Suzaku Observation : 505084010

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UDON2 to quickly extract spectrum and light-curve
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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '505084010'          / Observation identification string
OBSERVER= 'KATSUJI KOYAMA'     / Principal Investigator
OBJECT  = 'GALACTIC_BULGE15'   / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             265.6988 / planned target R.A.(deg)
DEC_OBJ =             -32.7884 / planned target DEC.(deg)
RA_NOM  = 2.656963000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -3.277840000000000E+01 / Declination of target (deci. deg)
PA_NOM  =              89.8786 / nominal position angle from north to DETY(deg)
MEAN_EA1=     265.696339400463 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     122.778407585631 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=       0.121441943053 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-03-06T05:36:44' / Start date of observations
DATE-END= '2011-03-07T13:01:11' / End date of observations
TSTART  = 3.527050260000000E+08 / time start
TSTOP   = 3.528172000000000E+08 / time stop
TELAPSE = 1.121740000000000E+05 / elapsed time
ONTIME  = 5.032570409685373E+04 / On-source time
EXPOSURE= 5.032570409685373E+04 / Exposure time
MJD-OBS = 5.562623484009259E+04 / MJD of data start time
FILIN001= 'ae505084010xi0_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= 'ae505084010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae505084010xi3_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 three classes of objects, which seem independent subjects, but are closely related with each others. These subjects are the Galactic center and the ridge diffuse X-rays (GCDX & GRDX), Unidentified sources (UIDHESS) found with HESS and the hard X-rays from radio faint supernova remnants (Hard SNR) found with ASCA. Our objectives are to study individual science on each subject, combined the results, and to finally approach to a unified picture on the diffuse high energy aspects in our Galaxy.