The following information is also available:
Time column is TIME ORDERED-> Determining observation start and end
Offset of 150009660.400800 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-10-03 05:20:56.40079 Modified Julian Day = 50724.222875009261770-> leapsec.fits already present in current directory
Offset of 150027084.341800 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1997-10-03 10:11:20.34180 Modified Julian Day = 50724.424540993059054-> Observation begins 150009660.4008 1997-10-03 05:20:56
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 : 150009664.400600 150027084.341800
Data file start and stop ascatime : 150009664.400600 150027084.341800
Aspecting run start and stop ascatime : 150009664.400679 150027084.341718
Time interval averaged over (seconds) : 17419.941039
Total pointing and manuver time (sec) : 11016.982422 6402.982422
Mean boresight Euler angles : 121.954489 128.559460 10.761398
RA DEC SUN ANGLE
Mean solar position (deg) : 188.41 -3.63
Mean aberration (arcsec) : -9.03 17.19
Mean sat X-axis (deg) : 284.997211 -50.193380 91.41
Mean sat Y-axis (deg) : 205.198103 8.395625 20.61
Mean sat Z-axis (deg) : 121.954489 -38.559461 69.44
RA DEC ROLL OFFSET
(deg) (deg) (deg) (arcmin)
Average 122.238167 -38.382046 280.937714 0.040274
Minimum 122.227913 -38.431103 280.901703 0.000000
Maximum 122.240417 -38.343403 280.960938 2.945418
Sigma (RMS) 0.000258 0.000211 0.001280 0.071343
Number of ASPECT records processed = 19025
Aspecting to RA/DEC : 122.23816681 -38.38204575
closing output file...
closing attitude file...
-> Standard Output From STOOL checkatt:
Opening file: ./out.tmp
***************** Observation Info ******************
RA (J2000 deg): 122.238 DEC: -38.382
START TIME: SC 150009664.4007 = UT 1997-10-03 05:21:04
****** 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
4.000097 2.158 8603 1 1 0 0 0 0 0 0 0 1 1 0 0 0 0 0 0
103.999878 1.135 8603 1 1 0 0 0 0 0 0 0 1 1 0 0 0 0 0 0
359.998962 0.106 8403 1 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0
599.998108 0.039 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0
2701.991211 0.077 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
6311.978516 0.014 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0
8445.971680 0.022 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
12041.958984 0.042 8C03 1 1 0 0 0 0 0 0 0 0 1 1 0 0 0 0 0
14189.952148 0.037 8003 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
17419.941406 2.945 9403 1 1 0 0 0 0 0 0 0 0 1 0 1 0 0 0 0
Attitude Records: 19025
Attitude Steps: 10
Maneuver ACM time: 6403.00 sec
Pointed ACM time: 11017.0 sec
-> Calculating aspect point99 99 count=1 sum1=121.945 sum2=128.523 sum3=10.768 99 100 count=1 sum1=121.945 sum2=128.525 sum3=10.766 100 100 count=12 sum1=1463.36 sum2=1542.35 sum3=129.261 100 101 count=15 sum1=1829.24 sum2=1928.09 sum3=161.495 100 102 count=23 sum1=2804.88 sum2=2956.6 sum3=247.564 100 103 count=18946 sum1=2.31055e+06 sum2=2.43569e+06 sum3=203882 101 103 count=26 sum1=3170.86 sum2=3342.56 sum3=279.921 101 108 count=1 sum1=121.956 sum2=128.608 sum3=10.725 0 out of 19025 points outside bin structure-> Euler angles: 121.954, 128.559, 10.7612
Interpolating 5 records in time interval 150027060.342 - 150027084.342
639.998 second gap between superframes 28 and 29 Dropping SF 269 with corrupted frame indicator Dropping SF 669 with corrupted frame indicator 595.998 second gap between superframes 1902 and 1903 Dropped 1st C3 read after clocking change in ft971003_0520_1011S001401H.fits Dropped 1st C0 read after clocking change in ft971003_0520_1011S001401H.fits Dropped 1st C1 read after clocking change in ft971003_0520_1011S001601H.fits 715.998 second gap between superframes 3849 and 3850 4764 of 4766 super frames processed-> Removing the following files with NEVENTS=0
ft971003_0520_1011G200570H.fits[0] ft971003_0520_1011G201470H.fits[0] ft971003_0520_1011G201570L.fits[0] ft971003_0520_1011G201670H.fits[0] ft971003_0520_1011G201770H.fits[0] ft971003_0520_1011G201870H.fits[0] ft971003_0520_1011G201970H.fits[0] ft971003_0520_1011G202070H.fits[0] ft971003_0520_1011G202870H.fits[0] ft971003_0520_1011G203070H.fits[0] ft971003_0520_1011G203170H.fits[0] ft971003_0520_1011G203270L.fits[0] ft971003_0520_1011G203370H.fits[0] ft971003_0520_1011G203470H.fits[0] ft971003_0520_1011G203570H.fits[0] ft971003_0520_1011G203670H.fits[0] ft971003_0520_1011G203770H.fits[0] ft971003_0520_1011G300570H.fits[0] ft971003_0520_1011G301470H.fits[0] ft971003_0520_1011G301570L.fits[0] ft971003_0520_1011G301670H.fits[0] ft971003_0520_1011G301770H.fits[0] ft971003_0520_1011G301870H.fits[0] ft971003_0520_1011G301970H.fits[0] ft971003_0520_1011G302670H.fits[0] ft971003_0520_1011G302870H.fits[0] ft971003_0520_1011G303070H.fits[0] ft971003_0520_1011G303170H.fits[0] ft971003_0520_1011G303270L.fits[0] ft971003_0520_1011G303370H.fits[0] ft971003_0520_1011G303470H.fits[0] ft971003_0520_1011G303570H.fits[0] ft971003_0520_1011G303670H.fits[0] ft971003_0520_1011S001802H.fits[0] ft971003_0520_1011S002402L.fits[0] ft971003_0520_1011S002502M.fits[0] ft971003_0520_1011S101702H.fits[0]-> Checking for empty GTI extensions
ft971003_0520_1011S000102M.fits[2] ft971003_0520_1011S000202L.fits[2] ft971003_0520_1011S000301L.fits[2] ft971003_0520_1011S000401H.fits[2] ft971003_0520_1011S000502M.fits[2] ft971003_0520_1011S000601M.fits[2] ft971003_0520_1011S000701H.fits[2] ft971003_0520_1011S000802H.fits[2] ft971003_0520_1011S000902L.fits[2] ft971003_0520_1011S001001L.fits[2] ft971003_0520_1011S001101H.fits[2] ft971003_0520_1011S001202M.fits[2] ft971003_0520_1011S001301M.fits[2] ft971003_0520_1011S001401H.fits[2] ft971003_0520_1011S001501H.fits[2] ft971003_0520_1011S001601H.fits[2] ft971003_0520_1011S001701H.fits[2] ft971003_0520_1011S001902L.fits[2] ft971003_0520_1011S002002L.fits[2] ft971003_0520_1011S002101L.fits[2] ft971003_0520_1011S002201H.fits[2] ft971003_0520_1011S002302H.fits[2]-> Merging GTIs from the following files:
ft971003_0520_1011S100102M.fits[2] ft971003_0520_1011S100202L.fits[2] ft971003_0520_1011S100301L.fits[2] ft971003_0520_1011S100401H.fits[2] ft971003_0520_1011S100502M.fits[2] ft971003_0520_1011S100601M.fits[2] ft971003_0520_1011S100701H.fits[2] ft971003_0520_1011S100802H.fits[2] ft971003_0520_1011S100902L.fits[2] ft971003_0520_1011S101001L.fits[2] ft971003_0520_1011S101101H.fits[2] ft971003_0520_1011S101202M.fits[2] ft971003_0520_1011S101301M.fits[2] ft971003_0520_1011S101401H.fits[2] ft971003_0520_1011S101501H.fits[2] ft971003_0520_1011S101601H.fits[2] ft971003_0520_1011S101802L.fits[2] ft971003_0520_1011S101902L.fits[2] ft971003_0520_1011S102001L.fits[2] ft971003_0520_1011S102101H.fits[2] ft971003_0520_1011S102202H.fits[2] ft971003_0520_1011S102302L.fits[2] ft971003_0520_1011S102402M.fits[2]-> Merging GTIs from the following files:
ft971003_0520_1011G200170M.fits[2] ft971003_0520_1011G200270L.fits[2] ft971003_0520_1011G200370H.fits[2] ft971003_0520_1011G200470H.fits[2] ft971003_0520_1011G200670H.fits[2] ft971003_0520_1011G200770H.fits[2] ft971003_0520_1011G200870H.fits[2] ft971003_0520_1011G200970H.fits[2] ft971003_0520_1011G201070M.fits[2] ft971003_0520_1011G201170M.fits[2] ft971003_0520_1011G201270H.fits[2] ft971003_0520_1011G201370H.fits[2] ft971003_0520_1011G202170H.fits[2] ft971003_0520_1011G202270H.fits[2] ft971003_0520_1011G202370H.fits[2] ft971003_0520_1011G202470M.fits[2] ft971003_0520_1011G202570M.fits[2] ft971003_0520_1011G202670H.fits[2] ft971003_0520_1011G202770H.fits[2] ft971003_0520_1011G202970H.fits[2] ft971003_0520_1011G203870H.fits[2] ft971003_0520_1011G203970H.fits[2] ft971003_0520_1011G204070H.fits[2] ft971003_0520_1011G204170L.fits[2] ft971003_0520_1011G204270L.fits[2] ft971003_0520_1011G204370M.fits[2]-> Merging GTIs from the following files:
