Suzaku Observation : 809021010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '809021010' / Observation identification string
OBSERVER= 'NAOMI OTA' / Principal Investigator
OBJECT = 'RXCJ2157.4-0747 NE' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 329.3708 / planned target R.A.(deg)
DEC_OBJ = -7.7975 / planned target DEC.(deg)
RA_NOM = 3.293742000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -7.800300000000000E+00 / Declination of target (deci. deg)
PA_NOM = 250.0004 / nominal position angle from north to DETY(deg)
MEAN_EA1= 329.374247529901 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 97.800285566326 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 199.999648968060 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-11-11T13:00:50' / Start date of observations
DATE-END= '2014-11-12T02:00:15' / End date of observations
TSTART = 4.690278496715095E+08 / time start
TSTOP = 4.690728016547484E+08 / time stop
TELAPSE = 4.495198323893547E+04 / elapsed time
ONTIME = 1.864598748159409E+04 / On-source time
EXPOSURE= 1.864598748159409E+04 / Exposure time
MJD-OBS = 5.697256381777210E+04 / MJD of data start time
FILIN001= 'ae809021010xi0_0_3x3n066t_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae809021010xi0_0_5x5n066t_cl.evt.gz' / Input file name
FILIN003= 'ae809021010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae809021010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae809021010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae809021010xi3_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:
About 5-10% of galaxy clusters in the ROSAT survey have a very diffuse, low X-ray surface brightness (hereafter, LSB clusters). There are only 5 LSB clusters in the nearby universe, but it is no surprise that the majority of them may have been missed in existing X-ray surveys. Revealing gas and mass profiles of this unexplored population is critical not only for understanding its nature but cluster cosmology. Our Suzaku study of 2 LSB clusters indicated that their gas profiles deviate from self-similar expectations. We thus aim at establishing our findings by observing 3 remaining LSB clusters, clarifying whether they follow a similar trend, and inferring their mean gas profiles and dispersions. This study can only be achieved by the Suzaku's high sensitivity for diffuse emission.