Suzaku Observation : 108004020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '108004020' / Observation identification string
OBSERVER= 'MASAHIRO TSUJIMOTO' / Principal Investigator
OBJECT = 'CYGNUS_LOOP_P8' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 313.9958 / planned target R.A.(deg)
DEC_OBJ = 31.4752 / planned target DEC.(deg)
RA_NOM = 3.140082000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.146520000000000E+01 / Declination of target (deci. deg)
PA_NOM = 240.0001 / nominal position angle from north to DETY(deg)
MEAN_EA1= 314.008243049972 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 58.534757225164 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 209.999851430971 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-12-05T04:16:56' / Start date of observations
DATE-END= '2013-12-05T09:37:15' / End date of observations
TSTART = 4.395322286704268E+08 / time start
TSTOP = 4.395514202873833E+08 / time stop
TELAPSE = 1.919161695653200E+04 / elapsed time
ONTIME = 1.178432926970720E+04 / On-source time
EXPOSURE= 1.178432926970720E+04 / Exposure time
MJD-OBS = 5.663117931544475E+04 / MJD of data start time
FILIN001= 'ae108004020xi0_0_3x3n066q_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= 'ae108004020xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae108004020xi3_0_3x3n066c_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.