Suzaku Observation : 806082010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '806082010' / Observation identification string
OBSERVER= 'AMALIA K HICKS' / Principal Investigator
OBJECT = 'RCS212414-6325.8' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 321.0583 / planned target R.A.(deg)
DEC_OBJ = -63.4300 / planned target DEC.(deg)
RA_NOM = 3.210509000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -6.342750000000000E+01 / Declination of target (deci. deg)
PA_NOM = 79.2319 / nominal position angle from north to DETY(deg)
MEAN_EA1= 321.050912272884 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 153.427454760709 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 10.768102099886 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-05-10T09:52:21' / Start date of observations
DATE-END= '2011-05-10T23:30:18' / End date of observations
TSTART = 3.583364274190806E+08 / time start
TSTOP = 3.583854034115471E+08 / time stop
TELAPSE = 4.897599246644974E+04 / elapsed time
ONTIME = 3.633041627585888E+04 / On-source time
EXPOSURE= 3.633041627585888E+04 / Exposure time
MJD-OBS = 5.569141309725788E+04 / MJD of data start time
FILIN001= 'ae806082010xi0_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= 'ae806082010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae806082010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae806082010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae806082010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae806082010xi3_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:
Accurate relationships between baryons in galaxy clusters and underlying dark matter distributions are crucial for using clusters as cosmological probes. Understanding the gamut of ICM properties, however, requires X-ray observations of samples chosen independently of their X-ray characteristics; likewise, such samples provide a powerful tool for quantifying redshift evolution in cluster properties. We have amassed X-ray observations of 19 optically-selected clusters of galaxies, half at z~0.3 and half at z~0.8. Here we propose 6 additional observations in order to uniformly span a total redshift range of 0.15