Suzaku Observation : 704002010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '704002010' / Observation identification string
OBSERVER= 'HISAMITSU AWAKI' / Principal Investigator
OBJECT = 'MRK 573 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 25.9908 / planned target R.A.(deg)
DEC_OBJ = 2.3499 / planned target DEC.(deg)
RA_NOM = 2.601610000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 2.290400000000000E+00 / Declination of target (deci. deg)
PA_NOM = 249.7100 / nominal position angle from north to DETY(deg)
MEAN_EA1= 26.016098668901 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 87.709589180413 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 200.289970796123 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-01-21T14:04:01' / Start date of observations
DATE-END= '2010-01-23T00:47:19' / End date of observations
TSTART = 3.173978920000000E+08 / time start
TSTOP = 3.175203440000000E+08 / time stop
TELAPSE = 1.224520000000000E+05 / elapsed time
ONTIME = 6.431176218366623E+04 / On-source time
EXPOSURE= 6.431176218366623E+04 / Exposure time
MJD-OBS = 5.521758745583333E+04 / MJD of data start time
FILIN001= 'ae704002010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 2 / 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= 'ae704002010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae704002010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae704002010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae704002010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae704002010xi3_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:
Monte Carlo simulation is one of the best tools to study the complex spectra of Compton-thick AGNs and to figure out the relation between their nuclear structures and X-ray spectra. We have simulated X-ray spectra of Compton-thick AGNs obscured by an accretion torus, and found that observed spectra of Compton thick objects, Mrk 3 and NGC 2273 are well reproduced by the simulated X-ray spectra. Furthermore, our simulation predicts that there are many obscured AGNs with a heavily absorbed reflection component. Their spectra are similar to that predicted from synthesis modeling of the Cosmic X-ray Background. We propose Suzaku observations of candidates of the Compton thick AGNs, Mrk 573 and Mrk 78.