Suzaku Observation : 803032010

QL FITS Image

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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '803032010'          / Observation identification string
OBSERVER= 'SHO NISHINO'        / Principal Investigator
OBJECT  = 'A3627CENTER'        / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             243.5766 / planned target R.A.(deg)
DEC_OBJ =             -60.8478 / planned target DEC.(deg)
RA_NOM  = 2.435672000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -6.084990000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             129.9148 / nominal position angle from north to DETY(deg)
MEAN_EA1=     243.567156011980 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     150.849926561981 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     320.085172972494 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2009-03-15T22:09:21' / Start date of observations
DATE-END= '2009-03-16T14:34:24' / End date of observations
TSTART  = 2.904701840000000E+08 / time start
TSTOP   = 2.905292507480446E+08 / time stop
TELAPSE = 5.906674804455042E+04 / elapsed time
ONTIME  = 4.604188182377815E+04 / On-source time
EXPOSURE= 4.604188182377815E+04 / Exposure time
MJD-OBS = 5.490592416879629E+04 / MJD of data start time
FILIN001= 'ae803032010xi0_0_3x3n066a_cl.evt.gz' / Input file name
SEQPNUM =                    3 / Number of times this dataset processed
PROCVER = '3.0.22.43'          / Processing script version
MK1STVER= 'mk1stfits20120530'  / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20151005_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae803032010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae803032010xi3_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 propsoe to observe the cluster of galaxies A3627, which has evidences of cluster merging, in order to detect hard X-rays from high energy particles acceralated in the cluster and also measure the doppler shift of the iron-K line. This cluster is a nearby bright cluster behind the Galactic plane, and thus so far X-ray studies have been poor. However, its proximity and relatively low temperature against other merging clusters enable us to constrain the hard X-ray emission more tightly.