Suzaku Observation : 108003020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '108003020' / Observation identification string
OBSERVER= 'MASAHIRO TSUJIMOTO' / Principal Investigator
OBJECT = 'E0102-72_1_4_WIN' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 16.0083 / planned target R.A.(deg)
DEC_OBJ = -72.0313 / planned target DEC.(deg)
RA_NOM = 1.598250000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -7.203030000000000E+01 / Declination of target (deci. deg)
PA_NOM = 171.8498 / nominal position angle from north to DETY(deg)
MEAN_EA1= 15.982484040984 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 162.030299574800 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 278.150239735198 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-09-29T11:39:14' / Start date of observations
DATE-END= '2013-09-30T09:45:13' / End date of observations
TSTART = 4.337713075784768E+08 / time start
TSTOP = 4.338490940000000E+08 / time stop
TELAPSE = 7.778642152321339E+04 / elapsed time
ONTIME = 3.361286932796240E+04 / On-source time
EXPOSURE= 3.361286932796240E+04 / Exposure time
MJD-OBS = 5.656450198799163E+04 / MJD of data start time
FILIN001= 'ae108003020xi0_0_3x3n090q_cl.evt.gz' / Input file name
SEQPNUM = 2 / Number of times this dataset processed
PROCVER = '3.0.22.44' / Processing script version
MK1STVER= 'mk1stfits20120530' / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20160607_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae108003020xi1_0_3x3n140b_cl.evt.gz' / Input file name
FILIN003= 'ae108003020xi3_0_3x3n092c_cl.evt.gz' / Input file name
COMMENT -------------------------
COMMENT BITPIX compressed from 32 to 8.
COMMENT Pixel values greater than 255 was set to 255.
COMMENT This file was made for JUDO-Suzaku.
COMMENT -------------------------
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
Abstract:
This is the proposal for the XIS calibration observations in the AO8 cycle.