Suzaku Observation : 708006030

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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '708006030'          / Observation identification string
OBSERVER= 'HIROFUMI NODA'      / Principal Investigator
OBJECT  = 'NGC 3516'           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             166.6979 / planned target R.A.(deg)
DEC_OBJ =              72.5685 / planned target DEC.(deg)
RA_NOM  = 1.666764000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 7.255740000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             307.6030 / nominal position angle from north to DETY(deg)
MEAN_EA1=     166.676443953018 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      17.442630070975 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     142.397020696216 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-05-12T00:22:24' / Start date of observations
DATE-END= '2013-05-13T02:30:23' / End date of observations
TSTART  = 4.216376487358278E+08 / time start
TSTOP   = 4.217255490000000E+08 / time stop
TELAPSE = 8.790026417219639E+04 / elapsed time
ONTIME  = 5.042830968922377E+04 / On-source time
EXPOSURE= 5.042830968922377E+04 / Exposure time
MJD-OBS = 5.642406612175726E+04 / MJD of data start time
FILIN001= 'ae708006030xi0_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= 'ae708006030xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae708006030xi3_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 series of Suzaku observations of the type I Seyfert galaxy NGC 3516 combined with an optical monitoring campaign. By applying the C3PO method (Noda et al. 2012) to the time variable AGN signals, we can decompose them into individual spectral components, and identify (presumably) primary X-ray emissions in the soft and hard X-ray band distinct from the well-known power law continuum, as well as the reflection component (Noda et al. 2011a, 2011b, 2012). Multiple observations enable us to see the time variability of each primary component, and compare it with an optical variation. From these studies, we can examine where the three primary sources generally exist in AGN central engines.