H.fits[2] ft980620_0532_1400G302670H.fits[2] ft980620_0532_1400G302770H.fits[2] ft980620_0532_1400G302870H.fits[2] ft980620_0532_1400G302970H.fits[2] ft980620_0532_1400G303370H.fits[2] ft980620_0532_1400G303470H.fits[2] ft980620_0532_1400G303570H.fits[2] ft980620_0532_1400G303670H.fits[2] ft980620_0532_1400G303770M.fits[2] ft980620_0532_1400G303870M.fits[2] ft980620_0532_1400G304470H.fits[2] ft980620_0532_1400G304570H.fits[2] ft980620_0532_1400G304670H.fits[2] ft980620_0532_1400G304770H.fits[2] ft980620_0532_1400G304870M.fits[2] ft980620_0532_1400G304970M.fits[2] ft980620_0532_1400G305070L.fits[2] ft980620_0532_1400G305270L.fits[2] ft980620_0532_1400G305370M.fits[2] ft980620_0532_1400G305470M.fits[2] ft980620_0532_1400G305570M.fits[2] ft980620_0532_1400G305670M.fits[2] ft980620_0532_1400G305770H.fits[2] ft980620_0532_1400G305870H.fits[2] ft980620_0532_1400G305970H.fits[2] ft980620_0532_1400G306070H.fits[2] ft980620_0532_1400G306170M.fits[2] ft980620_0532_1400G306270M.fits[2] ft980620_0532_1400G306370L.fits[2] ft980620_0532_1400G306470L.fits[2] ft980620_0532_1400G306570L.fits[2] ft980620_0532_1400G306670L.fits[2] ft980620_0532_1400G306770M.fits[2] ft980620_0532_1400G306870M.fits[2] ft980620_0532_1400G306970M.fits[2] ft980620_0532_1400G307070M.fits[2]
GISSORTCODE:LO:Start program GISSORTCODE:LO:End program-> Standard Error Output From STOOL gissortsplit:
GISSORTSPLIT:LO:Start program GISSORTSPLIT:LO:g200170h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200270h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200370h.prelist merge count = 8 photon cnt = 9093 GISSORTSPLIT:LO:g200470h.prelist merge count = 1 photon cnt = 5 GISSORTSPLIT:LO:g200570h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200670h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200770h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200870h.prelist merge count = 1 photon cnt = 5 GISSORTSPLIT:LO:g200170l.prelist merge count = 1 photon cnt = 4 GISSORTSPLIT:LO:g200270l.prelist merge count = 3 photon cnt = 296 GISSORTSPLIT:LO:g200370l.prelist merge count = 5 photon cnt = 2570 GISSORTSPLIT:LO:g200470l.prelist merge count = 1 photon cnt = 173 GISSORTSPLIT:LO:g200170m.prelist merge count = 1 photon cnt = 8 GISSORTSPLIT:LO:g200270m.prelist merge count = 1 photon cnt = 4 GISSORTSPLIT:LO:g200370m.prelist merge count = 7 photon cnt = 6796 GISSORTSPLIT:LO:g200470m.prelist merge count = 6 photon cnt = 100 GISSORTSPLIT:LO:g200570m.prelist merge count = 1 photon cnt = 15 GISSORTSPLIT:LO:g200670m.prelist merge count = 1 photon cnt = 13 GISSORTSPLIT:LO:g200770m.prelist merge count = 1 photon cnt = 13 GISSORTSPLIT:LO:g200870m.prelist merge count = 1 photon cnt = 16 GISSORTSPLIT:LO:g200970m.prelist merge count = 1 photon cnt = 20 GISSORTSPLIT:LO:g201070m.prelist merge count = 1 photon cnt = 24 GISSORTSPLIT:LO:Total filenames split = 46 GISSORTSPLIT:LO:Total split file cnt = 22 GISSORTSPLIT:LO:End program-> Creating ad86032020g200170h.unf
---- cmerge: version 1.6 ---- A total of 8 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G201470H.fits 2 -- ft980620_0532_1400G201570H.fits 3 -- ft980620_0532_1400G202770H.fits 4 -- ft980620_0532_1400G202870H.fits 5 -- ft980620_0532_1400G203570H.fits 6 -- ft980620_0532_1400G203670H.fits 7 -- ft980620_0532_1400G204770H.fits 8 -- ft980620_0532_1400G206070H.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G201470H.fits 2 -- ft980620_0532_1400G201570H.fits 3 -- ft980620_0532_1400G202770H.fits 4 -- ft980620_0532_1400G202870H.fits 5 -- ft980620_0532_1400G203570H.fits 6 -- ft980620_0532_1400G203670H.fits 7 -- ft980620_0532_1400G204770H.fits 8 -- ft980620_0532_1400G206070H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020g200270m.unf
---- cmerge: version 1.6 ---- A total of 7 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G200170M.fits 2 -- ft980620_0532_1400G200770M.fits 3 -- ft980620_0532_1400G201370M.fits 4 -- ft980620_0532_1400G204970M.fits 5 -- ft980620_0532_1400G205670M.fits 6 -- ft980620_0532_1400G206270M.fits 7 -- ft980620_0532_1400G207070M.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G200170M.fits 2 -- ft980620_0532_1400G200770M.fits 3 -- ft980620_0532_1400G201370M.fits 4 -- ft980620_0532_1400G204970M.fits 5 -- ft980620_0532_1400G205670M.fits 6 -- ft980620_0532_1400G206270M.fits 7 -- ft980620_0532_1400G207070M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020g200370l.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G200370L.fits 2 -- ft980620_0532_1400G201270L.fits 3 -- ft980620_0532_1400G205070L.fits 4 -- ft980620_0532_1400G206370L.fits 5 -- ft980620_0532_1400G206670L.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G200370L.fits 2 -- ft980620_0532_1400G201270L.fits 3 -- ft980620_0532_1400G205070L.fits 4 -- ft980620_0532_1400G206370L.fits 5 -- ft980620_0532_1400G206670L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000296 events
ft980620_0532_1400G201170L.fits ft980620_0532_1400G205270L.fits ft980620_0532_1400G206570L.fits-> Ignoring the following files containing 000000173 events
ft980620_0532_1400G200270L.fits-> Ignoring the following files containing 000000100 events
ft980620_0532_1400G200670M.fits ft980620_0532_1400G203770M.fits ft980620_0532_1400G204870M.fits ft980620_0532_1400G205570M.fits ft980620_0532_1400G206170M.fits ft980620_0532_1400G206970M.fits-> Ignoring the following files containing 000000024 events
ft980620_0532_1400G205470M.fits-> Ignoring the following files containing 000000020 events
ft980620_0532_1400G205370M.fits-> Ignoring the following files containing 000000016 events
ft980620_0532_1400G200570M.fits-> Ignoring the following files containing 000000015 events
ft980620_0532_1400G206770M.fits-> Ignoring the following files containing 000000013 events
ft980620_0532_1400G200470M.fits-> Ignoring the following files containing 000000013 events
ft980620_0532_1400G206870M.fits-> Ignoring the following files containing 000000008 events
ft980620_0532_1400G200870M.fits-> Ignoring the following files containing 000000005 events
ft980620_0532_1400G203470H.fits-> Ignoring the following files containing 000000005 events
ft980620_0532_1400G205970H.fits-> Ignoring the following files containing 000000004 events
ft980620_0532_1400G203870M.fits-> Ignoring the following files containing 000000004 events
ft980620_0532_1400G206470L.fits-> Ignoring the following files containing 000000002 events
ft980620_0532_1400G203370H.fits-> Ignoring the following files containing 000000002 events
ft980620_0532_1400G205870H.fits-> Ignoring the following files containing 000000001 events
ft980620_0532_1400G205770H.fits-> Ignoring the following files containing 000000001 events
ft980620_0532_1400G204670H.fits-> Ignoring the following files containing 000000001 events
ft980620_0532_1400G202570H.fits-> Collecting GIS3 event files by mode
GISSORTCODE:LO:Start program GISSORTCODE:LO:End program-> Standard Error Output From STOOL gissortsplit:
GISSORTSPLIT:LO:Start program GISSORTSPLIT:LO:g300170h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g300270h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300370h.prelist merge count = 2 photon cnt = 3 GISSORTSPLIT:LO:g300470h.prelist merge count = 2 photon cnt = 5 GISSORTSPLIT:LO:g300570h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g300670h.prelist merge count = 8 photon cnt = 8587 GISSORTSPLIT:LO:g300770h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g300870h.prelist merge count = 1 photon cnt = 3 GISSORTSPLIT:LO:g300970h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g301070h.prelist merge count = 1 photon cnt = 7 GISSORTSPLIT:LO:g300170l.prelist merge count = 1 photon cnt = 3 GISSORTSPLIT:LO:g300270l.prelist merge count = 3 photon cnt = 303 GISSORTSPLIT:LO:g300370l.prelist merge count = 5 photon cnt = 2437 GISSORTSPLIT:LO:g300470l.prelist merge count = 1 photon cnt = 194 GISSORTSPLIT:LO:g300170m.prelist merge count = 1 photon cnt = 4 GISSORTSPLIT:LO:g300270m.prelist merge count = 1 photon cnt = 6 GISSORTSPLIT:LO:g300370m.prelist merge count = 7 photon cnt = 6429 GISSORTSPLIT:LO:g300470m.prelist merge count = 6 photon cnt = 99 GISSORTSPLIT:LO:g300570m.prelist merge count = 1 photon cnt = 31 GISSORTSPLIT:LO:g300670m.prelist merge count = 1 photon cnt = 32 GISSORTSPLIT:LO:g300770m.prelist merge count = 1 photon cnt = 22 GISSORTSPLIT:LO:g300870m.prelist merge count = 1 photon cnt = 10 GISSORTSPLIT:LO:g300970m.prelist merge count = 1 photon cnt = 18 GISSORTSPLIT:LO:g301070m.prelist merge count = 1 photon cnt = 17 GISSORTSPLIT:LO:Total filenames split = 50 GISSORTSPLIT:LO:Total split file cnt = 24 GISSORTSPLIT:LO:End program-> Creating ad86032020g300170h.unf
---- cmerge: version 1.6 ---- A total of 8 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G301470H.fits 2 -- ft980620_0532_1400G301570H.fits 3 -- ft980620_0532_1400G302770H.fits 4 -- ft980620_0532_1400G302870H.fits 5 -- ft980620_0532_1400G303570H.fits 6 -- ft980620_0532_1400G303670H.fits 7 -- ft980620_0532_1400G304770H.fits 8 -- ft980620_0532_1400G306070H.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G301470H.fits 2 -- ft980620_0532_1400G301570H.fits 3 -- ft980620_0532_1400G302770H.fits 4 -- ft980620_0532_1400G302870H.fits 5 -- ft980620_0532_1400G303570H.fits 6 -- ft980620_0532_1400G303670H.fits 7 -- ft980620_0532_1400G304770H.fits 8 -- ft980620_0532_1400G306070H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020g300270m.unf
---- cmerge: version 1.6 ---- A total of 7 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G300170M.fits 2 -- ft980620_0532_1400G300770M.fits 3 -- ft980620_0532_1400G301370M.fits 4 -- ft980620_0532_1400G304970M.fits 5 -- ft980620_0532_1400G305670M.fits 6 -- ft980620_0532_1400G306270M.fits 7 -- ft980620_0532_1400G307070M.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G300170M.fits 2 -- ft980620_0532_1400G300770M.fits 3 -- ft980620_0532_1400G301370M.fits 4 -- ft980620_0532_1400G304970M.fits 5 -- ft980620_0532_1400G305670M.fits 6 -- ft980620_0532_1400G306270M.fits 7 -- ft980620_0532_1400G307070M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020g300370l.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400G300370L.fits 2 -- ft980620_0532_1400G301270L.fits 3 -- ft980620_0532_1400G305070L.fits 4 -- ft980620_0532_1400G306370L.fits 5 -- ft980620_0532_1400G306670L.fits Merging binary extension #: 2 1 -- ft980620_0532_1400G300370L.fits 2 -- ft980620_0532_1400G301270L.fits 3 -- ft980620_0532_1400G305070L.fits 4 -- ft980620_0532_1400G306370L.fits 5 -- ft980620_0532_1400G306670L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000303 events
ft980620_0532_1400G301170L.fits ft980620_0532_1400G305270L.fits ft980620_0532_1400G306570L.fits-> Ignoring the following files containing 000000194 events
ft980620_0532_1400G300270L.fits-> Ignoring the following files containing 000000099 events
ft980620_0532_1400G300670M.fits ft980620_0532_1400G303770M.fits ft980620_0532_1400G304870M.fits ft980620_0532_1400G305570M.fits ft980620_0532_1400G306170M.fits ft980620_0532_1400G306970M.fits-> Ignoring the following files containing 000000032 events
ft980620_0532_1400G305470M.fits-> Ignoring the following files containing 000000031 events
ft980620_0532_1400G305370M.fits-> Ignoring the following files containing 000000022 events
ft980620_0532_1400G300470M.fits-> Ignoring the following files containing 000000018 events
ft980620_0532_1400G306770M.fits-> Ignoring the following files containing 000000017 events
ft980620_0532_1400G306870M.fits-> Ignoring the following files containing 000000010 events
ft980620_0532_1400G300570M.fits-> Ignoring the following files containing 000000007 events
ft980620_0532_1400G302970H.fits-> Ignoring the following files containing 000000006 events
