Suzaku Observation : 805003010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '805003010' / Observation identification string
OBSERVER= 'KYOKO MATSUSHITA' / Principal Investigator
OBJECT = 'A478 OFFSET C' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 63.6291 / planned target R.A.(deg)
DEC_OBJ = 10.5099 / planned target DEC.(deg)
RA_NOM = 6.363280000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 1.050740000000000E+01 / Declination of target (deci. deg)
PA_NOM = 259.6787 / nominal position angle from north to DETY(deg)
MEAN_EA1= 63.632782698039 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 79.492627778629 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 190.321293066980 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-02-12T05:58:24' / Start date of observations
DATE-END= '2011-02-13T08:27:16' / End date of observations
TSTART = 3.508057040000000E+08 / time start
TSTOP = 3.508994920000000E+08 / time stop
TELAPSE = 9.378800000000000E+04 / elapsed time
ONTIME = 4.716455733388662E+04 / On-source time
EXPOSURE= 4.716455733388662E+04 / Exposure time
MJD-OBS = 5.560425194657407E+04 / MJD of data start time
FILIN001= 'ae805003010xi0_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= 'ae805003010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae805003010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae805003010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae805003010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae805003010xi3_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:
Clusters of galaxies are thought to form from accretion and merging of smaller systems among large-scale filaments. X-ray observations of cluster outskirts give us valuable information about the structure formation, gas heating and cooling, and metal enrichment of clusters of galaxies. Here, we propose deep surveys of a representative regular cluster, Abell 478