Suzaku Observation : 809042030
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '809042030' / Observation identification string
OBSERVER= 'KIYOSHI HAYASHIDA' / Principal Investigator
OBJECT = 'A1674_Offset' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 196.9992 / planned target R.A.(deg)
DEC_OBJ = 67.3092 / planned target DEC.(deg)
RA_NOM = 1.969691000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 6.729949999999999E+01 / Declination of target (deci. deg)
PA_NOM = 328.3620 / nominal position angle from north to DETY(deg)
MEAN_EA1= 196.969145092251 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 22.700506716095 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 121.638008294889 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-05-24T15:01:12' / Start date of observations
DATE-END= '2014-05-25T17:40:21' / End date of observations
TSTART = 4.542589027448838E+08 / time start
TSTOP = 4.543544890000000E+08 / time stop
TELAPSE = 9.558625511616468E+04 / elapsed time
ONTIME = 6.747553466135263E+04 / On-source time
EXPOSURE= 6.747553466135263E+04 / Exposure time
MJD-OBS = 5.680162693204726E+04 / MJD of data start time
FILIN001= 'ae809042030xi1_0_3x3n130b_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= 'ae809042030xi1_0_5x5n130b_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:
A1674 is a nearby cluster of galaxies, cataloged as richness class 3. Regardless of this extreme richness, its X-ray luminosity is as low as 5e43 erg/s. Our Suzaku AO1 observation revealed that A1674 consists of at least two clusters, one at z~0.2 and the other at z~0.1. Moreover, excess hard X-ray emission was detected with an intensity exceeding the 90% confidence range of the NXB modeling uncertainty. We aim to confirm this hard X-ray emission and to localize that component (really diffuse or point-like) by performing 4 pointings during the AO9 phase.