ft980620_0532_1400G303870M.fits-> Ignoring the following files containing 000000005 events
ft980620_0532_1400G302670H.fits ft980620_0532_1400G304670H.fits-> Ignoring the following files containing 000000004 events
ft980620_0532_1400G300870M.fits-> Ignoring the following files containing 000000003 events
ft980620_0532_1400G305770H.fits-> Ignoring the following files containing 000000003 events
ft980620_0532_1400G302570H.fits ft980620_0532_1400G304570H.fits-> Ignoring the following files containing 000000003 events
ft980620_0532_1400G306470L.fits-> Ignoring the following files containing 000000002 events
ft980620_0532_1400G305870H.fits-> Ignoring the following files containing 000000002 events
ft980620_0532_1400G305970H.fits-> Ignoring the following files containing 000000002 events
ft980620_0532_1400G303370H.fits-> Ignoring the following files containing 000000001 events
ft980620_0532_1400G303470H.fits-> Ignoring the following files containing 000000001 events
ft980620_0532_1400G304470H.fits-> Collecting SIS0 event files by mode
SIS0SORTCODE:LO:Start program SIS0SORTCODE:LO:End program-> Standard Error Output From STOOL sis0sortsplit:
SIS0SORTSPLIT:LO:Start program SIS0SORTSPLIT:LO:s000101h.prelist merge count = 4 photon cnt = 92384 SIS0SORTSPLIT:LO:s000201l.prelist merge count = 5 photon cnt = 9093 SIS0SORTSPLIT:LO:s000301l.prelist merge count = 2 photon cnt = 112 SIS0SORTSPLIT:LO:s000401m.prelist merge count = 11 photon cnt = 21693 SIS0SORTSPLIT:LO:s000501m.prelist merge count = 1 photon cnt = 8 SIS0SORTSPLIT:LO:Total filenames split = 23 SIS0SORTSPLIT:LO:Total split file cnt = 5 SIS0SORTSPLIT:LO:End program-> Creating ad86032020s000101h.unf
---- cmerge: version 1.6 ---- A total of 4 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S000701H.fits 2 -- ft980620_0532_1400S001101H.fits 3 -- ft980620_0532_1400S001501H.fits 4 -- ft980620_0532_1400S002101H.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S000701H.fits 2 -- ft980620_0532_1400S001101H.fits 3 -- ft980620_0532_1400S001501H.fits 4 -- ft980620_0532_1400S002101H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020s000201m.unf
---- cmerge: version 1.6 ---- A total of 11 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S000101M.fits 2 -- ft980620_0532_1400S000301M.fits 3 -- ft980620_0532_1400S000601M.fits 4 -- ft980620_0532_1400S000801M.fits 5 -- ft980620_0532_1400S001001M.fits 6 -- ft980620_0532_1400S001201M.fits 7 -- ft980620_0532_1400S001401M.fits 8 -- ft980620_0532_1400S001601M.fits 9 -- ft980620_0532_1400S002001M.fits 10 -- ft980620_0532_1400S002201M.fits 11 -- ft980620_0532_1400S002401M.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S000101M.fits 2 -- ft980620_0532_1400S000301M.fits 3 -- ft980620_0532_1400S000601M.fits 4 -- ft980620_0532_1400S000801M.fits 5 -- ft980620_0532_1400S001001M.fits 6 -- ft980620_0532_1400S001201M.fits 7 -- ft980620_0532_1400S001401M.fits 8 -- ft980620_0532_1400S001601M.fits 9 -- ft980620_0532_1400S002001M.fits 10 -- ft980620_0532_1400S002201M.fits 11 -- ft980620_0532_1400S002401M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020s000301l.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S000201L.fits 2 -- ft980620_0532_1400S000501L.fits 3 -- ft980620_0532_1400S001701L.fits 4 -- ft980620_0532_1400S001901L.fits 5 -- ft980620_0532_1400S002301L.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S000201L.fits 2 -- ft980620_0532_1400S000501L.fits 3 -- ft980620_0532_1400S001701L.fits 4 -- ft980620_0532_1400S001901L.fits 5 -- ft980620_0532_1400S002301L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000112 events
ft980620_0532_1400S000401L.fits ft980620_0532_1400S001801L.fits-> Ignoring the following files containing 000000008 events
ft980620_0532_1400S000901M.fits-> Collecting SIS1 event files by mode
SIS1SORTCODE:LO:Start program SIS1SORTCODE:LO:End program-> Standard Error Output From STOOL sis1sortsplit:
SIS1SORTSPLIT:LO:Start program SIS1SORTSPLIT:LO:s100101h.prelist merge count = 4 photon cnt = 111123 SIS1SORTSPLIT:LO:s100201l.prelist merge count = 5 photon cnt = 9640 SIS1SORTSPLIT:LO:s100301l.prelist merge count = 2 photon cnt = 112 SIS1SORTSPLIT:LO:s100401m.prelist merge count = 11 photon cnt = 41125 SIS1SORTSPLIT:LO:s100501m.prelist merge count = 1 photon cnt = 32 SIS1SORTSPLIT:LO:Total filenames split = 23 SIS1SORTSPLIT:LO:Total split file cnt = 5 SIS1SORTSPLIT:LO:End program-> Creating ad86032020s100101h.unf
---- cmerge: version 1.6 ---- A total of 4 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S100701H.fits 2 -- ft980620_0532_1400S101101H.fits 3 -- ft980620_0532_1400S101501H.fits 4 -- ft980620_0532_1400S102101H.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S100701H.fits 2 -- ft980620_0532_1400S101101H.fits 3 -- ft980620_0532_1400S101501H.fits 4 -- ft980620_0532_1400S102101H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020s100201m.unf
---- cmerge: version 1.6 ---- A total of 11 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S100101M.fits 2 -- ft980620_0532_1400S100301M.fits 3 -- ft980620_0532_1400S100601M.fits 4 -- ft980620_0532_1400S100801M.fits 5 -- ft980620_0532_1400S101001M.fits 6 -- ft980620_0532_1400S101201M.fits 7 -- ft980620_0532_1400S101401M.fits 8 -- ft980620_0532_1400S101601M.fits 9 -- ft980620_0532_1400S102001M.fits 10 -- ft980620_0532_1400S102201M.fits 11 -- ft980620_0532_1400S102401M.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S100101M.fits 2 -- ft980620_0532_1400S100301M.fits 3 -- ft980620_0532_1400S100601M.fits 4 -- ft980620_0532_1400S100801M.fits 5 -- ft980620_0532_1400S101001M.fits 6 -- ft980620_0532_1400S101201M.fits 7 -- ft980620_0532_1400S101401M.fits 8 -- ft980620_0532_1400S101601M.fits 9 -- ft980620_0532_1400S102001M.fits 10 -- ft980620_0532_1400S102201M.fits 11 -- ft980620_0532_1400S102401M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad86032020s100301l.unf
---- cmerge: version 1.6 ---- A total of 5 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft980620_0532_1400S100201L.fits 2 -- ft980620_0532_1400S100501L.fits 3 -- ft980620_0532_1400S101701L.fits 4 -- ft980620_0532_1400S101901L.fits 5 -- ft980620_0532_1400S102301L.fits Merging binary extension #: 2 1 -- ft980620_0532_1400S100201L.fits 2 -- ft980620_0532_1400S100501L.fits 3 -- ft980620_0532_1400S101701L.fits 4 -- ft980620_0532_1400S101901L.fits 5 -- ft980620_0532_1400S102301L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000112 events
ft980620_0532_1400S100401L.fits ft980620_0532_1400S101801L.fits-> Ignoring the following files containing 000000032 events
ft980620_0532_1400S100901M.fits-> Tar-ing together the leftover raw files
a ft980620_0532_1400G200270L.fits 34K a ft980620_0532_1400G200470M.fits 31K a ft980620_0532_1400G200570M.fits 31K a ft980620_0532_1400G200670M.fits 31K a ft980620_0532_1400G200870M.fits 31K a ft980620_0532_1400G201170L.fits 31K a ft980620_0532_1400G202570H.fits 31K a ft980620_0532_1400G203370H.fits 31K a ft980620_0532_1400G203470H.fits 31K a ft980620_0532_1400G203770M.fits 31K a ft980620_0532_1400G203870M.fits 31K a ft980620_0532_1400G204670H.fits 31K a ft980620_0532_1400G204870M.fits 31K a ft980620_0532_1400G205270L.fits 31K a ft980620_0532_1400G205370M.fits 31K a ft980620_0532_1400G205470M.fits 31K a ft980620_0532_1400G205570M.fits 31K a ft980620_0532_1400G205770H.fits 31K a ft980620_0532_1400G205870H.fits 31K a ft980620_0532_1400G205970H.fits 31K a ft980620_0532_1400G206170M.fits 31K a ft980620_0532_1400G206470L.fits 31K a ft980620_0532_1400G206570L.fits 34K a ft980620_0532_1400G206770M.fits 31K a ft980620_0532_1400G206870M.fits 31K a ft980620_0532_1400G206970M.fits 31K a ft980620_0532_1400G300270L.fits 37K a ft980620_0532_1400G300470M.fits 31K a ft980620_0532_1400G300570M.fits 31K a ft980620_0532_1400G300670M.fits 31K a ft980620_0532_1400G300870M.fits 31K a ft980620_0532_1400G301170L.fits 31K a ft980620_0532_1400G302570H.fits 31K a ft980620_0532_1400G302670H.fits 31K a ft980620_0532_1400G302970H.fits 31K a ft980620_0532_1400G303370H.fits 31K a ft980620_0532_1400G303470H.fits 31K a ft980620_0532_1400G303770M.fits 31K a ft980620_0532_1400G303870M.fits 31K a ft980620_0532_1400G304470H.fits 31K a ft980620_0532_1400G304570H.fits 31K a ft980620_0532_1400G304670H.fits 31K a ft980620_0532_1400G304870M.fits 31K a ft980620_0532_1400G305270L.fits 34K a ft980620_0532_1400G305370M.fits 31K a ft980620_0532_1400G305470M.fits 31K a ft980620_0532_1400G305570M.fits 31K a ft980620_0532_1400G305770H.fits 31K a ft980620_0532_1400G305870H.fits 31K a ft980620_0532_1400G305970H.fits 31K a ft980620_0532_1400G306170M.fits 31K a ft980620_0532_1400G306470L.fits 31K a ft980620_0532_1400G306570L.fits 34K a ft980620_0532_1400G306770M.fits 31K a ft980620_0532_1400G306870M.fits 31K a ft980620_0532_1400G306970M.fits 31K a ft980620_0532_1400S000401L.fits 29K a ft980620_0532_1400S000901M.fits 29K a ft980620_0532_1400S001801L.fits 31K a ft980620_0532_1400S100401L.fits 29K a ft980620_0532_1400S100901M.fits 29K a ft980620_0532_1400S101801L.fits 31K-> Checking OBJECT keywords in HK and event files
temp2gain v4.3 'ft980620_0532.1400' is successfully opened Data Start Time is 172474371.97 (19980620 053247) Time Margin 2.0 sec included Sync error detected in 5095 th SF 'ft980620_0532.1400' EOF detected, sf=6658 Data End Time is 172504839.87 (19980620 140035) Gain History is written in ft980620_0532_1400.ghf-> Stdout output from ISAS program temp2gain
leapsec FITS data was successfully read-> Checking if column CAL_START in ft980620_0532_1400.ghf[1] is in order
Time column is TIME ORDERED-> Checking if column CAL_STOP in ft980620_0532_1400.ghf[1] is in order
Time column is TIME ORDERED-> Calculating attitude correction from ft980620_0532_1400CMHK.fits
The sum of the selected column is 15090.000 The mean of the selected column is 99.276316 The standard deviation of the selected column is 1.5871895 The minimum of selected column is 96.000000 The maximum of selected column is 102.00000 The number of points used in calculation is 152-> Standard Output From FTOOL fstatistic:
The sum of the selected column is 15090.000 The mean of the selected column is 99.276316 The standard deviation of the selected column is 1.5871895 The minimum of selected column is 96.000000 The maximum of selected column is 102.00000 The number of points used in calculation is 152
ASCALIN_V0.9u(mod)-> Checking if ad86032020g200270m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020g200370l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020g300170h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020g300270m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020g300370l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000101h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000102h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000112h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000201m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000202m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000212m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000301l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000302l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s000312l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100101h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100102h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100112h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100201m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100202m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100212m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100301l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100302l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad86032020s100312l.unf is covered by attitude file
ASCALIN_V0.9u(mod)
