Suzaku Observation : 704038010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '704038010' / Observation identification string
OBSERVER= 'WAYNE BAUMGARTNER' / Principal Investigator
OBJECT = '3C 332 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 244.4272 / planned target R.A.(deg)
DEC_OBJ = 32.3763 / planned target DEC.(deg)
RA_NOM = 2.444239000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.236320000000000E+01 / Declination of target (deci. deg)
PA_NOM = 292.5008 / nominal position angle from north to DETY(deg)
MEAN_EA1= 244.423859681129 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 57.636782964586 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 157.499210222944 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2009-08-08T00:49:13' / Start date of observations
DATE-END= '2009-08-09T11:10:20' / End date of observations
TSTART = 3.030086891276743E+08 / time start
TSTOP = 3.031304069910273E+08 / time stop
TELAPSE = 1.217178633530140E+05 / elapsed time
ONTIME = 5.983387563395500E+04 / On-source time
EXPOSURE= 5.983387563395500E+04 / Exposure time
MJD-OBS = 5.505104575592215E+04 / MJD of data start time
FILIN001= 'ae704038010xi0_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= 'ae704038010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae704038010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae704038010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae704038010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae704038010xi3_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:
We propose to observe the five most luminous type II AGN detected in the Swift BAT all sky hard X-ray survey (14-195~keV). Because BAT's detection efficiency for absorbed sources in the high energy band is very high, these sources are the most luminous (log($L_x$) $> 45.5$~ergs~sec$^{-1}$) absorbed tyoe II QSOs in the local universe and the most ripe for study with suzaku. 3C~332 is believed to be Compton-thick as suggested by chandra observations, and the newly discovered source SWIFT~J2344.6-4233 at a redshift of $z=0.6$ is the most luminous object in the BAT sample with log($L_x$) $=46.5$~ergs~sec$^{-1}$.