Suzaku Observation : 807061010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '807061010' / Observation identification string
OBSERVER= 'ERIC D. MILLER' / Principal Investigator
OBJECT = 'SDSS J0837+4414' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 129.4973 / planned target R.A.(deg)
DEC_OBJ = 44.2489 / planned target DEC.(deg)
RA_NOM = 1.294975000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 4.425660000000000E+01 / Declination of target (deci. deg)
PA_NOM = 110.1912 / nominal position angle from north to DETY(deg)
MEAN_EA1= 129.497528970946 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 45.743356477331 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 339.808751389015 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-10-13T19:51:54' / Start date of observations
DATE-END= '2012-10-14T08:26:13' / End date of observations
TSTART = 4.034736580000000E+08 / time start
TSTOP = 4.035170970000000E+08 / time stop
TELAPSE = 4.343900000000000E+04 / elapsed time
ONTIME = 2.062193596798182E+04 / On-source time
EXPOSURE= 2.062193596798182E+04 / Exposure time
MJD-OBS = 5.621383474750000E+04 / MJD of data start time
FILIN001= 'ae807061010xi0_0_3x3n066l_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= 'ae807061010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae807061010xi3_0_3x3n066a_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:
Fossil groups (FGs) are systems dominated by a single large galaxy with a cluster-scale X-ray halo. They are thought to be old, isolated galaxy groups in which the large galaxies have coalesced through dynamical friction, but recent studies reveal a more complicated picture. We propose Suzaku observations of 5 optically selected FG candidates. These targets will extend our previous survey, which identified 12 FGs; when combined with 5 FG candidates approved for the current Chandra cycle, this will create the largest uniformly-selected sample of real FGs. The L_X and T_X measured will be used with optical spectroscopy to extend FG scaling relations to low mass, and to plan deeper X-ray spectroscopic follow-up to constrain the formation epoch and evolution of these puzzling systems.