S0-HK file: ft980620_0532_1400S0HK.fits S1-HK file: ft980620_0532_1400S1HK.fits G2-HK file: ft980620_0532_1400G2HK.fits G3-HK file: ft980620_0532_1400G3HK.fits Date and time are: 1998-06-20 05:32:05 mjd=50984.230625 Orbit file name is ./frf.orbit.241 Epoch of Orbital Elements: 1998-06-15 12:00:00 Rigidity Data File: ./rigidity.data.1.23 Attitude FRF: fa980620_0532.1400 output FITS File: ft980620_0532_1400.mkf mkfilter2: Warning, faQparam error: time= 1.724742779676e+08 outside range of attitude file Euler angles undefined for this bin mkfilter2: Warning, faQparam error: time= 1.724743099676e+08 outside range of attitude file Euler angles undefined for this bin Total 956 Data bins were processed.-> Checking if column TIME in ft980620_0532_1400.mkf is in order
Time column is TIME ORDERED-> Calculating dead time values for filter file
The sum of the selected column is 4583.0576 The mean of the selected column is 16.849476 The standard deviation of the selected column is 6.9274590 The minimum of selected column is 3.7500122 The maximum of selected column is 63.031445 The number of points used in calculation is 272-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<37.6 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad86032020s000112h.unf into ad86032020s000112h.evt
The sum of the selected column is 4583.0576 The mean of the selected column is 16.849476 The standard deviation of the selected column is 6.9274590 The minimum of selected column is 3.7500122 The maximum of selected column is 63.031445 The number of points used in calculation is 272-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<37.6 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad86032020s000201m.unf because of mode
The sum of the selected column is 2157.1005 The mean of the selected column is 16.985044 The standard deviation of the selected column is 7.5730996 The minimum of selected column is 5.9375186 The maximum of selected column is 71.562721 The number of points used in calculation is 127-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<39.7 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad86032020s000212m.unf into ad86032020s000212m.evt
The sum of the selected column is 2157.1005 The mean of the selected column is 16.985044 The standard deviation of the selected column is 7.5730996 The minimum of selected column is 5.9375186 The maximum of selected column is 71.562721 The number of points used in calculation is 127-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0 && S0_PIXL1<39.7 ) ) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad86032020s000301l.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0) )&&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad86032020s000302l.evt since it contains 0 events
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL1>0) )&&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&( (S0_SATF1<1) ||(S0_SATF1>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad86032020s000312l.evt since it contains 0 events
The sum of the selected column is 7486.2065 The mean of the selected column is 27.624378 The standard deviation of the selected column is 10.618045 The minimum of selected column is 5.8700185 The maximum of selected column is 68.125221 The number of points used in calculation is 271-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>0 && S1_PIXL3<59.4 ) ) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad86032020s100112h.unf into ad86032020s100112h.evt
The sum of the selected column is 7486.2065 The mean of the selected column is 27.624378 The standard deviation of the selected column is 10.618045 The minimum of selected column is 5.8700185 The maximum of selected column is 68.125221 The number of points used in calculation is 271-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>0 && S1_PIXL3<59.4 ) ) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad86032020s100201m.unf because of mode
The sum of the selected column is 2621.2895 The mean of the selected column is 25.449413 The standard deviation of the selected column is 7.8083926 The minimum of selected column is 9.3750286 The maximum of selected column is 52.218910 The number of points used in calculation is 103-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>2 && S1_PIXL3<48.8 ) ) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Filtering ad86032020s100212m.unf into ad86032020s100212m.evt
The sum of the selected column is 2621.2895 The mean of the selected column is 25.449413 The standard deviation of the selected column is 7.8083926 The minimum of selected column is 9.3750286 The maximum of selected column is 52.218910 The number of points used in calculation is 103-> Using the following selection criteria:
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>2 && S1_PIXL3<48.8 ) ) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Skipping ad86032020s100301l.unf because of mode
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>0) )&&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad86032020s100302l.evt since it contains 0 events
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S1_PIXL3>0) )&&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&( (S1_SATF3<1) ||(S1_SATF3>1)) &&((T_DY_NT<0)||(T_DY_NT>16)) &&((T_SAA <0)||(T_SAA >16))-> Deleting ad86032020s100312l.evt since it contains 0 events
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Filtering ad86032020g200270m.unf into ad86032020g200270m.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Filtering ad86032020g200370l.unf into ad86032020g200370l.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G2_L1>0)-> Deleting ad86032020g200370l.evt since it contains 0 events
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)-> Filtering ad86032020g300270m.unf into ad86032020g300270m.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)-> Filtering ad86032020g300370l.unf into ad86032020g300370l.evt
(SAA==0)&& (COR>4)&& (G2_H0+G2_H2+G3_H0+G3_H2<45)&& (G2_H0+G2_H2+G3_H0+G3_H2<0.45*COR**2-13*COR+125)&& (RBM_CONT<100)&& (ELV>5)&& (ACS==0)&& (ANG_DIST>0)&& (ANG_DIST<0.01)&& (G3_L1>0)-> Deleting ad86032020g300370l.evt since it contains 0 events
-ANNULUS(128.5,128.5,192,88) -ELLIPSE(167.5,220,24.66,28.95,245.298)-> gis2_ano_on_flf_180295.fits already present in current directory
ASCAEXPO_V0.9b reading data file: ad86032020g200170h.evt reading gti ext: STDGTI reading cal file: gis2_ano_on_flf_180295.fits reading inst file: GIS2_REGION256.4_regionmap.tmp making an inst map... rebin gis: 1 multiply inst map... reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3808 Mean RA/DEC/ROLL : 188.0067 8.1453 52.3808 Pnt RA/DEC/ROLL : 187.9651 8.1197 52.3808 Image rebin factor : 1 Attitude Records : 26714 GTI intervals : 17 Total GTI (secs) : 9721.955 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 1154.00 1154.00 20 Percent Complete: Total/live time: 2624.02 2624.02 30 Percent Complete: Total/live time: 3903.98 3903.98 40 Percent Complete: Total/live time: 4163.48 4163.48 50 Percent Complete: Total/live time: 5212.98 5212.98 60 Percent Complete: Total/live time: 7120.96 7120.96 70 Percent Complete: Total/live time: 7120.96 7120.96 80 Percent Complete: Total/live time: 8001.96 8001.96 90 Percent Complete: Total/live time: 9168.46 9168.46 100 Percent Complete: Total/live time: 9721.96 9721.96 Number of attitude steps used: 37 Number of attitude steps avail: 20901 Mean RA/DEC pixel offset: -11.0400 -3.6144 writing expo file: ad86032020g200170h.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020g200170h.evt
ASCAEXPO_V0.9b reading data file: ad86032020g200270m.evt reading gti ext: STDGTI reading cal file: gis2_ano_on_flf_180295.fits reading inst file: GIS2_REGION256.4_regionmap.tmp making an inst map... rebin gis: 1 multiply inst map... reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3803 Mean RA/DEC/ROLL : 188.0061 8.1545 52.3803 Pnt RA/DEC/ROLL : 187.9746 8.0982 52.3803 Image rebin factor : 1 Attitude Records : 26714 GTI intervals : 7 Total GTI (secs) : 5136.128 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 1039.96 1039.96 20 Percent Complete: Total/live time: 1491.96 1491.96 30 Percent Complete: Total/live time: 1867.96 1867.96 40 Percent Complete: Total/live time: 2240.03 2240.03 50 Percent Complete: Total/live time: 3631.95 3631.95 60 Percent Complete: Total/live time: 3631.95 3631.95 70 Percent Complete: Total/live time: 3936.03 3936.03 80 Percent Complete: Total/live time: 5129.21 5129.21 90 Percent Complete: Total/live time: 5129.21 5129.21 100 Percent Complete: Total/live time: 5136.13 5136.13 Number of attitude steps used: 22 Number of attitude steps avail: 3029 Mean RA/DEC pixel offset: 10.3525 1.0507 writing expo file: ad86032020g200270m.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020g200270m.evt
-ANNULUS(128.5,128.5,192,88) -ELLIPSE(217,95,21.56,25.92,169.216)-> gis3_ano_on_flf_180295.fits already present in current directory
ASCAEXPO_V0.9b reading data file: ad86032020g300170h.evt reading gti ext: STDGTI reading cal file: gis3_ano_on_flf_180295.fits reading inst file: GIS3_REGION256.4_regionmap.tmp making an inst map... rebin gis: 1 multiply inst map... reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3784 Mean RA/DEC/ROLL : 187.9895 8.1273 52.3784 Pnt RA/DEC/ROLL : 187.9823 8.1378 52.3784 Image rebin factor : 1 Attitude Records : 26714 GTI intervals : 17 Total GTI (secs) : 9721.955 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 1154.00 1154.00 20 Percent Complete: Total/live time: 2624.02 2624.02 30 Percent Complete: Total/live time: 3903.98 3903.98 40 Percent Complete: Total/live time: 4163.48 4163.48 50 Percent Complete: Total/live time: 5212.98 5212.98 60 Percent Complete: Total/live time: 7120.96 7120.96 70 Percent Complete: Total/live time: 7120.96 7120.96 80 Percent Complete: Total/live time: 8001.96 8001.96 90 Percent Complete: Total/live time: 9168.46 9168.46 100 Percent Complete: Total/live time: 9721.96 9721.96 Number of attitude steps used: 37 Number of attitude steps avail: 20901 Mean RA/DEC pixel offset: 0.7122 -2.4470 writing expo file: ad86032020g300170h.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020g300170h.evt
ASCAEXPO_V0.9b reading data file: ad86032020g300270m.evt reading gti ext: STDGTI reading cal file: gis3_ano_on_flf_180295.fits reading inst file: GIS3_REGION256.4_regionmap.tmp making an inst map... rebin gis: 1 multiply inst map... reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3780 Mean RA/DEC/ROLL : 187.9887 8.1363 52.3780 Pnt RA/DEC/ROLL : 187.9918 8.1163 52.3780 Image rebin factor : 1 Attitude Records : 26714 GTI intervals : 7 Total GTI (secs) : 5136.128 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 1039.96 1039.96 20 Percent Complete: Total/live time: 1491.96 1491.96 30 Percent Complete: Total/live time: 1867.96 1867.96 40 Percent Complete: Total/live time: 2240.03 2240.03 50 Percent Complete: Total/live time: 3631.95 3631.95 60 Percent Complete: Total/live time: 3631.95 3631.95 70 Percent Complete: Total/live time: 3936.03 3936.03 80 Percent Complete: Total/live time: 5129.21 5129.21 90 Percent Complete: Total/live time: 5129.21 5129.21 100 Percent Complete: Total/live time: 5136.13 5136.13 Number of attitude steps used: 22 Number of attitude steps avail: 3029 Mean RA/DEC pixel offset: 22.4311 2.2506 writing expo file: ad86032020g300270m.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020g300270m.evt
