Suzaku Observation : 801039010

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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '801039010'          / Observation identification string
OBSERVER= 'HIRONORI MATSUMOTO' / Principal Investigator
OBJECT  = 'NONE    '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             188.2679 / planned target R.A.(deg)
DEC_OBJ =              11.8322 / planned target DEC.(deg)
RA_NOM  = 1.882678000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 1.183670000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             119.8990 / nominal position angle from north to DETY(deg)
MEAN_EA1=     188.267794808833 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      78.163294283560 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     330.101040907077 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2006-12-02T03:03:49' / Start date of observations
DATE-END= '2006-12-03T07:29:20' / End date of observations
TSTART  = 2.183438338483044E+08 / time start
TSTOP   = 2.184448400000000E+08 / time stop
TELAPSE = 1.010061516956091E+05 / elapsed time
ONTIME  = 5.365811550614238E+04 / On-source time
EXPOSURE= 5.365811550614238E+04 / Exposure time
MJD-OBS = 5.407112844944796E+04 / MJD of data start time
FILIN001= 'ae801039010xi0_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= 'ae801039010xi0_0_5x5n066a_cl.evt.gz' / Input file name
FILIN003= 'ae801039010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae801039010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae801039010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae801039010xi3_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:

The black hole at the center of M87 is one of the most heaviest in the universe. Recently TeV-gamma ray emission from M87 was found. M87 is thus a very strong candidate for an accelerator of ultra-high energy cosmic rays. We aim at the detection of non-thermal hard X-rays from M87 to clarify the mechanism of the particle acceleration. The giant elliptical galaxy M87 is at the center of the Virgo cluster of galaxies, which is the nearest cluster. We can investigate the distribution of various metal elements. We will clarify how the metals, especially oxygen, diffuse to the intracluster space from the galaxy M87.