ft971003_0520_1011G300170M.fits[2] ft971003_0520_1011G300270L.fits[2] ft971003_0520_1011G300370H.fits[2] ft971003_0520_1011G300470H.fits[2] ft971003_0520_1011G300670H.fits[2] ft971003_0520_1011G300770H.fits[2] ft971003_0520_1011G300870H.fits[2] ft971003_0520_1011G300970H.fits[2] ft971003_0520_1011G301070M.fits[2] ft971003_0520_1011G301170M.fits[2] ft971003_0520_1011G301270H.fits[2] ft971003_0520_1011G301370H.fits[2] ft971003_0520_1011G302070H.fits[2] ft971003_0520_1011G302170H.fits[2] ft971003_0520_1011G302270H.fits[2] ft971003_0520_1011G302370H.fits[2] ft971003_0520_1011G302470M.fits[2] ft971003_0520_1011G302570M.fits[2] ft971003_0520_1011G302770H.fits[2] ft971003_0520_1011G302970H.fits[2] ft971003_0520_1011G303770H.fits[2] ft971003_0520_1011G303870H.fits[2] ft971003_0520_1011G303970H.fits[2] ft971003_0520_1011G304070H.fits[2] ft971003_0520_1011G304170L.fits[2] ft971003_0520_1011G304270L.fits[2] ft971003_0520_1011G304370M.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 = 2 photon cnt = 2 GISSORTSPLIT:LO:g200270h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200370h.prelist merge count = 3 photon cnt = 8 GISSORTSPLIT:LO:g200470h.prelist merge count = 3 photon cnt = 9 GISSORTSPLIT:LO:g200570h.prelist merge count = 6 photon cnt = 6019 GISSORTSPLIT:LO:g200670h.prelist merge count = 1 photon cnt = 1 GISSORTSPLIT:LO:g200770h.prelist merge count = 1 photon cnt = 2 GISSORTSPLIT:LO:g200170l.prelist merge count = 2 photon cnt = 937 GISSORTSPLIT:LO:g200270l.prelist merge count = 1 photon cnt = 145 GISSORTSPLIT:LO:g200170m.prelist merge count = 4 photon cnt = 1662 GISSORTSPLIT:LO:g200270m.prelist merge count = 2 photon cnt = 89 GISSORTSPLIT:LO:Total filenames split = 26 GISSORTSPLIT:LO:Total split file cnt = 11 GISSORTSPLIT:LO:End program-> Creating ad95009040g200170h.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011G200370H.fits 2 -- ft971003_0520_1011G200970H.fits 3 -- ft971003_0520_1011G201270H.fits 4 -- ft971003_0520_1011G202370H.fits 5 -- ft971003_0520_1011G202970H.fits 6 -- ft971003_0520_1011G204070H.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G200370H.fits 2 -- ft971003_0520_1011G200970H.fits 3 -- ft971003_0520_1011G201270H.fits 4 -- ft971003_0520_1011G202370H.fits 5 -- ft971003_0520_1011G202970H.fits 6 -- ft971003_0520_1011G204070H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040g200270m.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 -- ft971003_0520_1011G200170M.fits 2 -- ft971003_0520_1011G201170M.fits 3 -- ft971003_0520_1011G202570M.fits 4 -- ft971003_0520_1011G204370M.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G200170M.fits 2 -- ft971003_0520_1011G201170M.fits 3 -- ft971003_0520_1011G202570M.fits 4 -- ft971003_0520_1011G204370M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040g200370l.unf
---- cmerge: version 1.6 ---- A total of 2 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011G200270L.fits 2 -- ft971003_0520_1011G204270L.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G200270L.fits 2 -- ft971003_0520_1011G204270L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000145 events
ft971003_0520_1011G204170L.fits-> Ignoring the following files containing 000000089 events
ft971003_0520_1011G201070M.fits ft971003_0520_1011G202470M.fits-> Ignoring the following files containing 000000009 events
ft971003_0520_1011G200870H.fits ft971003_0520_1011G202270H.fits ft971003_0520_1011G203970H.fits-> Ignoring the following files containing 000000008 events
ft971003_0520_1011G200770H.fits ft971003_0520_1011G202170H.fits ft971003_0520_1011G203870H.fits-> Ignoring the following files containing 000000002 events
ft971003_0520_1011G202770H.fits-> Ignoring the following files containing 000000002 events
ft971003_0520_1011G200670H.fits-> Ignoring the following files containing 000000002 events
ft971003_0520_1011G200470H.fits ft971003_0520_1011G201370H.fits-> Ignoring the following files containing 000000001 events
ft971003_0520_1011G202670H.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 = 2 photon cnt = 2 GISSORTSPLIT:LO:g300270h.prelist merge count = 3 photon cnt = 5 GISSORTSPLIT:LO:g300370h.prelist merge count = 3 photon cnt = 5 GISSORTSPLIT:LO:g300470h.prelist merge count = 3 photon cnt = 6 GISSORTSPLIT:LO:g300570h.prelist merge count = 6 photon cnt = 5373 GISSORTSPLIT:LO:g300670h.prelist merge count = 1 photon cnt = 3 GISSORTSPLIT:LO:g300170l.prelist merge count = 2 photon cnt = 855 GISSORTSPLIT:LO:g300270l.prelist merge count = 1 photon cnt = 132 GISSORTSPLIT:LO:g300170m.prelist merge count = 4 photon cnt = 1581 GISSORTSPLIT:LO:g300270m.prelist merge count = 2 photon cnt = 87 GISSORTSPLIT:LO:Total filenames split = 27 GISSORTSPLIT:LO:Total split file cnt = 10 GISSORTSPLIT:LO:End program-> Creating ad95009040g300170h.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011G300370H.fits 2 -- ft971003_0520_1011G300970H.fits 3 -- ft971003_0520_1011G301270H.fits 4 -- ft971003_0520_1011G302370H.fits 5 -- ft971003_0520_1011G302970H.fits 6 -- ft971003_0520_1011G304070H.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G300370H.fits 2 -- ft971003_0520_1011G300970H.fits 3 -- ft971003_0520_1011G301270H.fits 4 -- ft971003_0520_1011G302370H.fits 5 -- ft971003_0520_1011G302970H.fits 6 -- ft971003_0520_1011G304070H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040g300270m.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 -- ft971003_0520_1011G300170M.fits 2 -- ft971003_0520_1011G301170M.fits 3 -- ft971003_0520_1011G302570M.fits 4 -- ft971003_0520_1011G304370M.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G300170M.fits 2 -- ft971003_0520_1011G301170M.fits 3 -- ft971003_0520_1011G302570M.fits 4 -- ft971003_0520_1011G304370M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040g300370l.unf
---- cmerge: version 1.6 ---- A total of 2 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011G300270L.fits 2 -- ft971003_0520_1011G304270L.fits Merging binary extension #: 2 1 -- ft971003_0520_1011G300270L.fits 2 -- ft971003_0520_1011G304270L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000132 events
ft971003_0520_1011G304170L.fits-> Ignoring the following files containing 000000087 events
ft971003_0520_1011G301070M.fits ft971003_0520_1011G302470M.fits-> Ignoring the following files containing 000000006 events
ft971003_0520_1011G300870H.fits ft971003_0520_1011G302270H.fits ft971003_0520_1011G303970H.fits-> Ignoring the following files containing 000000005 events
ft971003_0520_1011G300770H.fits ft971003_0520_1011G302170H.fits ft971003_0520_1011G303870H.fits-> Ignoring the following files containing 000000005 events
ft971003_0520_1011G300670H.fits ft971003_0520_1011G302070H.fits ft971003_0520_1011G303770H.fits-> Ignoring the following files containing 000000003 events
ft971003_0520_1011G302770H.fits-> Ignoring the following files containing 000000002 events
