Suzaku Observation : 703032010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '703032010' / Observation identification string
OBSERVER= 'RICHARD F MUSHOTZKY' / Principal Investigator
OBJECT = 'NGC 788 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 30.2769 / planned target R.A.(deg)
DEC_OBJ = -6.8155 / planned target DEC.(deg)
RA_NOM = 3.026200000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -6.759300000000000E+00 / Declination of target (deci. deg)
PA_NOM = 77.3580 / nominal position angle from north to DETY(deg)
MEAN_EA1= 30.262014009726 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 96.759265629656 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 12.641985913513 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-07-13T00:50:57' / Start date of observations
DATE-END= '2008-07-14T01:14:24' / End date of observations
TSTART = 2.692291210000000E+08 / time start
TSTOP = 2.693129410000000E+08 / time stop
TELAPSE = 8.382000000000000E+04 / elapsed time
ONTIME = 4.591527050024271E+04 / On-source time
EXPOSURE= 4.591527050024271E+04 / Exposure time
MJD-OBS = 5.466007853222222E+04 / MJD of data start time
FILIN001= 'ae703032010xi0_0_3x3n066a_cl.evt.gz' / Input file name
SEQPNUM = 5 / 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= 'ae703032010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae703032010xi3_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:
The classical unified model predicts only one type of Seyfert II (Sy2). Recent observations of SWIFT BAT-detected AGN found at least 4 classes of Sy2s: (1) objects with high column density and scattered soft x-rays, (2) Compton thick objects, (3) `hidden' AGN (Ueda et al. 2007), and (4) the `changing look' objects (Risaliti et al. 2006). The nature of these sources can only be revealed with high quality broad-band X-ray spectra from Suzaku. Thus, we are proposing 40ks observations for 2 of the brightest BAT AGN without high quality data, NGC 788, a type (3) object showing polarized optical broad lines, and NGC 3281, a classified (2) object. Such observations are necessary to build a reasonably large sample of high-quality, broad-band Sy2 spectra covering the range of X-ray/optical types.