ASCAEXPO_V0.9b reading data file: ad86032020s000102h.evt reading gti ext: STDGTI reading hp ext: HOT_PIXELS reading cal file: s0_teldef_ascalin.fits making an inst map... SIS AREA DISC ENABL OFF CHIP: 0 1 2 3 CCD POWER ON/OFF: OFF ON OFF OFF AREA DISC IN/OUT: OUT OUT IN IN AREA DISC H START: 6 6 6 316 AREA DISC H STOP: 425 425 200 425 AREA DISC V START: 2 2 2 2 AREA DISC V STOP: 422 422 150 112 reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3813 Mean RA/DEC/ROLL : 188.0101 8.1271 52.3813 Pnt RA/DEC/ROLL : 187.9623 8.1386 52.3813 Image rebin factor : 4 Attitude Records : 26714 Hot Pixels : 11 GTI intervals : 20 Total GTI (secs) : 8859.408 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 976.12 976.12 20 Percent Complete: Total/live time: 2078.62 2078.62 30 Percent Complete: Total/live time: 3552.11 3552.11 40 Percent Complete: Total/live time: 3811.60 3811.60 50 Percent Complete: Total/live time: 4830.93 4830.93 60 Percent Complete: Total/live time: 5427.98 5427.98 70 Percent Complete: Total/live time: 6354.92 6354.92 80 Percent Complete: Total/live time: 7195.41 7195.41 90 Percent Complete: Total/live time: 8346.03 8346.03 100 Percent Complete: Total/live time: 8859.41 8859.41 Number of attitude steps used: 40 Number of attitude steps avail: 19650 Mean RA/DEC pixel offset: -47.4052 -95.7338 writing expo file: ad86032020s000102h.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020s000102h.evt
ASCAEXPO_V0.9b reading data file: ad86032020s000202m.evt reading gti ext: STDGTI reading hp ext: HOT_PIXELS reading cal file: s0_teldef_ascalin.fits making an inst map... SIS AREA DISC ENABL OFF CHIP: 0 1 2 3 CCD POWER ON/OFF: OFF ON OFF OFF AREA DISC IN/OUT: OUT OUT IN IN AREA DISC H START: 6 6 6 316 AREA DISC H STOP: 425 425 200 425 AREA DISC V START: 2 2 2 2 AREA DISC V STOP: 422 422 150 112 reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3808 Mean RA/DEC/ROLL : 188.0100 8.1353 52.3808 Pnt RA/DEC/ROLL : 187.9710 8.1167 52.3808 Image rebin factor : 4 Attitude Records : 26714 Hot Pixels : 10 GTI intervals : 16 Total GTI (secs) : 4039.687 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 751.71 751.71 20 Percent Complete: Total/live time: 1307.84 1307.84 30 Percent Complete: Total/live time: 1307.84 1307.84 40 Percent Complete: Total/live time: 1683.84 1683.84 50 Percent Complete: Total/live time: 2927.70 2927.70 60 Percent Complete: Total/live time: 2927.70 2927.70 70 Percent Complete: Total/live time: 2927.82 2927.82 80 Percent Complete: Total/live time: 4032.99 4032.99 90 Percent Complete: Total/live time: 4032.99 4032.99 100 Percent Complete: Total/live time: 4039.69 4039.69 Number of attitude steps used: 22 Number of attitude steps avail: 2883 Mean RA/DEC pixel offset: 151.7119 -53.8166 writing expo file: ad86032020s000202m.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020s000202m.evt
ASCAEXPO_V0.9b reading data file: ad86032020s100102h.evt reading gti ext: STDGTI reading hp ext: HOT_PIXELS reading cal file: s1_teldef_ascalin.fits making an inst map... SIS AREA DISC ENABL OFF CHIP: 0 1 2 3 CCD POWER ON/OFF: OFF OFF OFF ON AREA DISC IN/OUT: OUT OUT OUT OUT AREA DISC H START: 6 6 6 6 AREA DISC H STOP: 425 425 425 425 AREA DISC V START: 2 2 2 2 AREA DISC V STOP: 422 422 422 422 reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3796 Mean RA/DEC/ROLL : 187.9980 8.1376 52.3796 Pnt RA/DEC/ROLL : 187.9744 8.1281 52.3796 Image rebin factor : 4 Attitude Records : 26714 Hot Pixels : 27 GTI intervals : 22 Total GTI (secs) : 8847.597 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 977.62 977.62 20 Percent Complete: Total/live time: 2046.62 2046.62 30 Percent Complete: Total/live time: 3516.11 3516.11 40 Percent Complete: Total/live time: 3775.60 3775.60 50 Percent Complete: Total/live time: 4758.93 4758.93 60 Percent Complete: Total/live time: 6346.92 6346.92 70 Percent Complete: Total/live time: 6346.92 6346.92 80 Percent Complete: Total/live time: 7252.23 7252.23 90 Percent Complete: Total/live time: 8302.22 8302.22 100 Percent Complete: Total/live time: 8847.60 8847.60 Number of attitude steps used: 40 Number of attitude steps avail: 19650 Mean RA/DEC pixel offset: -51.7384 -25.6790 writing expo file: ad86032020s100102h.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020s100102h.evt
ASCAEXPO_V0.9b reading data file: ad86032020s100202m.evt reading gti ext: STDGTI reading hp ext: HOT_PIXELS reading cal file: s1_teldef_ascalin.fits making an inst map... SIS AREA DISC ENABL OFF CHIP: 0 1 2 3 CCD POWER ON/OFF: OFF OFF OFF ON AREA DISC IN/OUT: OUT OUT OUT OUT AREA DISC H START: 6 6 6 6 AREA DISC H STOP: 425 425 425 425 AREA DISC V START: 2 2 2 2 AREA DISC V STOP: 422 422 422 422 reading att file: ./fa980620_0532.1400 making an exposure map... Aspect RA/DEC/ROLL : 187.9860 8.1320 52.3791 Mean RA/DEC/ROLL : 187.9977 8.1460 52.3791 Pnt RA/DEC/ROLL : 187.9831 8.1062 52.3791 Image rebin factor : 4 Attitude Records : 26714 Hot Pixels : 26 GTI intervals : 29 Total GTI (secs) : 3271.909 Max attitude excursion (arcsecs) : 5.000 0 Percent Complete: Total/live time: 0.00 0.00 10 Percent Complete: Total/live time: 655.71 655.71 20 Percent Complete: Total/live time: 1115.84 1115.84 30 Percent Complete: Total/live time: 1115.84 1115.84 40 Percent Complete: Total/live time: 1363.84 1363.84 50 Percent Complete: Total/live time: 2351.70 2351.70 60 Percent Complete: Total/live time: 2351.70 2351.70 70 Percent Complete: Total/live time: 2351.82 2351.82 80 Percent Complete: Total/live time: 3271.91 3271.91 90 Percent Complete: Total/live time: 3271.91 3271.91 100 Percent Complete: Total/live time: 3271.91 3271.91 Number of attitude steps used: 16 Number of attitude steps avail: 2877 Mean RA/DEC pixel offset: 152.8714 20.0003 writing expo file: ad86032020s100202m.expo closing attitude file... closing data file...-> Generating low and high energy images for ad86032020s100202m.evt
ad86032020s000102h.expo ad86032020s000202m.expo ad86032020s100102h.expo ad86032020s100202m.expo-> Summing the following images to produce ad86032020sis32002_all.totsky
ad86032020s000102h.img ad86032020s000202m.img ad86032020s100102h.img ad86032020s100202m.img-> Summing the following images to produce ad86032020sis32002_lo.totsky
ad86032020s000102h_lo.img ad86032020s000202m_lo.img ad86032020s100102h_lo.img ad86032020s100202m_lo.img-> Summing the following images to produce ad86032020sis32002_hi.totsky
ad86032020s000102h_hi.img ad86032020s000202m_hi.img ad86032020s100102h_hi.img ad86032020s100202m_hi.img-> Running XIMAGE to create ad86032020sis32002.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad86032020sis32002_all.totsky Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 3.00000 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 3 min: 0 ![2]XIMAGE> read/exp_map ad86032020sis32002.totexpo Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 416.977 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 416 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "VIRGO_SOUTH_N17" ![7]XIMAGE> title/lower "ASCA SIS0,SIS1 June 20, 1998 Exposure: 25018.5 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 25089 ![9]XIMAGE> grid ![10]XIMAGE> scale scal_f, min_inten 1.00000 0. i,inten,mm,pp 1 0. 0 0 i,inten,mm,pp 2 4.00000 40 -1 i,inten,mm,pp 3 8.00000 80 -1 i,inten,mm,pp 4 19.0000 19 0 ![11]XIMAGE> exit-> Summing gis images
ad86032020g200170h.expo ad86032020g200270m.expo ad86032020g300170h.expo ad86032020g300270m.expo-> Summing the following images to produce ad86032020gis25670_all.totsky
ad86032020g200170h.img ad86032020g200270m.img ad86032020g300170h.img ad86032020g300270m.img-> Summing the following images to produce ad86032020gis25670_lo.totsky
ad86032020g200170h_lo.img ad86032020g200270m_lo.img ad86032020g300170h_lo.img ad86032020g300270m_lo.img-> Summing the following images to produce ad86032020gis25670_hi.totsky
ad86032020g200170h_hi.img ad86032020g200270m_hi.img ad86032020g300170h_hi.img ad86032020g300270m_hi.img-> Running XIMAGE to create ad86032020gis25670.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad86032020gis25670_all.totsky Reading an image Telescope ASCA GIS2 Image display size = 256 Done, closing file Largest, Smallest 5.00000 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 5 min: 0 ![2]XIMAGE> read/exp_map ad86032020gis25670.totexpo Reading an image Telescope ASCA GIS2 Image display size = 256 Done, closing file Largest, Smallest 495.269 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 495 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "VIRGO_SOUTH_N17" ![7]XIMAGE> title/lower "ASCA GIS2,GIS3 June 20, 1998 Exposure: 29716.1 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 32767 ![9]XIMAGE> grid ![10]XIMAGE> scale scal_f, min_inten 1.00000 0. i,inten,mm,pp 1 0. 0 0 i,inten,mm,pp 2 4.00000 40 -1 i,inten,mm,pp 3 8.00000 80 -1 i,inten,mm,pp 4 59.0000 59 0 ![11]XIMAGE> exit
-> Standard Output From STOOL colorpic:
color plane 0 color plane 1 color plane 2 writing image image written-> Creating fits catalog of sources: ad86032020gis25670.src
-> Standard Output From STOOL colorpic:
color plane 0 color plane 1 color plane 2 writing image image written-> Creating fits catalog of sources: ad86032020sis32002.src
1 ad86032020s000102h.evt 721 1 ad86032020s000202m.evt 721-> Fetching SIS0_NOTCHIP0.1
ad86032020s000102h.evt ad86032020s000202m.evt-> Grouping ad86032020s010102_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS0 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 12899. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10462 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 512 No. of legal detector channels NCHAN - 512 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 16 of undefined grouping (Channel quality=bad) ... 17 - 22 are grouped by a factor 6 ... 23 - 29 are grouped by a factor 7 ... 30 - 37 are grouped by a factor 4 ... 38 - 52 are grouped by a factor 5 ... 53 - 59 are grouped by a factor 7 ... 60 - 72 are grouped by a factor 13 ... 73 - 95 are grouped by a factor 23 ... 96 - 126 are grouped by a factor 31 ... 127 - 177 are grouped by a factor 51 ... 178 - 254 are grouped by a factor 77 ... 255 - 327 are grouped by a factor 73 ... 328 - 511 are grouped by a factor 184 ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020s010102_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 1
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x512 S0C1 Bright PI RMF Calibration data files: ecd = ./sis0c1p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad86032020s010102_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 53 by 53 bins expanded to 53 by 53 bins First WMAP bin is at detector pixel 232 216 8 detector pixels per WMAP bin WMAP bin size is 0.21600 mm 0.21216 arcmin Selected region size is 7.5346 arcmin^2 Optical axis is detector pixel 662.72 559.02 1180 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 6.97000E+02 Weighted mean angle from optical axis = 7.418 arcmin-> Standard Output From STOOL group_event_files:
1 ad86032020s000112h.evt 756 1 ad86032020s000212m.evt 756-> SIS0_NOTCHIP0.1 already present in current directory
ad86032020s000112h.evt ad86032020s000212m.evt-> Grouping ad86032020s010212_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS0 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 12899. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10462 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 1024 No. of legal detector channels NCHAN - 1024 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 31 of undefined grouping (Channel quality=bad) ... 32 - 43 are grouped by a factor 12 ... 44 - 56 are grouped by a factor 13 ... 57 - 65 are grouped by a factor 9 ... 66 - 73 are grouped by a factor 8 ... 74 - 82 are grouped by a factor 9 ... 83 - 104 are grouped by a factor 11 ... 105 - 116 are grouped by a factor 12 ... 117 - 142 are grouped by a factor 26 ... 143 - 179 are grouped by a factor 37 ... 180 - 244 are grouped by a factor 65 ... 245 - 329 are grouped by a factor 85 ... 330 - 487 are grouped by a factor 158 ... 488 - 575 are grouped by a factor 88 ... 576 - 866 are grouped by a factor 291 ... 867 - 1023 are grouped by a factor 157 ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020s010212_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 1