ft971003_0520_1011G300470H.fits ft971003_0520_1011G301370H.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 = 5 photon cnt = 32003 SIS0SORTSPLIT:LO:s000201h.prelist merge count = 2 photon cnt = 4547 SIS0SORTSPLIT:LO:s000301h.prelist merge count = 1 photon cnt = 217 SIS0SORTSPLIT:LO:s000401l.prelist merge count = 3 photon cnt = 184 SIS0SORTSPLIT:LO:s000501m.prelist merge count = 2 photon cnt = 64 SIS0SORTSPLIT:LO:s000602h.prelist merge count = 2 photon cnt = 206 SIS0SORTSPLIT:LO:s000702l.prelist merge count = 3 photon cnt = 1751 SIS0SORTSPLIT:LO:s000802l.prelist merge count = 1 photon cnt = 48 SIS0SORTSPLIT:LO:s000902m.prelist merge count = 3 photon cnt = 1222 SIS0SORTSPLIT:LO:Total filenames split = 22 SIS0SORTSPLIT:LO:Total split file cnt = 9 SIS0SORTSPLIT:LO:End program-> Creating ad95009040s000101h.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 -- ft971003_0520_1011S000401H.fits 2 -- ft971003_0520_1011S000701H.fits 3 -- ft971003_0520_1011S001101H.fits 4 -- ft971003_0520_1011S001601H.fits 5 -- ft971003_0520_1011S002201H.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S000401H.fits 2 -- ft971003_0520_1011S000701H.fits 3 -- ft971003_0520_1011S001101H.fits 4 -- ft971003_0520_1011S001601H.fits 5 -- ft971003_0520_1011S002201H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040s000201h.unf
---- cmerge: version 1.6 ---- A total of 2 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011S001401H.fits 2 -- ft971003_0520_1011S001501H.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S001401H.fits 2 -- ft971003_0520_1011S001501H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040s000302l.unf
---- cmerge: version 1.6 ---- A total of 3 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011S000202L.fits 2 -- ft971003_0520_1011S000902L.fits 3 -- ft971003_0520_1011S002002L.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S000202L.fits 2 -- ft971003_0520_1011S000902L.fits 3 -- ft971003_0520_1011S002002L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040s000402m.unf
---- cmerge: version 1.6 ---- A total of 3 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011S000102M.fits 2 -- ft971003_0520_1011S000502M.fits 3 -- ft971003_0520_1011S001202M.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S000102M.fits 2 -- ft971003_0520_1011S000502M.fits 3 -- ft971003_0520_1011S001202M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000217 events
ft971003_0520_1011S001701H.fits-> Ignoring the following files containing 000000206 events
ft971003_0520_1011S000802H.fits ft971003_0520_1011S002302H.fits-> Ignoring the following files containing 000000184 events
ft971003_0520_1011S000301L.fits ft971003_0520_1011S001001L.fits ft971003_0520_1011S002101L.fits-> Ignoring the following files containing 000000064 events
ft971003_0520_1011S000601M.fits ft971003_0520_1011S001301M.fits-> Ignoring the following files containing 000000048 events
ft971003_0520_1011S001902L.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 = 6 photon cnt = 46423 SIS1SORTSPLIT:LO:s100201h.prelist merge count = 1 photon cnt = 256 SIS1SORTSPLIT:LO:s100301l.prelist merge count = 3 photon cnt = 184 SIS1SORTSPLIT:LO:s100401m.prelist merge count = 2 photon cnt = 64 SIS1SORTSPLIT:LO:s100502h.prelist merge count = 2 photon cnt = 415 SIS1SORTSPLIT:LO:s100602l.prelist merge count = 4 photon cnt = 4900 SIS1SORTSPLIT:LO:s100702l.prelist merge count = 1 photon cnt = 37 SIS1SORTSPLIT:LO:s100802m.prelist merge count = 4 photon cnt = 3997 SIS1SORTSPLIT:LO:Total filenames split = 23 SIS1SORTSPLIT:LO:Total split file cnt = 8 SIS1SORTSPLIT:LO:End program-> Creating ad95009040s100101h.unf
---- cmerge: version 1.6 ---- A total of 6 fits files ...... Sorting files using KEY: TSTART ... Checking GTI overlap in input files ... Merging binary extension #: 1 1 -- ft971003_0520_1011S100401H.fits 2 -- ft971003_0520_1011S100701H.fits 3 -- ft971003_0520_1011S101101H.fits 4 -- ft971003_0520_1011S101401H.fits 5 -- ft971003_0520_1011S101501H.fits 6 -- ft971003_0520_1011S102101H.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S100401H.fits 2 -- ft971003_0520_1011S100701H.fits 3 -- ft971003_0520_1011S101101H.fits 4 -- ft971003_0520_1011S101401H.fits 5 -- ft971003_0520_1011S101501H.fits 6 -- ft971003_0520_1011S102101H.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040s100202l.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 -- ft971003_0520_1011S100202L.fits 2 -- ft971003_0520_1011S100902L.fits 3 -- ft971003_0520_1011S101902L.fits 4 -- ft971003_0520_1011S102302L.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S100202L.fits 2 -- ft971003_0520_1011S100902L.fits 3 -- ft971003_0520_1011S101902L.fits 4 -- ft971003_0520_1011S102302L.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Creating ad95009040s100302m.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 -- ft971003_0520_1011S100102M.fits 2 -- ft971003_0520_1011S100502M.fits 3 -- ft971003_0520_1011S101202M.fits 4 -- ft971003_0520_1011S102402M.fits Merging binary extension #: 2 1 -- ft971003_0520_1011S100102M.fits 2 -- ft971003_0520_1011S100502M.fits 3 -- ft971003_0520_1011S101202M.fits 4 -- ft971003_0520_1011S102402M.fits Checking the output file ... Extention # 1 ...... OK Extention # 2 ...... OK The program appears to have finished successfully!-> Ignoring the following files containing 000000415 events
ft971003_0520_1011S100802H.fits ft971003_0520_1011S102202H.fits-> Ignoring the following files containing 000000256 events
ft971003_0520_1011S101601H.fits-> Ignoring the following files containing 000000184 events
ft971003_0520_1011S100301L.fits ft971003_0520_1011S101001L.fits ft971003_0520_1011S102001L.fits-> Ignoring the following files containing 000000064 events
ft971003_0520_1011S100601M.fits ft971003_0520_1011S101301M.fits-> Ignoring the following files containing 000000037 events
ft971003_0520_1011S101802L.fits-> Tar-ing together the leftover raw files
a ft971003_0520_1011G200470H.fits 31K a ft971003_0520_1011G200670H.fits 31K a ft971003_0520_1011G200770H.fits 31K a ft971003_0520_1011G200870H.fits 31K a ft971003_0520_1011G201070M.fits 31K a ft971003_0520_1011G201370H.fits 31K a ft971003_0520_1011G202170H.fits 31K a ft971003_0520_1011G202270H.fits 31K a ft971003_0520_1011G202470M.fits 31K a ft971003_0520_1011G202670H.fits 31K a ft971003_0520_1011G202770H.fits 31K a ft971003_0520_1011G203870H.fits 31K a ft971003_0520_1011G203970H.fits 31K a ft971003_0520_1011G204170L.fits 34K a ft971003_0520_1011G300470H.fits 31K a ft971003_0520_1011G300670H.fits 31K a ft971003_0520_1011G300770H.fits 31K a ft971003_0520_1011G300870H.fits 31K a ft971003_0520_1011G301070M.fits 31K a ft971003_0520_1011G301370H.fits 31K a ft971003_0520_1011G302070H.fits 31K a ft971003_0520_1011G302170H.fits 31K a ft971003_0520_1011G302270H.fits 31K a ft971003_0520_1011G302470M.fits 31K a ft971003_0520_1011G302770H.fits 31K a ft971003_0520_1011G303770H.fits 31K a ft971003_0520_1011G303870H.fits 31K a ft971003_0520_1011G303970H.fits 31K a ft971003_0520_1011G304170L.fits 34K a ft971003_0520_1011S000301L.fits 29K a ft971003_0520_1011S000601M.fits 29K a ft971003_0520_1011S000802H.fits 31K a ft971003_0520_1011S001001L.fits 31K a ft971003_0520_1011S001301M.fits 29K a ft971003_0520_1011S001701H.fits 37K a ft971003_0520_1011S001902L.fits 29K a ft971003_0520_1011S002101L.fits 29K a ft971003_0520_1011S002302H.fits 29K a ft971003_0520_1011S100301L.fits 29K a ft971003_0520_1011S100601M.fits 29K a ft971003_0520_1011S100802H.fits 31K a ft971003_0520_1011S101001L.fits 31K a ft971003_0520_1011S101301M.fits 29K a ft971003_0520_1011S101601H.fits 37K a ft971003_0520_1011S101802L.fits 29K a ft971003_0520_1011S102001L.fits 29K a ft971003_0520_1011S102202H.fits 34K-> Checking OBJECT keywords in HK and event files
temp2gain v4.3 'ft971003_0520.1011' is successfully opened Data Start Time is 150009658.40 (19971003 052054) Time Margin 2.0 sec included 'ft971003_0520.1011' EOF detected, sf=4766 Data End Time is 150027086.34 (19971003 101122) Gain History is written in ft971003_0520_1011.ghf-> Stdout output from ISAS program temp2gain
