Suzaku Observation : 705011010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '705011010' / Observation identification string
OBSERVER= 'JUN KATAOKA' / Principal Investigator
OBJECT = 'EMS0857 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 198.1860 / planned target R.A.(deg)
DEC_OBJ = 0.8370 / planned target DEC.(deg)
RA_NOM = 1.981882000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 8.497000000000000E-01 / Declination of target (deci. deg)
PA_NOM = 111.0249 / nominal position angle from north to DETY(deg)
MEAN_EA1= 198.188189748846 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 89.150344332763 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 338.975082398340 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-01-17T04:38:43' / Start date of observations
DATE-END= '2011-01-17T17:54:22' / End date of observations
TSTART = 3.485543340000000E+08 / time start
TSTOP = 3.486009440000000E+08 / time stop
TELAPSE = 4.661000000000000E+04 / elapsed time
ONTIME = 2.208499817943573E+04 / On-source time
EXPOSURE= 2.208499817943573E+04 / Exposure time
MJD-OBS = 5.557819442342592E+04 / MJD of data start time
FILIN001= 'ae705011010xi0_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= 'ae705011010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae705011010xi3_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 observe with Suzaku a selected set of 7 Fermi-LAT observed high galactic latitude gamma-ray sources that have no identified counterpart in any other energy range. These sources have been detected by the Fermi-LAT with high confidence and are either active galactic nuclei, galactic pulsars, or an as-yet unidentified new class of gamma-ray sources. The proposed observations are for 40 ks or 20 ks per source covering the Fermi-LAT source error region allowing us to detect sources to a flux level several times 10^(-14) erg/cm^2/s. We will determine the X-ray counterpart within the Fermi-LAT error circle, and characterize its variability and spectral properties to reveal the nature of "GeV dark accelerators".