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x1024 S0C1 Bright2 PI RMF Calibration data files: ecd = ./sis0c1p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad86032020s010212_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 53 by 52 bins expanded to 53 by 52 bins First WMAP bin is at detector pixel 232 216 8 detector pixels per WMAP bin WMAP bin size is 0.21600 mm 0.21216 arcmin Selected region size is 7.5346 arcmin^2 Optical axis is detector pixel 662.72 559.02 1180 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 7.31000E+02 Weighted mean angle from optical axis = 7.435 arcmin-> Standard Output From STOOL group_event_files:
1 ad86032020s100102h.evt 639 1 ad86032020s100202m.evt 639-> Fetching SIS1_NOTCHIP0.1
ad86032020s100102h.evt ad86032020s100202m.evt-> Grouping ad86032020s110102_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS1 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 12120. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10462 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 512 No. of legal detector channels NCHAN - 512 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 16 of undefined grouping (Channel quality=bad) ... 17 - 25 are grouped by a factor 9 ... 26 - 43 are grouped by a factor 6 ... 44 - 50 are grouped by a factor 7 ... 51 - 58 are grouped by a factor 8 ... 59 - 73 are grouped by a factor 15 ... 74 - 106 are grouped by a factor 33 ... 107 - 158 are grouped by a factor 52 ... 159 - 232 are grouped by a factor 74 ... 233 - 283 are grouped by a factor 51 ... 284 - 453 are grouped by a factor 170 ... 454 - 467 are grouped by a factor 14 ... 468 - 511 of undefined grouping (Channel quality=bad) ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020s110102_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 3
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x512 S1C3 Bright PI RMF Calibration data files: ecd = ./sis1c3p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad86032020s110102_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 53 by 53 bins expanded to 53 by 53 bins First WMAP bin is at detector pixel 232 216 8 detector pixels per WMAP bin WMAP bin size is 0.21600 mm 0.21216 arcmin Selected region size is 7.5346 arcmin^2 Optical axis is detector pixel 618.28 773.83 1180 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 6.10000E+02 Weighted mean angle from optical axis = 10.893 arcmin-> Standard Output From STOOL group_event_files:
1 ad86032020s100112h.evt 684 1 ad86032020s100212m.evt 684-> SIS1_NOTCHIP0.1 already present in current directory
ad86032020s100112h.evt ad86032020s100212m.evt-> Grouping ad86032020s110212_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - SIS1 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 12120. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.10462 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 1024 No. of legal detector channels NCHAN - 1024 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - FALSE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 32 of undefined grouping (Channel quality=bad) ... 33 - 49 are grouped by a factor 17 ... 50 - 62 are grouped by a factor 13 ... 63 - 73 are grouped by a factor 11 ... 74 - 83 are grouped by a factor 10 ... 84 - 96 are grouped by a factor 13 ... 97 - 110 are grouped by a factor 14 ... 111 - 133 are grouped by a factor 23 ... 134 - 170 are grouped by a factor 37 ... 171 - 268 are grouped by a factor 98 ... 269 - 370 are grouped by a factor 102 ... 371 - 514 are grouped by a factor 144 ... 515 - 736 are grouped by a factor 222 ... 737 - 905 are grouped by a factor 169 ... 906 - 930 are grouped by a factor 25 ... 931 - 1023 are grouped by a factor 93 ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020s110212_0.pi ** grppha 2.8.1 completed successfully-> Source occupies chip(s) 3
Sisrmg Version 1.1, Configured 04/97 This version resolves *all* known keyword incompatibilities with other FTOOLS tasks. If you have previously fudged *any* keywords in the PHA file to compensate, incorrect results will follow. Setting 1st PHA channel to 0 Making v1.1 1180x1024 S1C3 Bright2 PI RMF Calibration data files: ecd = ./sis1c3p40_290296.fits cti = ./sisph2pi_110397.fits echo = ./sisechos_290296.fits rdd = ./sisrddis_290296.fits Please stand by... ...Done.-> Generating ad86032020s110212_0.arf with point=no
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 53 by 53 bins expanded to 53 by 53 bins First WMAP bin is at detector pixel 232 216 8 detector pixels per WMAP bin WMAP bin size is 0.21600 mm 0.21216 arcmin Selected region size is 7.5346 arcmin^2 Optical axis is detector pixel 618.28 773.83 1180 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 6.56000E+02 Weighted mean angle from optical axis = 10.850 arcmin-> Standard Output From STOOL group_event_files:
1 ad86032020g200170h.evt 4756 1 ad86032020g200270m.evt 4756-> GIS2_REGION256.4 already present in current directory
ad86032020g200170h.evt ad86032020g200270m.evt-> Correcting ad86032020g210170_0.pi for dead time
... read all the files from deadlist.tmp-> Grouping ad86032020g210170_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - GIS2 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 14858. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.36888 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 1024 No. of legal detector channels NCHAN - 1024 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - TRUE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 21 are grouped by a factor 22 ... 22 - 27 are grouped by a factor 3 ... 28 - 31 are grouped by a factor 4 ... 32 - 41 are grouped by a factor 5 ... 42 - 47 are grouped by a factor 6 ... 48 - 57 are grouped by a factor 5 ... 58 - 61 are grouped by a factor 4 ... 62 - 66 are grouped by a factor 5 ... 67 - 81 are grouped by a factor 3 ... 82 - 83 are grouped by a factor 2 ... 84 - 86 are grouped by a factor 3 ... 87 - 90 are grouped by a factor 2 ... 91 - 93 are grouped by a factor 3 ... 94 - 95 are grouped by a factor 2 ... 96 - 98 are grouped by a factor 3 ... 99 - 110 are grouped by a factor 2 ... 111 - 113 are grouped by a factor 3 ... 114 - 115 are grouped by a factor 2 ... 116 - 118 are grouped by a factor 3 ... 119 - 120 are grouped by a factor 2 ... 121 - 129 are grouped by a factor 3 ... 130 - 131 are grouped by a factor 2 ... 132 - 137 are grouped by a factor 3 ... 138 - 139 are grouped by a factor 2 ... 140 - 142 are grouped by a factor 3 ... 143 - 144 are grouped by a factor 2 ... 145 - 147 are grouped by a factor 3 ... 148 - 151 are grouped by a factor 4 ... 152 - 154 are grouped by a factor 3 ... 155 - 158 are grouped by a factor 4 ... 159 - 161 are grouped by a factor 3 ... 162 - 169 are grouped by a factor 4 ... 170 - 175 are grouped by a factor 3 ... 176 - 183 are grouped by a factor 4 ... 184 - 189 are grouped by a factor 6 ... 190 - 193 are grouped by a factor 4 ... 194 - 199 are grouped by a factor 6 ... 200 - 204 are grouped by a factor 5 ... 205 - 210 are grouped by a factor 6 ... 211 - 217 are grouped by a factor 7 ... 218 - 229 are grouped by a factor 6 ... 230 - 236 are grouped by a factor 7 ... 237 - 252 are grouped by a factor 8 ... 253 - 261 are grouped by a factor 9 ... 262 - 269 are grouped by a factor 8 ... 270 - 276 are grouped by a factor 7 ... 277 - 294 are grouped by a factor 9 ... 295 - 305 are grouped by a factor 11 ... 306 - 345 are grouped by a factor 10 ... 346 - 354 are grouped by a factor 9 ... 355 - 378 are grouped by a factor 12 ... 379 - 386 are grouped by a factor 8 ... 387 - 398 are grouped by a factor 12 ... 399 - 408 are grouped by a factor 10 ... 409 - 422 are grouped by a factor 14 ... 423 - 438 are grouped by a factor 16 ... 439 - 474 are grouped by a factor 18 ... 475 - 486 are grouped by a factor 12 ... 487 - 516 are grouped by a factor 15 ... 517 - 534 are grouped by a factor 18 ... 535 - 584 are grouped by a factor 25 ... 585 - 610 are grouped by a factor 26 ... 611 - 634 are grouped by a factor 24 ... 635 - 659 are grouped by a factor 25 ... 660 - 681 are grouped by a factor 22 ... 682 - 706 are grouped by a factor 25 ... 707 - 766 are grouped by a factor 30 ... 767 - 811 are grouped by a factor 45 ... 812 - 893 are grouped by a factor 41 ... 894 - 933 are grouped by a factor 40 ... 934 - 984 are grouped by a factor 51 ... 985 - 1023 are grouped by a factor 39 ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020g210170_0.pi ** grppha 2.8.1 completed successfully-> Fetching gis2v4_0.rmf
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 177 by 178 bins expanded to 256 by 256 bins First WMAP bin is at detector pixel 1 1 1 detector pixels per WMAP bin WMAP bin size is 0.25000 mm 0.24555 arcmin Selected region size is 1458.0 arcmin^2 Optical axis is detector pixel 133.00 130.96 201 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 4.75600E+03 Weighted mean angle from optical axis = 13.947 arcmin-> Standard Output From STOOL group_event_files:
1 ad86032020g300170h.evt 4945 1 ad86032020g300270m.evt 4945-> GIS3_REGION256.4 already present in current directory
ad86032020g300170h.evt ad86032020g300270m.evt-> Correcting ad86032020g310170_0.pi for dead time
... read all the files from deadlist.tmp-> Grouping ad86032020g310170_0.pi to 40 counts/bin
------------------------- MANDATORY KEYWORDS/VALUES ------------------------- -------------------------------------------------------------------- -------------------------------------------------------------------- EXTNAME - SPECTRUM Name of this BINTABLE TELESCOP - ASCA Mission/Satellite name INSTRUME - GIS3 Instrument/Detector FILTER - NONE Instrument filter in use EXPOSURE - 14858. Integration time (in secs) of PHA data AREASCAL - 1.0000 Area scaling factor BACKSCAL - 0.36783 Background scaling factor BACKFILE - NONE Associated background file CORRSCAL - 1.0000 Correlation scaling factor CORRFILE - none Associated correlation file RESPFILE - NONE Associated redistribution matrix file ANCRFILE - none Associated ancillary response file XFLT0001 - none XSPEC selection filter POISSERR - TRUE Whether Poissonian errors apply CHANTYPE - PI Whether channels have been corrected TLMIN1 - 0 First legal Detector channel DETCHANS - 1024 No. of legal detector channels NCHAN - 1024 No. of detector channels in dataset PHAVERSN - 1.1.0 OGIP FITS version number STAT_ERR - FALSE Statistical Error SYS_ERR - TRUE Fractional Systematic Error QUALITY - TRUE Quality Flag GROUPING - TRUE Grouping Flag -------------------------------------------------------------------- -------------------------------------------------------------------- ... ... -------- ... GROUPING ... -------- ... --------------------------------------------- ... Channel Grouping (Channel-Channel) : ... 0 - 22 are grouped by a factor 23 ... 23 - 34 are grouped by a factor 3 ... 35 - 38 are grouped by a factor 4 ... 39 - 44 are grouped by a factor 6 ... 45 - 48 are grouped by a factor 4 ... 49 - 55 are grouped by a factor 7 ... 56 - 67 are grouped by a factor 4 ... 68 - 76 are grouped by a factor 3 ... 77 - 84 are grouped by a factor 2 ... 85 - 93 are grouped by a factor 3 ... 94 - 103 are grouped by a factor 2 ... 104 - 112 are grouped by a factor 3 ... 113 - 114 are grouped by a factor 2 ... 115 - 117 are grouped by a factor 3 ... 118 - 119 are grouped by a factor 2 ... 120 - 122 are grouped by a factor 3 ... 123 - 126 are grouped by a factor 2 ... 127 - 132 are grouped by a factor 3 ... 133 - 134 are grouped by a factor 2 ... 