Suzaku Observation : 100028020
QL FITS Image
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '100028020' / Observation identification string
OBSERVER= 'Suzaku SWG' / Principal Investigator
OBJECT = 'HESS J1616-508_BGD1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 243.6615 / planned target R.A.(deg)
DEC_OBJ = -51.1763 / planned target DEC.(deg)
RA_NOM = 2.436660000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -5.117420000000000E+01 / Declination of target (deci. deg)
PA_NOM = 283.0062 / nominal position angle from north to DETY(deg)
MEAN_EA1= 243.665981240572 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 141.174216623782 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 166.993769051621 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2005-09-18T22:47:36' / Start date of observations
DATE-END= '2005-09-19T11:58:41' / End date of observations
TSTART = 1.804017900000000E+08 / time start
TSTOP = 1.804427347219504E+08 / time stop
TELAPSE = 4.094472195041180E+04 / elapsed time
ONTIME = 2.062999981123209E+04 / On-source time
EXPOSURE= 2.062999981123209E+04 / Exposure time
MJD-OBS = 5.363198442342592E+04 / MJD of data start time
FILIN001= 'ae100028020xi0_0_3x3n000a_cl.evt.gz' / Input file name
SEQPNUM = 3 / Number of times this dataset processed
PROCVER = '3.0.22.43' / Processing script version
MK1STVER= 'mk1stfits20120530' / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20151005_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae100028020xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN003= 'ae100028020xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN004= 'ae100028020xi3_0_3x3n000a_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: