Suzaku Observation : 701047010

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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '701047010'          / Observation identification string
OBSERVER= 'NANCY A. LEVENSON'  / Principal Investigator
OBJECT  = 'MRK 1   '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =              19.0300 / planned target R.A.(deg)
DEC_OBJ =              33.0894 / planned target DEC.(deg)
RA_NOM  = 1.906000000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 3.302890000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             249.7486 / nominal position angle from north to DETY(deg)
MEAN_EA1=      19.060042129745 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      56.971117214382 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     200.251405090395 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2007-01-11T12:45:49' / Start date of observations
DATE-END= '2007-01-14T14:00:24' / End date of observations
TSTART  = 2.218368510000000E+08 / time start
TSTOP   = 2.220975400000000E+08 / time stop
TELAPSE = 2.606890000000000E+05 / elapsed time
ONTIME  = 1.264441277174056E+05 / On-source time
EXPOSURE= 1.264441277174056E+05 / Exposure time
MJD-OBS = 5.411155688870370E+04 / MJD of data start time
FILIN001= 'ae701047010xi0_0_3x3n066a_cl.evt.gz' / Input file name
SEQPNUM =                    8 / 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= 'ae701047010xi0_0_5x5n066a_cl.evt.gz' / Input file name
FILIN003= 'ae701047010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae701047010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae701047010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae701047010xi3_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 supermassive black holes of active galactic nuclei (AGN) are fundamentally connected to the stars of their host galaxies, but it is not clear whether this relationship is evident at X-ray energies. We will test the prediction that prolific star formation is responsible for the soft X-ray emission from a Compton thick AGN that also contains a powerful circumnuclear starburst. The AGN's deep obscuration facilitates the soft X-ray measurements, and Compton thick AGN are generally significant, both as a large fraction of the local AGN population and for their contribution to the X-ray background. Furthermore, we will use the direct measurement of the intrinsic AGN luminosity to test unified AGN models and the validity of indirect luminosity indicators.