135 - 137 are grouped by a factor 3 ... 138 - 139 are grouped by a factor 2 ... 140 - 145 are grouped by a factor 3 ... 146 - 147 are grouped by a factor 2 ... 148 - 150 are grouped by a factor 3 ... 151 - 152 are grouped by a factor 2 ... 153 - 156 are grouped by a factor 4 ... 157 - 159 are grouped by a factor 3 ... 160 - 163 are grouped by a factor 4 ... 164 - 166 are grouped by a factor 3 ... 167 - 174 are grouped by a factor 4 ... 175 - 177 are grouped by a factor 3 ... 178 - 185 are grouped by a factor 4 ... 186 - 205 are grouped by a factor 5 ... 206 - 229 are grouped by a factor 6 ... 230 - 236 are grouped by a factor 7 ... 237 - 245 are grouped by a factor 9 ... 246 - 252 are grouped by a factor 7 ... 253 - 262 are grouped by a factor 5 ... 263 - 269 are grouped by a factor 7 ... 270 - 278 are grouped by a factor 9 ... 279 - 290 are grouped by a factor 6 ... 291 - 297 are grouped by a factor 7 ... 298 - 305 are grouped by a factor 8 ... 306 - 315 are grouped by a factor 10 ... 316 - 327 are grouped by a factor 12 ... 328 - 337 are grouped by a factor 10 ... 338 - 349 are grouped by a factor 12 ... 350 - 358 are grouped by a factor 9 ... 359 - 368 are grouped by a factor 10 ... 369 - 376 are grouped by a factor 8 ... 377 - 385 are grouped by a factor 9 ... 386 - 396 are grouped by a factor 11 ... 397 - 414 are grouped by a factor 9 ... 415 - 428 are grouped by a factor 14 ... 429 - 441 are grouped by a factor 13 ... 442 - 452 are grouped by a factor 11 ... 453 - 472 are grouped by a factor 20 ... 473 - 489 are grouped by a factor 17 ... 490 - 505 are grouped by a factor 16 ... 506 - 545 are grouped by a factor 20 ... 546 - 567 are grouped by a factor 22 ... 568 - 590 are grouped by a factor 23 ... 591 - 610 are grouped by a factor 20 ... 611 - 635 are grouped by a factor 25 ... 636 - 673 are grouped by a factor 19 ... 674 - 693 are grouped by a factor 20 ... 694 - 710 are grouped by a factor 17 ... 711 - 734 are grouped by a factor 24 ... 735 - 766 are grouped by a factor 32 ... 767 - 808 are grouped by a factor 42 ... 809 - 849 are grouped by a factor 41 ... 850 - 897 are grouped by a factor 48 ... 898 - 924 are grouped by a factor 27 ... 925 - 963 are grouped by a factor 39 ... 964 - 1015 are grouped by a factor 52 ... 1016 - 1023 of undefined grouping (Channel quality=bad) ... --------------------------------------------- ... ...... exiting, changes written to file : ad86032020g310170_0.pi ** grppha 2.8.1 completed successfully-> Fetching gis3v4_0.rmf
ASCAARF vers 2.81 28 Aug 1998. Input WMAP array has size 177 by 178 bins expanded to 256 by 256 bins First WMAP bin is at detector pixel 1 1 1 detector pixels per WMAP bin WMAP bin size is 0.25000 mm 0.24555 arcmin Selected region size is 1453.8 arcmin^2 Optical axis is detector pixel 119.36 134.44 201 energies from RMF file Effective area fudge applied Arf filter applied Total counts in region = 4.94500E+03 Weighted mean angle from optical axis = 14.015 arcmin-> Plotting ad86032020g210170_0_pi.ps from ad86032020g210170_0.pi
XSPEC 9.01 01:55:15 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020g210170_0.pi Net count rate (cts/s) for file 1 0.3201 +/- 4.6415E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Plotting ad86032020g310170_0_pi.ps from ad86032020g310170_0.pi
XSPEC 9.01 01:55:27 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020g310170_0.pi Net count rate (cts/s) for file 1 0.3328 +/- 4.7347E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Plotting ad86032020s010102_0_pi.ps from ad86032020s010102_0.pi
XSPEC 9.01 01:55:39 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020s010102_0.pi Net count rate (cts/s) for file 1 5.4267E-02+/- 2.0715E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Plotting ad86032020s010212_0_pi.ps from ad86032020s010212_0.pi
XSPEC 9.01 01:55:52 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020s010212_0.pi Net count rate (cts/s) for file 1 5.6748E-02+/- 2.1386E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Plotting ad86032020s110102_0_pi.ps from ad86032020s110102_0.pi
XSPEC 9.01 01:56:08 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020s110102_0.pi Net count rate (cts/s) for file 1 5.0992E-02+/- 2.1294E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Plotting ad86032020s110212_0_pi.ps from ad86032020s110212_0.pi
XSPEC 9.01 01:56:20 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> data ad86032020s110212_0.pi Net count rate (cts/s) for file 1 5.4788E-02+/- 2.1705E-03 1 data set is in use !XSPEC> setplot energy !XSPEC> ignore bad !XSPEC> iplot !PLT> log y on !PLT> rescale y !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit
Type "help" for information [1]xronos> Current User Interface is ; command driven [2]xronos> Enter up to 50 input filenames and options for series 1 (or rtn) Ser. A filename 1 +options[.rbf]=> ad86032020s000002_0.lc Selected FITS extensions: 1 - RATE TABLE; Source ............ VIRGO_SOUTH_N17 Start Time (d) .... 10984 06:29:09.968 FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10984 14:00:21.745 No. of Rows ....... 14 Bin Time (s) ...... 894.5 Right Ascension ... 1.8799E+02 Internal time sys.. Converted to TJD Declination ....... 8.1320E+00 Experiment ........ ASCA SIS0 Filter ............ NONE Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - No Selected Columns: 1 - Time; 2 - Y-axis; 3 - Y-error; File contains binned data. Ser. A filename 2 +options[.rbf]=> Enter up to 50 input filenames and options for series 2 (or rtn) Ser. B filename 1 +options[.rbf]=> Enter up to 50 input filenames and options for series 3 (or rtn) Ser. C filename 1 +options[.rbf]=> [3]xronos> Maximum of 1 Intvs. with 31 Newbins of 894.528 (s) Intv 1 Start10984 7:36:15 Ser.1 Avg 0.5665E-01 Chisq 25.60 Var 0.1323E-03 Newbs. 14 Min 0.3962E-01 Max 0.7768E-01expVar 0.7239E-04 Bins 14 Results from Statistical Analysis Newbin Integration Time (s).. 894.53 Interval Duration (s)........ 22363. No. of Newbins .............. 14 Average (c/s) ............... 0.56651E-01 +/- 0.24E-02 Standard Deviation (c/s)..... 0.11504E-01 Minimum (c/s)................ 0.39619E-01 Maximum (c/s)................ 0.77679E-01 Variance ((c/s)**2).......... 0.13234E-03 +/- 0.52E-04 Expected Variance ((c/s)**2). 0.72386E-04 +/- 0.28E-04 Third Moment ((c/s)**3)...... 0.39505E-06 Average Deviation (c/s)...... 0.10167E-01 Skewness..................... 0.25948 +/- 0.65 Kurtosis..................... -1.1650 +/- 1.3 RMS fractional variation....< 0.13102 (3 sigma) Chi-Square................... 25.596 dof 13 Chi-Square Prob of constancy. 0.19257E-01 (0 means < 1.e-38) Kolm.-Smir. Prob of constancy 0.14614 (0 means < 1.e-38) [4]xronos> [5]xronos> Maximum of 1 Intvs. with 31 Newbins of 894.528 (s) Intv 1 Start10984 7:36:15 Ser.1 Avg 0.5665E-01 Chisq 25.60 Var 0.1323E-03 Newbs. 14 Min 0.3962E-01 Max 0.7768E-01expVar 0.7239E-04 Bins 14 Light curve ready ! Frme 1 Written to output file : xronos.qlc1 PLT> LA File ad86032020s000002_0.lc PLT> hard /ps PLT> [6]xronos>-> TIMEDEL=4.0000000000E+00 for ad86032020s100102h.evt
Type "help" for information [1]xronos> Current User Interface is ; command driven [2]xronos> Enter up to 50 input filenames and options for series 1 (or rtn) Ser. A filename 1 +options[.rbf]=> ad86032020s100002_0.lc Selected FITS extensions: 1 - RATE TABLE; Source ............ VIRGO_SOUTH_N17 Start Time (d) .... 10984 06:29:09.968 FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10984 13:59:49.968 No. of Rows ....... 14 Bin Time (s) ...... 948.3 Right Ascension ... 1.8799E+02 Internal time sys.. Converted to TJD Declination ....... 8.1320E+00 Experiment ........ ASCA SIS1 Filter ............ NONE Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - No Selected Columns: 1 - Time; 2 - Y-axis; 3 - Y-error; File contains binned data. Ser. A filename 2 +options[.rbf]=> Enter up to 50 input filenames and options for series 2 (or rtn) Ser. B filename 1 +options[.rbf]=> Enter up to 50 input filenames and options for series 3 (or rtn) Ser. C filename 1 +options[.rbf]=> [3]xronos> Maximum of 1 Intvs. with 29 Newbins of 948.318 (s) Intv 1 Start10984 7:40:17 Ser.1 Avg 0.5249E-01 Chisq 8.519 Var 0.4524E-04 Newbs. 14 Min 0.4049E-01 Max 0.6893E-01expVar 0.7435E-04 Bins 14 Results from Statistical Analysis Newbin Integration Time (s).. 948.32 Interval Duration (s)........ 18966. No. of Newbins .............. 14 Average (c/s) ............... 0.52489E-01 +/- 0.24E-02 Standard Deviation (c/s)..... 0.67260E-02 Minimum (c/s)................ 0.40494E-01 Maximum (c/s)................ 0.68930E-01 Variance ((c/s)**2).......... 0.45240E-04 +/- 0.18E-04 Expected Variance ((c/s)**2). 0.74345E-04 +/- 0.29E-04 Third Moment ((c/s)**3)...... 0.19557E-06 Average Deviation (c/s)...... 0.48995E-02 Skewness..................... 0.64273 +/- 0.65 Kurtosis..................... 0.64497 +/- 1.3 RMS fractional variation....< 0.23120 (3 sigma) Chi-Square................... 8.5191 dof 13 Chi-Square Prob of constancy. 0.80819 (0 means < 1.e-38) Kolm.-Smir. Prob of constancy 0.39180 (0 means < 1.e-38) [4]xronos> [5]xronos> Maximum of 1 Intvs. with 29 Newbins of 948.318 (s) Intv 1 Start10984 7:40:17 Ser.1 Avg 0.5249E-01 Chisq 8.519 Var 0.4524E-04 Newbs. 14 Min 0.4049E-01 Max 0.6893E-01expVar 0.7435E-04 Bins 14 Light curve ready ! Frme 1 Written to output file : xronos.qlc1 PLT> LA File ad86032020s100002_0.lc PLT> hard /ps PLT> [6]xronos>-> TIMEDEL=6.2500000000E-02 for ad86032020g200170h.evt
Type "help" for information [1]xronos> Current User Interface is ; command driven [2]xronos> Enter up to 50 input filenames and options for series 1 (or rtn) Ser. A filename 1 +options[.rbf]=> ad86032020g200070_0.lc Selected FITS extensions: 1 - RATE TABLE; Source ............ VIRGO_SOUTH_N17 Start Time (d) .... 10984 06:29:09.968 FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10984 14:00:21.968 No. of Rows ....... 97 Bin Time (s) ...... 156.2 Right Ascension ... 1.8799E+02 Internal time sys.. Converted to TJD Declination ....... 8.1320E+00 Experiment ........ ASCA GIS2 Filter ............ NONE Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - No Selected Columns: 1 - Time; 2 - Y-axis; 3 - Y-error; File contains binned data. Ser. A filename 2 +options[.rbf]=> Enter up to 50 input filenames and options for series 2 (or rtn) Ser. B filename 1 +options[.rbf]=> Enter up to 50 input filenames and options for series 3 (or rtn) Ser. C filename 1 +options[.rbf]=> [3]xronos> Maximum of 1 Intvs. with 174 Newbins of 156.204 (s) Intv 1 Start10984 6:30:28 Ser.1 Avg 0.3209 Chisq 85.65 Var 0.1926E-02 Newbs. 97 Min 0.2241 Max 0.4347 expVar 0.2181E-02 Bins 97 Results from Statistical Analysis Newbin Integration Time (s).. 156.20 Interval Duration (s)........ 26867. No. of Newbins .............. 97 Average (c/s) ............... 0.32095 +/- 0.48E-02 Standard Deviation (c/s)..... 0.43881E-01 Minimum (c/s)................ 0.22407 Maximum (c/s)................ 0.43468 Variance ((c/s)**2).......... 0.19255E-02 +/- 0.28E-03 Expected Variance ((c/s)**2). 0.21806E-02 +/- 0.31E-03 Third Moment ((c/s)**3)...... 0.30867E-04 Average Deviation (c/s)...... 0.35460E-01 Skewness..................... 0.36532 +/- 0.25 Kurtosis.....................-0.14754 +/- 0.50 RMS fractional variation....< 0.11321 (3 sigma) Chi-Square................... 85.654 dof 96 Chi-Square Prob of constancy. 0.76627 (0 means < 1.e-38) Kolm.-Smir. Prob of constancy 0.36290 (0 means < 1.e-38) [4]xronos> [5]xronos> Maximum of 1 Intvs. with 174 Newbins of 156.204 (s) Intv 1 Start10984 6:30:28 Ser.1 Avg 0.3209 Chisq 85.65 Var 0.1926E-02 Newbs. 97 Min 0.2241 Max 0.4347 expVar 0.2181E-02 Bins 97 Light curve ready ! Frme 1 Written to output file : xronos.qlc1 PLT> LA File ad86032020g200070_0.lc PLT> hard /ps PLT> [6]xronos>-> TIMEDEL=6.2500000000E-02 for ad86032020g300170h.evt
