Suzaku Observation : 807073020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '807073020' / Observation identification string
OBSERVER= 'ERIC D. MILLER' / Principal Investigator
OBJECT = 'ABELL 2597' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 351.1533 / planned target R.A.(deg)
DEC_OBJ = -12.0431 / planned target DEC.(deg)
RA_NOM = 3.511561000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -1.204460000000000E+01 / Declination of target (deci. deg)
PA_NOM = 250.0003 / nominal position angle from north to DETY(deg)
MEAN_EA1= 351.156086452159 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 102.044616644723 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 199.999686453339 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-12-01T07:56:27' / Start date of observations
DATE-END= '2012-12-02T12:53:10' / End date of observations
TSTART = 4.076637938708608E+08 / time start
TSTOP = 4.077678530000000E+08 / time stop
TELAPSE = 1.040591291392446E+05 / elapsed time
ONTIME = 5.005852155482769E+04 / On-source time
EXPOSURE= 5.005852155482769E+04 / Exposure time
MJD-OBS = 5.626233169044978E+04 / MJD of data start time
FILIN001= 'ae807073020xi0_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= 'ae807073020xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae807073020xi3_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:
We propose observations of 2 clusters of galaxies to probe the cluster environment out to r200 in order to (1) determine the temperature and density profiles for a representative sample of clusters; (2) search for azimuthal variations at these scales which may be indicative of the ongoing cluster accretion process; (3) construct the largest sample to date of clusters with accurate X-ray temperature and pressure determination out to r200; and (4) provide a fiducial data set for detailed comparison with high resolution numerical simulations. These targets capitalize on our large sample of clusters surveyed with XMM, expanding on a project started in previous cycles, and will provide a large enough data set to truly sample the properties of clusters at large radii.