leapsec FITS data was successfully read-> Checking if column CAL_START in ft971003_0520_1011.ghf[1] is in order
Time column is TIME ORDERED-> Checking if column CAL_STOP in ft971003_0520_1011.ghf[1] is in order
Time column is TIME ORDERED-> Calculating attitude correction from ft971003_0520_1011CMHK.fits
The sum of the selected column is 10639.000 The mean of the selected column is 92.513043 The standard deviation of the selected column is 1.3069666 The minimum of selected column is 90.000000 The maximum of selected column is 94.000000 The number of points used in calculation is 115-> Standard Output From FTOOL fstatistic:
The sum of the selected column is 10639.000 The mean of the selected column is 92.513043 The standard deviation of the selected column is 1.3069666 The minimum of selected column is 90.000000 The maximum of selected column is 94.000000 The number of points used in calculation is 115
ASCALIN_V0.9u(mod)-> Checking if ad95009040g200270m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040g200370l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040g300170h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040g300270m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040g300370l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000101h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000102h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000112h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000201h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000202h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000212h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000302l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s000402m.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s100101h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s100102h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s100112h.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s100202l.unf is covered by attitude file
ASCALIN_V0.9u(mod)-> Checking if ad95009040s100302m.unf is covered by attitude file
ASCALIN_V0.9u(mod)
S0-HK file: ft971003_0520_1011S0HK.fits
S1-HK file: ft971003_0520_1011S1HK.fits
G2-HK file: ft971003_0520_1011G2HK.fits
G3-HK file: ft971003_0520_1011G3HK.fits
Date and time are: 1997-10-03 05:20:28 mjd=50724.222551
Orbit file name is ./frf.orbit.241
Epoch of Orbital Elements: 1997-09-29 20:00:00
Rigidity Data File: ./rigidity.data.1.23
Attitude FRF: fa971003_0520.1011
output FITS File: ft971003_0520_1011.mkf
mkfilter2: Warning, faQparam error: time= 1.500095804008e+08 outside range of attitude file
Euler angles undefined for this bin
mkfilter2: Warning, faQparam error: time= 1.500096124008e+08 outside range of attitude file
Euler angles undefined for this bin
Total 548 Data bins were processed.
-> Checking if column TIME in ft971003_0520_1011.mkf is in orderTime column is TIME ORDERED-> Calculating dead time values for filter file
The sum of the selected column is 2194.8424 The mean of the selected column is 22.862942 The standard deviation of the selected column is 11.709123 The minimum of selected column is 7.6875262 The maximum of selected column is 64.437721 The number of points used in calculation is 96-> 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<57.9 ) ) &&( (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 ad95009040s000112h.unf into ad95009040s000112h.evt
The sum of the selected column is 2194.8424 The mean of the selected column is 22.862942 The standard deviation of the selected column is 11.709123 The minimum of selected column is 7.6875262 The maximum of selected column is 64.437721 The number of points used in calculation is 96-> 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<57.9 ) ) &&( (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 ad95009040s000201h.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_PIXL0>0)&&(S0_PIXL3>0) )&&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&((T_DY_NT<0)||(T_DY_NT>32)) &&((T_SAA <0)||(T_SAA >32))-> Filtering ad95009040s000212h.unf into ad95009040s000212h.evt
(SAA==0) &&(BR_EARTH>20) &&(ELV>10) &&(COR>6) &&(ACS==0) &&(ANG_DIST>0)&& (ANG_DIST<0.01) &&(FOV==0) && ( (S0_PIXL0>0)&&(S0_PIXL3>0) )&&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&( (S0_SATF3<1) ||(S0_SATF3>1)) &&( (S0_SATF0<1) ||(S0_SATF0>1)) &&((T_DY_NT<0)||(T_DY_NT>32)) &&((T_SAA <0)||(T_SAA >32))-> Filtering ad95009040s000302l.unf into ad95009040s000302l.evt
(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 ad95009040s000302l.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 ad95009040s000402m.evt since it contains 0 events
The sum of the selected column is 3613.0208 The mean of the selected column is 36.867560 The standard deviation of the selected column is 19.193180 The minimum of selected column is 12.375042 The maximum of selected column is 116.59415 The number of points used in calculation is 98-> 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<94.4 ) ) &&( (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 ad95009040s100112h.unf into ad95009040s100112h.evt
The sum of the selected column is 3613.0208 The mean of the selected column is 36.867560 The standard deviation of the selected column is 19.193180 The minimum of selected column is 12.375042 The maximum of selected column is 116.59415 The number of points used in calculation is 98-> 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<94.4 ) ) &&( (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 ad95009040s100202l.unf into ad95009040s100202l.evt
(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 ad95009040s100202l.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 ad95009040s100302m.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 ad95009040g200270m.unf into ad95009040g200270m.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 ad95009040g200270m.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)-> Deleting ad95009040g200370l.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 ad95009040g300270m.unf into ad95009040g300270m.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 ad95009040g300270m.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)-> Deleting ad95009040g300370l.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: ad95009040g200170h.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: ./fa971003_0520.1011
making an exposure map...
Aspect RA/DEC/ROLL : 122.2380 -38.3816 280.9401
Mean RA/DEC/ROLL : 122.2317 -38.3993 280.9401
Pnt RA/DEC/ROLL : 122.2413 -38.3599 280.9401
Image rebin factor : 1
Attitude Records : 19031
GTI intervals : 12
Total GTI (secs) : 3646.027
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 573.49 573.49
20 Percent Complete: Total/live time: 1492.00 1492.00
30 Percent Complete: Total/live time: 1492.00 1492.00
40 Percent Complete: Total/live time: 1564.98 1564.98
50 Percent Complete: Total/live time: 2484.00 2484.00
60 Percent Complete: Total/live time: 2484.00 2484.00
70 Percent Complete: Total/live time: 2656.44 2656.44
80 Percent Complete: Total/live time: 3303.97 3303.97
90 Percent Complete: Total/live time: 3326.03 3326.03
100 Percent Complete: Total/live time: 3646.03 3646.03
Number of attitude steps used: 14
Number of attitude steps avail: 12517
Mean RA/DEC pixel offset: -7.5095 -3.7706
writing expo file: ad95009040g200170h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad95009040g200170h.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: ad95009040g300170h.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: ./fa971003_0520.1011
making an exposure map...