Type "help" for information [1]xronos> Current User Interface is ; command driven [2]xronos> Enter up to 50 input filenames and options for series 1 (or rtn) Ser. A filename 1 +options[.rbf]=> ad86032020g300070_0.lc Selected FITS extensions: 1 - RATE TABLE; Source ............ VIRGO_SOUTH_N17 Start Time (d) .... 10984 06:29:09.968 FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10984 14:00:21.968 No. of Rows ....... 103 Bin Time (s) ...... 150.2 Right Ascension ... 1.8799E+02 Internal time sys.. Converted to TJD Declination ....... 8.1320E+00 Experiment ........ ASCA GIS3 Filter ............ NONE Corrections applied: Vignetting - No ; Deadtime - No ; Bkgd - No ; Clock - No Selected Columns: 1 - Time; 2 - Y-axis; 3 - Y-error; File contains binned data. Ser. A filename 2 +options[.rbf]=> Enter up to 50 input filenames and options for series 2 (or rtn) Ser. B filename 1 +options[.rbf]=> Enter up to 50 input filenames and options for series 3 (or rtn) Ser. C filename 1 +options[.rbf]=> [3]xronos> Maximum of 1 Intvs. with 181 Newbins of 150.233 (s) Intv 1 Start10984 6:30:25 Ser.1 Avg 0.3313 Chisq 89.36 Var 0.2056E-02 Newbs. 103 Min 0.2396 Max 0.4260 expVar 0.2370E-02 Bins 103 Results from Statistical Analysis Newbin Integration Time (s).. 150.23 Interval Duration (s)........ 26892. No. of Newbins .............. 103 Average (c/s) ............... 0.33132 +/- 0.48E-02 Standard Deviation (c/s)..... 0.45343E-01 Minimum (c/s)................ 0.23963 Maximum (c/s)................ 0.42600 Variance ((c/s)**2).......... 0.20560E-02 +/- 0.29E-03 Expected Variance ((c/s)**2). 0.23699E-02 +/- 0.33E-03 Third Moment ((c/s)**3)......-0.79150E-05 Average Deviation (c/s)...... 0.37089E-01 Skewness.....................-0.84904E-01 +/- 0.24 Kurtosis.....................-0.71596 +/- 0.48 RMS fractional variation....< 0.11428 (3 sigma) Chi-Square................... 89.356 dof 102 Chi-Square Prob of constancy. 0.80990 (0 means < 1.e-38) Kolm.-Smir. Prob of constancy 0.39285 (0 means < 1.e-38) [4]xronos> [5]xronos> Maximum of 1 Intvs. with 181 Newbins of 150.233 (s) Intv 1 Start10984 6:30:25 Ser.1 Avg 0.3313 Chisq 89.36 Var 0.2056E-02 Newbs. 103 Min 0.2396 Max 0.4260 expVar 0.2370E-02 Bins 103 Light curve ready ! Frme 1 Written to output file : xronos.qlc1 PLT> LA File ad86032020g300070_0.lc PLT> hard /ps PLT> [6]xronos>-> Merging GTIs from the following files:
ad86032020g200170h.evt[2] ad86032020g200270m.evt[2]-> Making L1 light curve of ft980620_0532_1400G2HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 17469 output records from 17486 good input G2_L1 records.-> Making L1 light curve of ft980620_0532_1400G2HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 12874 output records from 21939 good input G2_L1 records.-> Merging GTIs from the following files:
ad86032020g300170h.evt[2] ad86032020g300270m.evt[2]-> Making L1 light curve of ft980620_0532_1400G3HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 16608 output records from 16625 good input G3_L1 records.-> Making L1 light curve of ft980620_0532_1400G3HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 12746 output records from 21030 good input G3_L1 records.
*** tlmFrm Version 1.1 (1997-08-25) *** total number of superframes: 6658 Total of 0 sets of frame data are extracted.-> Extracting corner pixel GTIs with the following criteria:
SUNSHINE==0 && T_DY_NT>64 && T_SAA>64 && SAA==0 && COR>6 && (ELV>10 || ELV<10 )-> Extracting GTIs from ft980620_0532_1400.mkf
1 ad86032020g200170h.unf 18459 1 ad86032020g200270m.unf 18459 1 ad86032020g200370l.unf 18459-> Fetching GIS2_CALSRC256.2
XSPEC 9.01 02:09:22 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> query yes Querying disabled - assuming answer is yes !XSPEC> data ad86032020g220170.cal Net count rate (cts/s) for file 1 0.1329 +/- 2.4870E-03 1 data set is in use !XSPEC> ignore bad !XSPEC> ignore **-4.0 !XSPEC> ignore 8.0-** !XSPEC> model const/b + gauss/b + gauss/b Background components must be from the additive model list mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Input parameter value, delta, min, bot, top, and max values for ... Mod parameter 1 of component 1 constant factor 1.000 1.0000E-02 0. 0. 1.0000E+10 1.0000E+10 ! Mod parameter 2 of component 2 gaussian LineE 6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06 ! 5.9 Mod parameter 3 of component 2 gaussian Sigma 0.1000 5.0000E-02 0. 0. 10.00 20.00 ! 0.0 Mod parameter 4 of component 2 gaussian norm 1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24 ! Mod parameter 5 of component 3 gaussian LineE 6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06 ! 6.5 Mod parameter 6 of component 3 gaussian Sigma 0.1000 5.0000E-02 0. 0. 10.00 20.00 ! 0.0 Mod parameter 7 of component 3 gaussian norm 1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24 ! --------------------------------------------------------------------------- --------------------------------------------------------------------------- mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Model Fit Model Component Parameter Value par par comp 1 1 1 constant factor 1.00000 +/- 0. 2 2 2 gaussian/b LineE 5.90000 +/- 0. 3 3 2 gaussian/b Sigma 0. +/- 0. 4 4 2 gaussian/b norm 1.00000 +/- 0. 5 5 3 gaussian/b LineE 6.50000 +/- 0. 6 6 3 gaussian/b Sigma 0. +/- 0. 7 7 3 gaussian/b norm 1.00000 +/- 0. --------------------------------------------------------------------------- --------------------------------------------------------------------------- 7 variable fit parameters Chi-Squared = 1.0791E+06 using 84 PHA bins. Reduced chi-squared = 1.4014E+04 !XSPEC> newpar 5 = 2 1.101005 6 variable fit parameters Chi-Squared = 1.0732E+06 using 84 PHA bins. Reduced chi-squared = 1.3759E+04 !XSPEC> newpar 6 = 3 1.049288 5 variable fit parameters Chi-Squared = 1.0732E+06 using 84 PHA bins. Reduced chi-squared = 1.3585E+04 !XSPEC> renorm Chi-Squared = 584.0 using 84 PHA bins. Reduced chi-squared = 7.392 !XSPEC> fit Chi-Squared Lvl Fit param # 1 2 3 4 5 Due to zero model norms fit parameter 1 is temporarily frozen 468.12 0 1.000 5.895 0.1002 3.8789E-02 3.5533E-02 Due to zero model norms fit parameter 1 is temporarily frozen 266.46 0 1.000 5.880 0.1520 5.0940E-02 3.1912E-02 Due to zero model norms fit parameter 1 is temporarily frozen 159.89 -1 1.000 5.934 0.1778 6.8096E-02 2.3066E-02 Due to zero model norms fit parameter 1 is temporarily frozen 134.08 -2 1.000 5.995 0.2046 7.9971E-02 1.4552E-02 Due to zero model norms fit parameter 1 is temporarily frozen 133.17 -3 1.000 5.983 0.1949 7.8320E-02 1.6142E-02 Due to zero model norms fit parameter 1 is temporarily frozen 133.14 -4 1.000 5.986 0.1961 7.8801E-02 1.5663E-02 Due to zero model norms fit parameter 1 is temporarily frozen 133.12 -5 1.000 5.985 0.1955 7.8666E-02 1.5796E-02 Due to zero model norms fit parameter 1 is temporarily frozen 133.12 0 1.000 5.985 0.1955 7.8671E-02 1.5790E-02 --------------------------------------------------------------------------- --------------------------------------------------------------------------- mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Model Fit Model Component Parameter Value par par comp 1 1 1 constant factor 1.00000 +/- -1.0000 2 2 2 gaussian/b LineE 5.98537 +/- 0.12477E-01 3 3 2 gaussian/b Sigma 0.195463 +/- 0.12511E-01 4 4 2 gaussian/b norm 7.867076E-02 +/- 0.25771E-02 5 2 3 gaussian/b LineE 6.58992 = par 2 * 1.1010 6 3 3 gaussian/b Sigma 0.205097 = par 3 * 1.0493 7 5 3 gaussian/b norm 1.578981E-02 +/- 0.19058E-02 --------------------------------------------------------------------------- --------------------------------------------------------------------------- Chi-Squared = 133.1 using 84 PHA bins. Reduced chi-squared = 1.685 !XSPEC> setplot energy !XSPEC> iplot data !PLT> label top GIS2 Calibration Source, should peak near 5.9 keV !PLT> log x off !PLT> rescale x 4 8 !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Calibration source ad86032020g220170.cal peaks at 5.98537 +/- 0.012477 keV
1 ad86032020g300170h.unf 17453 1 ad86032020g300270m.unf 17453 1 ad86032020g300370l.unf 17453-> Fetching GIS3_CALSRC256.2
XSPEC 9.01 02:10:01 12-Dec-99 Plot device not set, use "cpd" to set it Type "help" or "?" for further information !XSPEC> query yes Querying disabled - assuming answer is yes !XSPEC> data ad86032020g320170.cal Net count rate (cts/s) for file 1 0.1163 +/- 2.3342E-03 1 data set is in use !XSPEC> ignore bad !XSPEC> ignore **-4.0 !XSPEC> ignore 8.0-** !XSPEC> model const/b + gauss/b + gauss/b Background components must be from the additive model list mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Input parameter value, delta, min, bot, top, and max values for ... Mod parameter 1 of component 1 constant factor 1.000 1.0000E-02 0. 0. 1.0000E+10 1.0000E+10 ! Mod parameter 2 of component 2 gaussian LineE 6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06 ! 5.9 Mod parameter 3 of component 2 gaussian Sigma 0.1000 5.0000E-02 0. 0. 10.00 20.00 ! 0.0 Mod parameter 4 of component 2 gaussian norm 1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24 ! Mod parameter 5 of component 3 gaussian LineE 6.500 5.0000E-02 0. 0. 1.0000E+06 1.0000E+06 ! 6.5 Mod parameter 6 of component 3 gaussian Sigma 0.1000 5.0000E-02 0. 0. 10.00 20.00 ! 0.0 Mod parameter 7 of component 3 gaussian norm 1.000 1.0000E-02 0. 0. 1.0000E+24 1.0000E+24 ! --------------------------------------------------------------------------- --------------------------------------------------------------------------- mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Model Fit Model Component Parameter Value par par comp 1 1 1 constant factor 1.00000 +/- 0. 2 2 2 gaussian/b LineE 5.90000 +/- 0. 3 3 2 gaussian/b Sigma 0. +/- 0. 4 4 2 gaussian/b norm 1.00000 +/- 0. 5 5 3 gaussian/b LineE 6.50000 +/- 0. 6 6 3 gaussian/b Sigma 0. +/- 0. 7 7 3 gaussian/b norm 1.00000 +/- 0. --------------------------------------------------------------------------- --------------------------------------------------------------------------- 7 variable fit parameters Chi-Squared = 1.6112E+06 using 84 PHA bins. Reduced chi-squared = 2.0924E+04 !XSPEC> newpar 5 = 2 1.101005 6 variable fit parameters Chi-Squared = 1.5914E+06 using 84 PHA bins. Reduced chi-squared = 2.0403E+04 !XSPEC> newpar 6 = 3 1.049288 5 variable fit parameters Chi-Squared = 1.5914E+06 using 84 PHA bins. Reduced chi-squared = 2.0145E+04 !XSPEC> renorm Chi-Squared = 942.0 using 84 PHA bins. Reduced chi-squared = 11.92 !XSPEC> fit Chi-Squared Lvl Fit param # 1 2 3 4 5 Due to zero model norms fit parameter 1 is temporarily frozen 784.60 0 1.000 5.891 5.5950E-02 2.9289E-02 2.4315E-02 Due to zero model norms fit parameter 1 is temporarily frozen 306.96 0 1.000 5.856 7.5365E-02 4.9886E-02 2.0738E-02 Due to zero model norms fit parameter 1 is temporarily frozen 152.76 -1 1.000 5.875 0.1447 6.9944E-02 1.5922E-02 Due to zero model norms fit parameter 1 is temporarily frozen 104.64 -2 1.000 5.928 0.1659 8.0733E-02 9.0120E-03 Due to zero model norms fit parameter 1 is temporarily frozen 103.48 -3 1.000 5.937 0.1715 8.2444E-02 7.8413E-03 Due to zero model norms fit parameter 1 is temporarily frozen 103.48 -4 1.000 5.937 0.1726 8.2558E-02 7.7822E-03 --------------------------------------------------------------------------- --------------------------------------------------------------------------- mo = constant[1] ) + gaussian/b[2] + gaussian/b[3] Model Fit Model Component Parameter Value par par comp 1 1 1 constant factor 1.00000 +/- -1.0000 2 2 2 gaussian/b LineE 5.93735 +/- 0.92640E-02 3 3 2 gaussian/b Sigma 0.172556 +/- 0.11057E-01 4 4 2 gaussian/b norm 8.255832E-02 +/- 0.22524E-02 5 2 3 gaussian/b LineE 6.53705 = par 2 * 1.1010 6 3 3 gaussian/b Sigma 0.181061 = par 3 * 1.0493 7 5 3 gaussian/b norm 7.782214E-03 +/- 0.13787E-02 --------------------------------------------------------------------------- --------------------------------------------------------------------------- Chi-Squared = 103.5 using 84 PHA bins. Reduced chi-squared = 1.310 !XSPEC> setplot energy !XSPEC> iplot data !PLT> label top GIS3 Calibration Source, should peak near 5.9 keV !PLT> log x off !PLT> rescale x 4 8 !PLT> hard /ps !PLT> quit !XSPEC> exit !Do you really want to exit (y) y XSPEC: quit-> Calibration source ad86032020g320170.cal peaks at 5.93735 +/- 0.009264 keV
