Suzaku Observation : 806080010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '806080010' / Observation identification string
OBSERVER= 'AMALIA K HICKS' / Principal Investigator
OBJECT = 'RCS044406-2820.4' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 71.0250 / planned target R.A.(deg)
DEC_OBJ = -28.3400 / planned target DEC.(deg)
RA_NOM = 7.102209999999999E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -2.834300000000000E+01 / Declination of target (deci. deg)
PA_NOM = 99.3268 / nominal position angle from north to DETY(deg)
MEAN_EA1= 71.022149302002 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 118.342958905620 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 350.673214772692 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-09-23T15:09:33' / Start date of observations
DATE-END= '2011-09-24T21:00:15' / End date of observations
TSTART = 3.701059379409731E+08 / time start
TSTOP = 3.702126060000000E+08 / time stop
TELAPSE = 1.066680590268970E+05 / elapsed time
ONTIME = 5.067232687604427E+04 / On-source time
EXPOSURE= 5.067232687604427E+04 / Exposure time
MJD-OBS = 5.582763428385385E+04 / MJD of data start time
FILIN001= 'ae806080010xi0_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= 'ae806080010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae806080010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae806080010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae806080010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae806080010xi3_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