Suzaku Observation : 808104010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '808104010' / Observation identification string
OBSERVER= 'LORENZO LOVISARI' / Principal Investigator
OBJECT = 'A3528-S OFFSET 1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 193.8760 / planned target R.A.(deg)
DEC_OBJ = -29.4464 / planned target DEC.(deg)
RA_NOM = 1.938801000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.947680000000000E+01 / Declination of target (deci. deg)
PA_NOM = 289.4829 / nominal position angle from north to DETY(deg)
MEAN_EA1= 193.880116767745 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 119.476805602530 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 160.517082485835 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-07-27T10:27:50' / Start date of observations
DATE-END= '2013-07-28T12:41:10' / End date of observations
TSTART = 4.282361740000000E+08 / time start
TSTOP = 4.283304550396113E+08 / time stop
TELAPSE = 9.428103961127996E+04 / elapsed time
ONTIME = 4.034907843917608E+04 / On-source time
EXPOSURE= 4.034907843917608E+04 / Exposure time
MJD-OBS = 5.650043794194444E+04 / MJD of data start time
FILIN001= 'ae808104010xi0_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= 'ae808104010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae808104010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae808104010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae808104010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae808104010xi3_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:
We propose to observe, for a total of 180 ks, the region between the galaxy cluster A3528 and the complex A3530-A3532, in which we expect to find the filament connecting the clusters. With the requested time we aim to detect the Warm Hot Intergalactic Medium (WHIM) by its thermal soft-Xray emission, to resolve one of the major problems of modern astrophysics - the missing baryons , which are now thought to reside in the filaments connecting clusters. In addition to a full understanding of the typical baryon fraction, the proposed observations will allow us to study the gas clumping in the cluster outskirts. Furthermore, a combined analysis of X-ray and optical data will enable us to shed light on the influence of the environments on galaxy evolution.