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000102h.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 319 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 6 297 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 6 Number of (internal) image counts : 319 Number of image cts rejected (N, %) : 29793.10 By chip : 0 1 2 3 Pixels rejected : 0 6 0 0 Image counts : 0 319 0 0 Image cts rejected: 0 297 0 0 Image cts rej (%) : 0.00 93.10 0.00 0.00 filtering data... Total counts : 0 319 0 0 Total cts rejected: 0 297 0 0 Total cts rej (%) : 0.00 93.10 0.00 0.00 Number of clean counts accepted : 22 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 6 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s000112h.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000112h.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 324 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 6 297 Flickering pixels iter, pixels & cnts : 1 1 6 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 7 Number of (internal) image counts : 324 Number of image cts rejected (N, %) : 30393.52 By chip : 0 1 2 3 Pixels rejected : 0 7 0 0 Image counts : 0 324 0 0 Image cts rejected: 0 303 0 0 Image cts rej (%) : 0.00 93.52 0.00 0.00 filtering data... Total counts : 0 324 0 0 Total cts rejected: 0 303 0 0 Total cts rej (%) : 0.00 93.52 0.00 0.00 Number of clean counts accepted : 21 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 7 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s000202m.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000202m.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 253 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 6 224 Flickering pixels iter, pixels & cnts : 1 1 4 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 7 Number of (internal) image counts : 253 Number of image cts rejected (N, %) : 22890.12 By chip : 0 1 2 3 Pixels rejected : 0 7 0 0 Image counts : 0 253 0 0 Image cts rejected: 0 228 0 0 Image cts rej (%) : 0.00 90.12 0.00 0.00 filtering data... Total counts : 0 253 0 0 Total cts rejected: 0 228 0 0 Total cts rej (%) : 0.00 90.12 0.00 0.00 Number of clean counts accepted : 25 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 7 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s000212m.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000212m.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 260 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 6 224 Flickering pixels iter, pixels & cnts : 1 1 4 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 7 Number of (internal) image counts : 260 Number of image cts rejected (N, %) : 22887.69 By chip : 0 1 2 3 Pixels rejected : 0 7 0 0 Image counts : 0 260 0 0 Image cts rejected: 0 228 0 0 Image cts rej (%) : 0.00 87.69 0.00 0.00 filtering data... Total counts : 0 260 0 0 Total cts rejected: 0 228 0 0 Total cts rej (%) : 0.00 87.69 0.00 0.00 Number of clean counts accepted : 32 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 7 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s000302l.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000302l.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 1665 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 7 1547 Flickering pixels iter, pixels & cnts : 1 4 18 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 11 Number of (internal) image counts : 1665 Number of image cts rejected (N, %) : 156593.99 By chip : 0 1 2 3 Pixels rejected : 0 11 0 0 Image counts : 0 1665 0 0 Image cts rejected: 0 1565 0 0 Image cts rej (%) : 0.00 93.99 0.00 0.00 filtering data... Total counts : 0 1665 0 0 Total cts rejected: 0 1565 0 0 Total cts rej (%) : 0.00 93.99 0.00 0.00 Number of clean counts accepted : 100 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 11 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s000312l.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s000312l.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 1684 copy bad pix array... cleaning chip # 0 cleaning chip # 1 Hot pixels & counts : 7 1547 Flickering pixels iter, pixels & cnts : 1 4 18 cleaning chip # 2 cleaning chip # 3 Number of pixels rejected : 11 Number of (internal) image counts : 1684 Number of image cts rejected (N, %) : 156592.93 By chip : 0 1 2 3 Pixels rejected : 0 11 0 0 Image counts : 0 1684 0 0 Image cts rejected: 0 1565 0 0 Image cts rej (%) : 0.00 92.93 0.00 0.00 filtering data... Total counts : 0 1684 0 0 Total cts rejected: 0 1565 0 0 Total cts rej (%) : 0.00 92.93 0.00 0.00 Number of clean counts accepted : 119 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 11 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100102h.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100102h.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 1191 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 15 1138 Flickering pixels iter, pixels & cnts : 1 1 5 Number of pixels rejected : 16 Number of (internal) image counts : 1191 Number of image cts rejected (N, %) : 114395.97 By chip : 0 1 2 3 Pixels rejected : 0 0 0 16 Image counts : 0 0 0 1191 Image cts rejected: 0 0 0 1143 Image cts rej (%) : 0.00 0.00 0.00 95.97 filtering data... Total counts : 0 0 0 1191 Total cts rejected: 0 0 0 1143 Total cts rej (%) : 0.00 0.00 0.00 95.97 Number of clean counts accepted : 48 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 16 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100112h.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100112h.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 1195 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 15 1138 Flickering pixels iter, pixels & cnts : 1 1 5 Number of pixels rejected : 16 Number of (internal) image counts : 1195 Number of image cts rejected (N, %) : 114395.65 By chip : 0 1 2 3 Pixels rejected : 0 0 0 16 Image counts : 0 0 0 1195 Image cts rejected: 0 0 0 1143 Image cts rej (%) : 0.00 0.00 0.00 95.65 filtering data... Total counts : 0 0 0 1195 Total cts rejected: 0 0 0 1143 Total cts rej (%) : 0.00 0.00 0.00 95.65 Number of clean counts accepted : 52 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 16 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100202m.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100202m.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 911 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 15 877 Flickering pixels iter, pixels & cnts : 1 1 3 Number of pixels rejected : 16 Number of (internal) image counts : 911 Number of image cts rejected (N, %) : 88096.60 By chip : 0 1 2 3 Pixels rejected : 0 0 0 16 Image counts : 0 0 0 911 Image cts rejected: 0 0 0 880 Image cts rej (%) : 0.00 0.00 0.00 96.60 filtering data... Total counts : 0 0 0 911 Total cts rejected: 0 0 0 880 Total cts rej (%) : 0.00 0.00 0.00 96.60 Number of clean counts accepted : 31 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 16 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100212m.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100212m.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 914 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 15 877 Flickering pixels iter, pixels & cnts : 1 1 3 Number of pixels rejected : 16 Number of (internal) image counts : 914 Number of image cts rejected (N, %) : 88096.28 By chip : 0 1 2 3 Pixels rejected : 0 0 0 16 Image counts : 0 0 0 914 Image cts rejected: 0 0 0 880 Image cts rej (%) : 0.00 0.00 0.00 96.28 filtering data... Total counts : 0 0 0 914 Total cts rejected: 0 0 0 880 Total cts rej (%) : 0.00 0.00 0.00 96.28 Number of clean counts accepted : 34 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 16 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100302l.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100302l.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 2919 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 14 2813 Flickering pixels iter, pixels & cnts : 1 5 53 Number of pixels rejected : 19 Number of (internal) image counts : 2919 Number of image cts rejected (N, %) : 286698.18 By chip : 0 1 2 3 Pixels rejected : 0 0 0 19 Image counts : 0 0 0 2919 Image cts rejected: 0 0 0 2866 Image cts rej (%) : 0.00 0.00 0.00 98.18 filtering data... Total counts : 0 0 0 2919 Total cts rejected: 0 0 0 2866 Total cts rej (%) : 0.00 0.00 0.00 98.18 Number of clean counts accepted : 53 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 19 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020s100312l.unf
CLEANSIS_V1.6 allocating image arrays... PROGRAM TO MAKE AN SIS SCIENCE FILE CLEANED OF ANOMALOUS PIXELS. * Anomalous pixels may consist of at least two populations. 1. Persistent HOT pixels are removed by comparing to the chip mean. 2. Flickering WARM pixels are removed by comparing to the cell mean. 3. In faint areas (zero bgd), flickering pixels are removed with a cutoff threshold. Hints: Choose cell size and thresholds based on the expected background and the PSF. Use the DIRTYSIS option to examine the anomalous pixel spectra. Try a multiple pass clean: Choose a PHA cut to optimize the S/N of the flickering pixels, then a broad band clean. Be suspicious of extended source cleans. For very bright sources you may need to turn off the iteration option. See the help page for further info (fhelp cleansis) Poisson clean cell size : 5 Poisson probability threshold : 0.575E-05 Zero Bgd Cutoff threshold (>) : 3 Iterate : F Dirtysis : F Minimum PHA value (inclusive) : 0 Maximum PHA value (inclusive) : 4095 open output file: ad86032020s100312l.drk reading data file: event.tmp copying primary header to output file... making chip image... Total counts in chip images : 2928 copy bad pix array... cleaning chip # 0 cleaning chip # 1 cleaning chip # 2 cleaning chip # 3 Hot pixels & counts : 14 2813 Flickering pixels iter, pixels & cnts : 1 5 53 Number of pixels rejected : 19 Number of (internal) image counts : 2928 Number of image cts rejected (N, %) : 286697.88 By chip : 0 1 2 3 Pixels rejected : 0 0 0 19 Image counts : 0 0 0 2928 Image cts rejected: 0 0 0 2866 Image cts rej (%) : 0.00 0.00 0.00 97.88 filtering data... Total counts : 0 0 0 2928 Total cts rejected: 0 0 0 2866 Total cts rej (%) : 0.00 0.00 0.00 97.88 Number of clean counts accepted : 62 writing history cards... copying extensions... writing out hot pixs... Number of rejected pixels : 19 updating NEVENTS keywords... closing data file... closing clean file...-> Extracting bright and dark Earth events from ad86032020g200170h.unf
Offset of 208224004.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1999-08-08 00:00:00.00000 Modified Julian Day = 51398.000000000000000-> leapsec.fits already present in current directory
Offset of 197078404.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1999-04-01 00:00:00.00000 Modified Julian Day = 51269.000000000000000-> leapsec.fits already present in current directory
Offset of 150000000.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-10-03 02:39:56.00000 Modified Julian Day = 50724.111064814816928
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