Aspect RA/DEC/ROLL : 122.2380 -38.3816 280.9420
Mean RA/DEC/ROLL : 122.2288 -38.3746 280.9420
Pnt RA/DEC/ROLL : 122.2443 -38.3846 280.9420
Image rebin factor : 1
Attitude Records : 19031
GTI intervals : 12
Total GTI (secs) : 3642.027
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 573.49 573.49
20 Percent Complete: Total/live time: 1490.00 1490.00
30 Percent Complete: Total/live time: 1490.00 1490.00
40 Percent Complete: Total/live time: 1562.98 1562.98
50 Percent Complete: Total/live time: 2482.00 2482.00
60 Percent Complete: Total/live time: 2482.00 2482.00
70 Percent Complete: Total/live time: 2654.44 2654.44
80 Percent Complete: Total/live time: 3301.97 3301.97
90 Percent Complete: Total/live time: 3322.03 3322.03
100 Percent Complete: Total/live time: 3642.03 3642.03
Number of attitude steps used: 14
Number of attitude steps avail: 12513
Mean RA/DEC pixel offset: 3.9798 -2.8785
writing expo file: ad95009040g300170h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad95009040g300170h.evt
ASCAEXPO_V0.9b
reading data file: ad95009040s000102h.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: ./fa971003_0520.1011
making an exposure map...
Aspect RA/DEC/ROLL : 122.2380 -38.3816 280.9529
Mean RA/DEC/ROLL : 122.2109 -38.3898 280.9529
Pnt RA/DEC/ROLL : 122.2617 -38.3698 280.9529
Image rebin factor : 4
Attitude Records : 19031
Hot Pixels : 8
GTI intervals : 14
Total GTI (secs) : 3280.172
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 700.99 700.99
20 Percent Complete: Total/live time: 700.99 700.99
30 Percent Complete: Total/live time: 1560.00 1560.00
40 Percent Complete: Total/live time: 1560.00 1560.00
50 Percent Complete: Total/live time: 1822.47 1822.47
60 Percent Complete: Total/live time: 2168.00 2168.00
70 Percent Complete: Total/live time: 2360.00 2360.00
80 Percent Complete: Total/live time: 2906.12 2906.12
90 Percent Complete: Total/live time: 3184.62 3184.62
100 Percent Complete: Total/live time: 3280.17 3280.17
Number of attitude steps used: 13
Number of attitude steps avail: 11899
Mean RA/DEC pixel offset: -16.7461 -93.3242
writing expo file: ad95009040s000102h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad95009040s000102h.evt
ASCAEXPO_V0.9b
reading data file: ad95009040s100102h.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: ./fa971003_0520.1011
making an exposure map...
Aspect RA/DEC/ROLL : 122.2380 -38.3816 280.9404
Mean RA/DEC/ROLL : 122.2310 -38.3877 280.9404
Pnt RA/DEC/ROLL : 122.2416 -38.3718 280.9404
Image rebin factor : 4
Attitude Records : 19031
Hot Pixels : 12
GTI intervals : 11
Total GTI (secs) : 3288.172
Max attitude excursion (arcsecs) : 5.000
0 Percent Complete: Total/live time: 0.00 0.00
10 Percent Complete: Total/live time: 704.99 704.99
20 Percent Complete: Total/live time: 704.99 704.99
30 Percent Complete: Total/live time: 1600.00 1600.00
40 Percent Complete: Total/live time: 1600.00 1600.00
50 Percent Complete: Total/live time: 1862.47 1862.47
60 Percent Complete: Total/live time: 2208.00 2208.00
70 Percent Complete: Total/live time: 2400.00 2400.00
80 Percent Complete: Total/live time: 2946.12 2946.12
90 Percent Complete: Total/live time: 3224.62 3224.62
100 Percent Complete: Total/live time: 3288.17 3288.17
Number of attitude steps used: 13
Number of attitude steps avail: 11835
Mean RA/DEC pixel offset: -20.8313 -26.9988
writing expo file: ad95009040s100102h.expo
closing attitude file...
closing data file...
-> Generating low and high energy images for ad95009040s100102h.evtad95009040s000102h.expo ad95009040s100102h.expo-> Summing the following images to produce ad95009040sis32002_all.totsky
ad95009040s000102h.img ad95009040s100102h.img-> Summing the following images to produce ad95009040sis32002_lo.totsky
ad95009040s000102h_lo.img ad95009040s100102h_lo.img-> Summing the following images to produce ad95009040sis32002_hi.totsky
ad95009040s000102h_hi.img ad95009040s100102h_hi.img-> Running XIMAGE to create ad95009040sis32002.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad95009040sis32002_all.totsky Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 4.00000 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 4 min: 0 ![2]XIMAGE> read/exp_map ad95009040sis32002.totexpo Reading an image Telescope ASCA SIS0 Image display size = 320 Done, closing file Largest, Smallest 109.472 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 109 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "C-HALE-BOPP_N5" ![7]XIMAGE> title/lower "ASCA SIS0,SIS1 October 3, 1997 Exposure: 6568.3 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 205 ![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 9.00000 90 -1 i,inten,mm,pp 4 16.0000 16 0 ![11]XIMAGE> exit-> Summing gis images
ad95009040g200170h.expo ad95009040g300170h.expo-> Summing the following images to produce ad95009040gis25670_all.totsky
ad95009040g200170h.img ad95009040g300170h.img-> Summing the following images to produce ad95009040gis25670_lo.totsky
ad95009040g200170h_lo.img ad95009040g300170h_lo.img-> Summing the following images to produce ad95009040gis25670_hi.totsky
ad95009040g200170h_hi.img ad95009040g300170h_hi.img-> Running XIMAGE to create ad95009040gis25670.gif
No of detectors read in: 20 ![1]XIMAGE> read/fits ad95009040gis25670_all.totsky Reading an image Telescope ASCA GIS2 Image display size = 256 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 ad95009040gis25670.totexpo Reading an image Telescope ASCA GIS2 Image display size = 256 Done, closing file Largest, Smallest 121.468 0. Bscale, Bzero from file 1.0000000000000 0. After internal scaling Bscale and Bzero 1.0000000000000 0. Image level, max: 121 min: 0 ![3]XIMAGE> smooth ![4]XIMAGE> cpd /ppm ![5]XIMAGE> cey 2000 ![6]XIMAGE> title "C-HALE-BOPP_N5" ![7]XIMAGE> title/lower "ASCA GIS2,GIS3 October 3, 1997 Exposure: 7288 s" ![8]XIMAGE> disp/correct/noframe Displaying image The image is exposure corrected Min = 0 max = 29566 ![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 10.00000 100 -1 i,inten,mm,pp 4 52.0000 52 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: ad95009040gis25670.src
-> Standard Output From STOOL colorpic:
color plane 0 color plane 1 color plane 2 writing image image written-> Creating fits catalog of sources: ad95009040sis32002.src
1 ad95009040s000102h.evt 128-> Standard Output From STOOL group_event_files:
1 ad95009040s000112h.evt 147-> Standard Output From STOOL group_event_files:
1 ad95009040s100102h.evt 158-> Standard Output From STOOL group_event_files:
1 ad95009040s100112h.evt 181-> Standard Output From STOOL group_event_files:
1 ad95009040g200170h.evt 894-> GIS2_REGION256.4 already present in current directory
ad95009040g200170h.evt-> Correcting ad95009040g210170_0.pi for dead time
