Suzaku Observation : 705008010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '705008010' / Observation identification string
OBSERVER= 'YOSHITO HABA' / Principal Investigator
OBJECT = 'ESO 428-G014' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 109.1300 / planned target R.A.(deg)
DEC_OBJ = -29.3247 / planned target DEC.(deg)
RA_NOM = 1.091256000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.932480000000000E+01 / Declination of target (deci. deg)
PA_NOM = 123.1273 / nominal position angle from north to DETY(deg)
MEAN_EA1= 109.125622337390 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 119.324790813825 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 326.872664114044 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-11-16T03:17:39' / Start date of observations
DATE-END= '2010-11-18T13:13:15' / End date of observations
TSTART = 3.431958880000000E+08 / time start
TSTOP = 3.433996527763344E+08 / time stop
TELAPSE = 2.037647763344049E+05 / elapsed time
ONTIME = 8.290338074773550E+04 / On-source time
EXPOSURE= 8.290338074773550E+04 / Exposure time
MJD-OBS = 5.551617537250000E+04 / MJD of data start time
FILIN001= 'ae705008010xi0_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= 'ae705008010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae705008010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae705008010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae705008010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae705008010xi3_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:
Non-Hidden Broad Line Region Seyfert 2 galaxies (NHBLR Sey2s) are classified as Seyfert 2 galaxies without broad Balmer lines even in the polarized light. One possible interpretation for the absence of broad lines is that NHBLR Sey2s are viewed from an extreme edge-on direction, so that the scattered light is obscured by the accretion torus. Hence observation of NHBLR Sey2s provides us the unique opportunity to investigate the densest region of the torus. We, therefore, propose 80 ksec observation of NHBLR Sey2 ESO 428-G014. High sensitivity throughout the 0.5-70 keV wide energy band of Suzaku allows us to strictly constrain the intrinsic X-ray luminosity and column density of the obscuring material. From our observation, we expect to derive more complete unified picture of AGNs.