Suzaku Observation : 702084010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '702084010' / Observation identification string
OBSERVER= 'CHRISTINE JONES' / Principal Investigator
OBJECT = 'XBONGBLUE2' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 217.7596 / planned target R.A.(deg)
DEC_OBJ = 34.3327 / planned target DEC.(deg)
RA_NOM = 2.177653000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.434130000000000E+01 / Declination of target (deci. deg)
PA_NOM = 130.3787 / nominal position angle from north to DETY(deg)
MEAN_EA1= 217.765337130503 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 55.658682159455 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 319.621312341619 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2007-12-20T04:02:55' / Start date of observations
DATE-END= '2007-12-20T12:07:18' / End date of observations
TSTART = 2.514410960000000E+08 / time start
TSTOP = 2.514666360000000E+08 / time stop
TELAPSE = 2.554000000000000E+04 / elapsed time
ONTIME = 1.481615574246645E+04 / On-source time
EXPOSURE= 1.481615574246645E+04 / Exposure time
MJD-OBS = 5.445419861324074E+04 / MJD of data start time
FILIN001= 'ae702084010xi0_0_3x3n066a_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= 'ae702084010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae702084010xi3_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 to use Suzaku's large collecting area and excellent energy response to measure accurate X-ray spectra for 9 XBONGs and 8 luminous Type 2 AGN selected from very large samples of identified XBONGs and Type 2 AGN found in our Chandra XBootes survey. We have obtained optical spectra for 258 XBONGs and identified ~700 X-ray luminous Type 2 AGN at z>0.7. With known source positions and X-ray fluxes, we select sources that are relatively bright with little or no contamination from other X-ray sources. Thus we will measure individual spectra for these bright sources. We propose eight 15 ksec Suzaku XIS observations to measure the absorption in 8 luminous z > 0.8 Type 2 AGN and eight 10 ksec observations to measure the absorption and iron emission for nine XBONGs.