... read all the files from deadlist.tmp-> Grouping ad95009040g210170_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 - 3646.0 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 - 27 are grouped by a factor 28 ... 28 - 46 are grouped by a factor 19 ... 47 - 68 are grouped by a factor 22 ... 69 - 83 are grouped by a factor 15 ... 84 - 95 are grouped by a factor 12 ... 96 - 111 are grouped by a factor 16 ... 112 - 129 are grouped by a factor 18 ... 130 - 145 are grouped by a factor 16 ... 146 - 162 are grouped by a factor 17 ... 163 - 185 are grouped by a factor 23 ... 186 - 212 are grouped by a factor 27 ... 213 - 232 are grouped by a factor 20 ... 233 - 263 are grouped by a factor 31 ... 264 - 304 are grouped by a factor 41 ... 305 - 342 are grouped by a factor 38 ... 343 - 401 are grouped by a factor 59 ... 402 - 454 are grouped by a factor 53 ... 455 - 525 are grouped by a factor 71 ... 526 - 628 are grouped by a factor 103 ... 629 - 726 are grouped by a factor 98 ... 727 - 881 are grouped by a factor 155 ... 882 - 1023 of undefined grouping (Channel quality=bad) ... --------------------------------------------- ... ...... exiting, changes written to file : ad95009040g210170_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 = 8.94000E+02
Weighted mean angle from optical axis = 14.658 arcmin
-> Standard Output From STOOL group_event_files:1 ad95009040g300170h.evt 880-> GIS3_REGION256.4 already present in current directory
ad95009040g300170h.evt-> Correcting ad95009040g310170_0.pi for dead time
... read all the files from deadlist.tmp-> Grouping ad95009040g310170_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 - 3642.0 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 - 26 are grouped by a factor 27 ... 27 - 42 are grouped by a factor 16 ... 43 - 68 are grouped by a factor 26 ... 69 - 82 are grouped by a factor 14 ... 83 - 97 are grouped by a factor 15 ... 98 - 133 are grouped by a factor 18 ... 134 - 147 are grouped by a factor 14 ... 148 - 167 are grouped by a factor 20 ... 168 - 186 are grouped by a factor 19 ... 187 - 211 are grouped by a factor 25 ... 212 - 244 are grouped by a factor 33 ... 245 - 272 are grouped by a factor 28 ... 273 - 305 are grouped by a factor 33 ... 306 - 340 are grouped by a factor 35 ... 341 - 380 are grouped by a factor 40 ... 381 - 440 are grouped by a factor 60 ... 441 - 515 are grouped by a factor 75 ... 516 - 612 are grouped by a factor 97 ... 613 - 711 are grouped by a factor 99 ... 712 - 883 are grouped by a factor 172 ... 884 - 1023 of undefined grouping (Channel quality=bad) ... --------------------------------------------- ... ...... exiting, changes written to file : ad95009040g310170_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 = 8.80000E+02
Weighted mean angle from optical axis = 14.272 arcmin
-> Plotting ad95009040g210170_0_pi.ps from ad95009040g210170_0.pi
XSPEC 9.01 05:08:58 5-Jan-00
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> data ad95009040g210170_0.pi
Net count rate (cts/s) for file 1 0.2452 +/- 8.6992E-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 ad95009040g310170_0_pi.ps from ad95009040g310170_0.pi
XSPEC 9.01 05:09:12 5-Jan-00
Plot device not set, use "cpd" to set it
Type "help" or "?" for further information
!XSPEC> data ad95009040g310170_0.pi
Net count rate (cts/s) for file 1 0.2416 +/- 8.6871E-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]=> ad95009040g200070_0.lc
Selected FITS extensions: 1 - RATE TABLE;
Source ............ C-HALE-BOPP_N5 Start Time (d) .... 10724 05:55:40.401
FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10724 10:03:40.401
No. of Rows ....... 19 Bin Time (s) ...... 203.9
Right Ascension ... 1.2224E+02 Internal time sys.. Converted to TJD
Declination ....... -3.8382E+01 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 73 Newbins of 203.917 (s)
Intv 1 Start10724 5:57:22
Ser.1 Avg 0.2439 Chisq 18.03 Var 0.1318E-02 Newbs. 19
Min 0.1716 Max 0.3242 expVar 0.1389E-02 Bins 19
Results from Statistical Analysis
Newbin Integration Time (s).. 203.92
Interval Duration (s)........ 14682.
No. of Newbins .............. 19
Average (c/s) ............... 0.24393 +/- 0.88E-02
Standard Deviation (c/s)..... 0.36304E-01
Minimum (c/s)................ 0.17164
Maximum (c/s)................ 0.32418
Variance ((c/s)**2).......... 0.13180E-02 +/- 0.44E-03
Expected Variance ((c/s)**2). 0.13890E-02 +/- 0.46E-03
Third Moment ((c/s)**3)...... 0.89918E-05
Average Deviation (c/s)...... 0.27921E-01
Skewness..................... 0.18792 +/- 0.56
Kurtosis.....................-0.12298 +/- 1.1
RMS fractional variation....< 0.17756 (3 sigma)
Chi-Square................... 18.029 dof 18
Chi-Square Prob of constancy. 0.45365 (0 means < 1.e-38)
Kolm.-Smir. Prob of constancy 0.30675 (0 means < 1.e-38)
[4]xronos> [5]xronos>
Maximum of 1 Intvs. with 73 Newbins of 203.917 (s)
Intv 1 Start10724 5:57:22
Ser.1 Avg 0.2439 Chisq 18.03 Var 0.1318E-02 Newbs. 19
Min 0.1716 Max 0.3242 expVar 0.1389E-02 Bins 19
Light curve ready !
Frme 1 Written to output file : xronos.qlc1
PLT> LA File ad95009040g200070_0.lc
PLT> hard /ps
PLT> [6]xronos>
-> TIMEDEL=6.2500000000E-02 for ad95009040g300170h.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]=> ad95009040g300070_0.lc
Selected FITS extensions: 1 - RATE TABLE;
Source ............ C-HALE-BOPP_N5 Start Time (d) .... 10724 05:55:40.401
FITS Extension .... 1 - `RATE ` Stop Time (d) ..... 10724 10:03:40.401
No. of Rows ....... 17 Bin Time (s) ...... 206.9
Right Ascension ... 1.2224E+02 Internal time sys.. Converted to TJD
Declination ....... -3.8382E+01 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 72 Newbins of 206.933 (s)
Intv 1 Start10724 5:57:23
Ser.1 Avg 0.2364 Chisq 13.48 Var 0.9938E-03 Newbs. 17
Min 0.1836 Max 0.3024 expVar 0.1254E-02 Bins 17
Results from Statistical Analysis
Newbin Integration Time (s).. 206.93
Interval Duration (s)........ 14692.
No. of Newbins .............. 17
Average (c/s) ............... 0.23643 +/- 0.89E-02
Standard Deviation (c/s)..... 0.31525E-01
Minimum (c/s)................ 0.18363
Maximum (c/s)................ 0.30242
Variance ((c/s)**2).......... 0.99380E-03 +/- 0.35E-03
Expected Variance ((c/s)**2). 0.12535E-02 +/- 0.44E-03
Third Moment ((c/s)**3)...... 0.15867E-05
Average Deviation (c/s)...... 0.26250E-01
Skewness..................... 0.50647E-01 +/- 0.59
Kurtosis.....................-0.55576 +/- 1.2
RMS fractional variation....< 0.18970 (3 sigma)
Chi-Square................... 13.478 dof 16
Chi-Square Prob of constancy. 0.63752 (0 means < 1.e-38)
Kolm.-Smir. Prob of constancy 0.47964 (0 means < 1.e-38)
[4]xronos> [5]xronos>
Maximum of 1 Intvs. with 72 Newbins of 206.933 (s)
Intv 1 Start10724 5:57:23
Ser.1 Avg 0.2364 Chisq 13.48 Var 0.9938E-03 Newbs. 17
Min 0.1836 Max 0.3024 expVar 0.1254E-02 Bins 17
Light curve ready !
