Suzaku Observation : 807120010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '807120010' / Observation identification string
OBSERVER= 'AURORA SIMIONESCU' / Principal Investigator
OBJECT = 'VIRGO S6' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 187.6496 / planned target R.A.(deg)
DEC_OBJ = 10.5551 / planned target DEC.(deg)
RA_NOM = 1.876479000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 1.055130000000000E+01 / Declination of target (deci. deg)
PA_NOM = 308.4999 / nominal position angle from north to DETY(deg)
MEAN_EA1= 187.647934306124 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 79.448729374907 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 141.500054180610 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-07-04T18:26:52' / Start date of observations
DATE-END= '2012-07-05T01:55:07' / End date of observations
TSTART = 3.947418530000000E+08 / time start
TSTOP = 3.947670464477673E+08 / time stop
TELAPSE = 2.519344776731730E+04 / elapsed time
ONTIME = 1.270135184043646E+04 / On-source time
EXPOSURE= 1.270135184043646E+04 / Exposure time
MJD-OBS = 5.611277218962963E+04 / MJD of data start time
FILIN001= 'ae807120010xi0_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= 'ae807120010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae807120010xi3_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 propose a legacy-class study of the outskirts of the Virgo Cluster, the nearest, second brightest galaxy cluster in the X-ray sky. This will provide the first detailed study of the outer parts of a low-mass system, with unparalleled signal-to-noise and spatial resolution. We will observe along four distinct directions which will provide unique insight into the ongoing virialization and equilibration processes that occur during large-scale structure formation. The Virgo Cluster is dynamically complex, with clear differences in its X-ray and optical properties along the chosen axes. This, its proximity and brightness, and the unrivaled multi-wavelength follow-up data make it the ideal system for studying the effects that different accretion rates have in shaping the ICM at large radii.