Suzaku Observation : 805089010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '805089010' / Observation identification string
OBSERVER= 'AMALIA K HICKS' / Principal Investigator
OBJECT = 'RCS2318-0024' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 349.6267 / planned target R.A.(deg)
DEC_OBJ = -0.4113 / planned target DEC.(deg)
RA_NOM = 3.496301000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -4.169000000000000E-01 / Declination of target (deci. deg)
PA_NOM = 248.0438 / nominal position angle from north to DETY(deg)
MEAN_EA1= 349.630093092323 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 90.416857521383 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 201.956229973122 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-11-26T00:26:44' / Start date of observations
DATE-END= '2010-11-27T07:03:14' / End date of observations
TSTART = 3.440464171247174E+08 / time start
TSTOP = 3.441565807565453E+08 / time stop
TELAPSE = 1.101636318279505E+05 / elapsed time
ONTIME = 5.033701673430204E+04 / On-source time
EXPOSURE= 5.033701673430204E+04 / Exposure time
MJD-OBS = 5.552601945959163E+04 / MJD of data start time
FILIN001= 'ae805089010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 2 / 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= 'ae805089010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae805089010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae805089010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae805089010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae805089010xi3_0_5x5n066a_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:
Understanding relationships between baryons in galaxy clusters and underlying dark matter distributions is crucial for using clusters as cosmological probes. Recent work indicates massive low-Lx clusters at all redshifts, in conflict with self-similarity predictions. The only way to quantify these findings is to observe a sample chosen independently of X-ray properties. We propose to study 13 clusters at 0.15