Frme 1 Written to output file : xronos.qlc1
PLT> LA File ad95009040g300070_0.lc
PLT> hard /ps
PLT> [6]xronos>
-> Merging GTIs from the following files:ad95009040g200170h.evt[2]-> Making L1 light curve of ft971003_0520_1011G2HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 7552 output records from 7564 good input G2_L1 records.-> Making L1 light curve of ft971003_0520_1011G2HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 3269 output records from 7564 good input G2_L1 records.-> Merging GTIs from the following files:
ad95009040g300170h.evt[2]-> Making L1 light curve of ft971003_0520_1011G3HK.fits with irate=HIGH
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 6859 output records from 6871 good input G3_L1 records.-> Making L1 light curve of ft971003_0520_1011G3HK.fits with irate=HI+MED
ghkcurve: ALLGTI found in input HK file, will be applied to data. ghkcurve: 3168 output records from 6871 good input G3_L1 records.
*** tlmFrm Version 1.1 (1997-08-25) ***
total number of superframes: 4766
frame data: 150021820.359643 ---> 150021964.359166
S0, C3, 2 ccd mode; Output File = fr971003_0520.1011_s0c3m2a.fits
frame data: 150021984.3591 ---> 150022128.358623
S0, C0, 2 ccd mode; Output File = fr971003_0520.1011_s0c0m2a.fits
frame data: 150022148.358557 ---> 150022292.358084
S0, C3, 2 ccd mode; Output File = fr971003_0520.1011_s0c3m2b.fits
frame data: 150022312.358018 ---> 150022456.357545
S0, C0, 2 ccd mode; Output File = fr971003_0520.1011_s0c0m2b.fits
Total of 4 sets of frame data are extracted.
-> Processing fr971003_0520.1011_s0c0m2a.fitsDark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971003_0520.1011_s0c0m2a.fits Output zero level image : rdd.tmp Bias level = 341-> Adding keywords to header of fr971003_0520.1011_s0c0m2a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971003_0520.1011_s0c0m2b.fits Output zero level image : rdd.tmp Bias level = 340-> Adding keywords to header of fr971003_0520.1011_s0c0m2b.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971003_0520.1011_s0c3m2a.fits Output zero level image : rdd.tmp Bias level = 321-> Adding keywords to header of fr971003_0520.1011_s0c3m2a.fits
Dark upper (ADU) : 40 Dark lower (ADU) : -40 Input frame data : fr971003_0520.1011_s0c3m2b.fits Output zero level image : rdd.tmp Bias level = 321-> Adding keywords to header of fr971003_0520.1011_s0c3m2b.fits
SUNSHINE==0 && T_DY_NT>64 && T_SAA>64 && SAA==0 && COR>6 && (ELV>10 || ELV<10 )-> Extracting GTIs from ft971003_0520_1011.mkf
1 ad95009040g200170h.unf 8618 1 ad95009040g200270m.unf 8618 1 ad95009040g200370l.unf 8618-> Fetching GIS2_CALSRC256.2
XSPEC 9.01 05:20:32 5-Jan-00
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 ad95009040g220170.cal
Net count rate (cts/s) for file 1 0.1526 +/- 3.8138E-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 = 4.6463E+05 using 84 PHA bins.
Reduced chi-squared = 6034.
!XSPEC> newpar 5 = 2 1.101005
6 variable fit parameters
Chi-Squared = 4.6127E+05 using 84 PHA bins.
Reduced chi-squared = 5914.
!XSPEC> newpar 6 = 3 1.049288
5 variable fit parameters
Chi-Squared = 4.6127E+05 using 84 PHA bins.
Reduced chi-squared = 5839.
!XSPEC> renorm
Chi-Squared = 414.0 using 84 PHA bins.
Reduced chi-squared = 5.240
!XSPEC> fit
Chi-Squared Lvl Fit param # 1 2 3 4
5
Due to zero model norms
fit parameter 1 is temporarily frozen
327.49 0 1.000 5.894 0.1079 4.5277E-02
4.0731E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
181.83 0 1.000 5.876 0.1585 6.2476E-02
3.6349E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
92.479 -1 1.000 5.950 0.1806 8.7251E-02
2.3665E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
81.621 -2 1.000 6.005 0.2047 0.1015
1.4542E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
79.590 -3 1.000 5.977 0.1815 9.6544E-02
1.9367E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
79.047 -4 1.000 5.990 0.1915 9.9255E-02
1.6599E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
78.872 -5 1.000 5.984 0.1858 9.7978E-02
1.7841E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
78.865 -6 1.000 5.987 0.1884 9.8603E-02
1.7216E-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 5.98707 +/- 0.14702E-01
3 3 2 gaussian/b Sigma 0.188364 +/- 0.15542E-01
4 4 2 gaussian/b norm 9.860315E-02 +/- 0.38642E-02
5 2 3 gaussian/b LineE 6.59179 = par 2 * 1.1010
6 3 3 gaussian/b Sigma 0.197648 = par 3 * 1.0493
7 5 3 gaussian/b norm 1.721615E-02 +/- 0.26747E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
Chi-Squared = 78.86 using 84 PHA bins.
Reduced chi-squared = 0.9983
!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 ad95009040g220170.cal peaks at 5.98707 +/- 0.014702 keV1 ad95009040g300170h.unf 7809 1 ad95009040g300270m.unf 7809 1 ad95009040g300370l.unf 7809-> Fetching GIS3_CALSRC256.2
XSPEC 9.01 05:21:25 5-Jan-00
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 ad95009040g320170.cal
Net count rate (cts/s) for file 1 0.1322 +/- 3.5829E-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 = 6.5799E+05 using 84 PHA bins.
Reduced chi-squared = 8545.
!XSPEC> newpar 5 = 2 1.101005
6 variable fit parameters
Chi-Squared = 6.5431E+05 using 84 PHA bins.
Reduced chi-squared = 8389.
!XSPEC> newpar 6 = 3 1.049288
5 variable fit parameters
Chi-Squared = 6.5431E+05 using 84 PHA bins.
Reduced chi-squared = 8282.
!XSPEC> renorm
Chi-Squared = 542.5 using 84 PHA bins.
Reduced chi-squared = 6.867
!XSPEC> fit
Chi-Squared Lvl Fit param # 1 2 3 4
5
Due to zero model norms
fit parameter 1 is temporarily frozen
412.82 0 1.000 5.893 0.1495 3.4791E-02
2.9185E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
196.86 0 1.000 5.867 0.1882 5.8207E-02
2.5301E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
96.431 -1 1.000 5.958 0.1929 8.9346E-02
1.1725E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
88.614 -2 1.000 5.916 0.1447 8.8233E-02
1.6215E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
85.808 -3 1.000 5.944 0.1667 9.3096E-02
1.1481E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.808 -4 1.000 5.927 0.1474 9.0111E-02
1.4309E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.403 -5 1.000 5.938 0.1575 9.1990E-02
1.2407E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.218 -6 1.000 5.932 0.1503 9.0855E-02
1.3506E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.177 -7 1.000 5.936 0.1543 9.1552E-02
1.2809E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.143 -8 1.000 5.934 0.1517 9.1131E-02
1.3222E-02
Number of trials exceeded - last iteration delta = 3.4393E-02
Due to zero model norms
fit parameter 1 is temporarily frozen
84.142 -9 1.000 5.935 0.1533 9.1388E-02
1.2967E-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 5.93505 +/- 0.12091E-01
3 3 2 gaussian/b Sigma 0.153262 +/- 0.15832E-01
4 4 2 gaussian/b norm 9.138766E-02 +/- 0.34367E-02
5 2 3 gaussian/b LineE 6.53452 = par 2 * 1.1010
6 3 3 gaussian/b Sigma 0.160816 = par 3 * 1.0493
7 5 3 gaussian/b norm 1.296743E-02 +/- 0.20666E-02
---------------------------------------------------------------------------
---------------------------------------------------------------------------
Chi-Squared = 84.14 using 84 PHA bins.
Reduced chi-squared = 1.065
!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 ad95009040g320170.cal peaks at 5.93505 +/- 0.012091 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: ad95009040s000102h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 207
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 3 176
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 3
Number of (internal) image counts : 207
Number of image cts rejected (N, %) : 17685.02
By chip : 0 1 2 3
Pixels rejected : 0 3 0 0
Image counts : 0 207 0 0
Image cts rejected: 0 176 0 0
Image cts rej (%) : 0.00 85.02 0.00 0.00
filtering data...
