Suzaku Observation : 807075010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '807075010' / Observation identification string
OBSERVER= 'AMALIA K HICKS' / Principal Investigator
OBJECT = 'RCS110619-0423.6' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 166.5792 / planned target R.A.(deg)
DEC_OBJ = -4.3933 / planned target DEC.(deg)
RA_NOM = 1.665769000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -4.391500000000000E+00 / Declination of target (deci. deg)
PA_NOM = 109.9541 / nominal position angle from north to DETY(deg)
MEAN_EA1= 166.576937583299 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 94.391549281853 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 340.045877235315 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-11-22T20:27:04' / Start date of observations
DATE-END= '2012-11-25T00:13:19' / End date of observations
TSTART = 4.069312419763504E+08 / time start
TSTOP = 4.071161220000000E+08 / time stop
TELAPSE = 1.848800236495733E+05 / elapsed time
ONTIME = 7.710049685287476E+04 / On-source time
EXPOSURE= 7.710049685287476E+04 / Exposure time
MJD-OBS = 5.625385308055961E+04 / MJD of data start time
FILIN001= 'ae807075010xi0_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= 'ae807075010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae807075010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae807075010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae807075010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae807075010xi3_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 24 optically-selected clusters of galaxies out to z~1. Here we propose 5 additional observations in order to uniformly span our total mass-redshift space over the range 0.15