Total counts : 0 207 0 0
Total cts rejected: 0 176 0 0
Total cts rej (%) : 0.00 85.02 0.00 0.00
Number of clean counts accepted : 31
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 3
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s000112h.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: ad95009040s000112h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 215
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 3 176
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 3
Number of (internal) image counts : 215
Number of image cts rejected (N, %) : 17681.86
By chip : 0 1 2 3
Pixels rejected : 0 3 0 0
Image counts : 0 215 0 0
Image cts rejected: 0 176 0 0
Image cts rej (%) : 0.00 81.86 0.00 0.00
filtering data...
Total counts : 0 215 0 0
Total cts rejected: 0 176 0 0
Total cts rej (%) : 0.00 81.86 0.00 0.00
Number of clean counts accepted : 39
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 3
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s000202h.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: ad95009040s000202h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3329
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 63 1398
Flickering pixels iter, pixels & cnts : 1 59 414
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 36 690
Flickering pixels iter, pixels & cnts : 1 48 230
Number of pixels rejected : 206
Number of (internal) image counts : 3329
Number of image cts rejected (N, %) : 273282.07
By chip : 0 1 2 3
Pixels rejected : 122 0 0 84
Image counts : 2132 0 0 1197
Image cts rejected: 1812 0 0 920
Image cts rej (%) : 84.99 0.00 0.00 76.86
filtering data...
Total counts : 2132 0 0 1197
Total cts rejected: 1812 0 0 920
Total cts rej (%) : 84.99 0.00 0.00 76.86
Number of clean counts accepted : 597
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 206
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s000212h.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: ad95009040s000212h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 3370
copy bad pix array...
cleaning chip # 0
Hot pixels & counts : 63 1399
Flickering pixels iter, pixels & cnts : 1 59 414
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 36 693
Flickering pixels iter, pixels & cnts : 1 49 233
Number of pixels rejected : 207
Number of (internal) image counts : 3370
Number of image cts rejected (N, %) : 273981.28
By chip : 0 1 2 3
Pixels rejected : 122 0 0 85
Image counts : 2146 0 0 1224
Image cts rejected: 1813 0 0 926
Image cts rej (%) : 84.48 0.00 0.00 75.65
filtering data...
Total counts : 2146 0 0 1224
Total cts rejected: 1813 0 0 926
Total cts rej (%) : 84.48 0.00 0.00 75.65
Number of clean counts accepted : 631
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 207
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s000302l.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: ad95009040s000302l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 714
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 5 614
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 5
Number of (internal) image counts : 714
Number of image cts rejected (N, %) : 61485.99
By chip : 0 1 2 3
Pixels rejected : 0 5 0 0
Image counts : 0 714 0 0
Image cts rejected: 0 614 0 0
Image cts rej (%) : 0.00 85.99 0.00 0.00
filtering data...
Total counts : 0 714 0 0
Total cts rejected: 0 614 0 0
Total cts rej (%) : 0.00 85.99 0.00 0.00
Number of clean counts accepted : 100
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 5
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s000402m.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: ad95009040s000402m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 987
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
Hot pixels & counts : 5 891
cleaning chip # 2
cleaning chip # 3
Number of pixels rejected : 5
Number of (internal) image counts : 987
Number of image cts rejected (N, %) : 89190.27
By chip : 0 1 2 3
Pixels rejected : 0 5 0 0
Image counts : 0 987 0 0
Image cts rejected: 0 891 0 0
Image cts rej (%) : 0.00 90.27 0.00 0.00
filtering data...
Total counts : 0 987 0 0
Total cts rejected: 0 891 0 0
Total cts rej (%) : 0.00 90.27 0.00 0.00
Number of clean counts accepted : 96
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 5
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s100102h.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: ad95009040s100102h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 1046
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 9 999
Flickering pixels iter, pixels & cnts : 1 1 8
Number of pixels rejected : 10
Number of (internal) image counts : 1046
Number of image cts rejected (N, %) : 100796.27
By chip : 0 1 2 3
Pixels rejected : 0 0 0 10
Image counts : 0 0 0 1046
Image cts rejected: 0 0 0 1007
Image cts rej (%) : 0.00 0.00 0.00 96.27
filtering data...
Total counts : 0 0 0 1046
Total cts rejected: 0 0 0 1007
Total cts rej (%) : 0.00 0.00 0.00 96.27
Number of clean counts accepted : 39
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 10
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s100112h.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: ad95009040s100112h.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 1052
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 9 999
Flickering pixels iter, pixels & cnts : 1 1 8
Number of pixels rejected : 10
Number of (internal) image counts : 1052
Number of image cts rejected (N, %) : 100795.72
By chip : 0 1 2 3
Pixels rejected : 0 0 0 10
Image counts : 0 0 0 1052
Image cts rejected: 0 0 0 1007
Image cts rej (%) : 0.00 0.00 0.00 95.72
filtering data...
Total counts : 0 0 0 1052
Total cts rejected: 0 0 0 1007
Total cts rej (%) : 0.00 0.00 0.00 95.72
Number of clean counts accepted : 45
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 10
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s100202l.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: ad95009040s100202l.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 1994
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 9 1916
Flickering pixels iter, pixels & cnts : 1 1 7
Number of pixels rejected : 10
Number of (internal) image counts : 1994
Number of image cts rejected (N, %) : 192396.44
By chip : 0 1 2 3
Pixels rejected : 0 0 0 10
Image counts : 0 0 0 1994
Image cts rejected: 0 0 0 1923
Image cts rej (%) : 0.00 0.00 0.00 96.44
filtering data...
Total counts : 0 0 0 1994
Total cts rejected: 0 0 0 1923
Total cts rej (%) : 0.00 0.00 0.00 96.44
Number of clean counts accepted : 71
writing history cards...
copying extensions...
writing out hot pixs...
Number of rejected pixels : 10
updating NEVENTS keywords...
closing data file...
closing clean file...
-> Extracting bright and dark Earth events from ad95009040s100302m.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: ad95009040s100302m.drk
reading data file: event.tmp
copying primary header to output file...
making chip image...
Total counts in chip images : 2829
copy bad pix array...
cleaning chip # 0
cleaning chip # 1
cleaning chip # 2
cleaning chip # 3
Hot pixels & counts : 9 2709
Flickering pixels iter, pixels & cnts : 1 2 11
Number of pixels rejected : 11
Number of (internal) image counts : 2829
Number of image cts rejected (N, %) : 272096.15
By chip : 0 1 2 3
Pixels rejected : 0 0 0 11
Image counts : 0 0 0 2829
Image cts rejected: 0 0 0 2720
Image cts rej (%) : 0.00 0.00 0.00 96.15
filtering data...
Total counts : 0 0 0 2829
Total cts rejected: 0 0 0 2720
Total cts rej (%) : 0.00 0.00 0.00 96.15
Number of clean counts accepted : 109
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 ad95009040g200170h.unfOffset of 213408004.000000 from 1993-01-01 00:00:00 is date and time (including leapseconds) = 1999-10-07 00:00:00.00000 Modified Julian Day = 51458.000000000000000-> 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
ad95009040s000102h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000202h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000102h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000202h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000102h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad95009040s000202h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad95009040s000102h.unf
ad95009040s000112h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000212h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000112h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000212h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000112h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad95009040s000212h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad95009040s000112h.unf
ad95009040s000101h.unf|S0CCDPOW|0100|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000201h.unf|S0CCDPOW|1001|Which S0 CCDs are in use(0123): 0=OFF 1=ON ad95009040s000101h.unf|S0CCDMOD|1|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000201h.unf|S0CCDMOD|2|How many S0 CCDs are in use: 1, 2, or 4 ad95009040s000101h.unf|S0CCDLST|1 1 1 1|S0 CCD readout order ad95009040s000201h.unf|S0CCDLST|3 0 3 0|S0 CCD readout order-> listing ad95009040s000101h.unf
29 704 1903 612 3850 718 2
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Checksum keywords updated successfully.-> Doing inventory of all files