Suzaku Observation : 505087010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '505087010' / Observation identification string
OBSERVER= 'KATSUJI KOYAMA' / Principal Investigator
OBJECT = 'GALACTIC_BULGE18' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 269.3150 / planned target R.A.(deg)
DEC_OBJ = -34.5767 / planned target DEC.(deg)
RA_NOM = 2.693126000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -3.457160000000000E+01 / Declination of target (deci. deg)
PA_NOM = 70.9023 / nominal position angle from north to DETY(deg)
MEAN_EA1= 269.312630426207 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 124.571597344013 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 19.097656245316 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-03-13T10:20:22' / Start date of observations
DATE-END= '2011-03-14T12:39:21' / End date of observations
TSTART = 3.533268273953378E+08 / time start
TSTOP = 3.534211740000000E+08 / time stop
TELAPSE = 9.434660466223955E+04 / elapsed time
ONTIME = 5.147550186187029E+04 / On-source time
EXPOSURE= 5.147550186187029E+04 / Exposure time
MJD-OBS = 5.563343161550159E+04 / MJD of data start time
FILIN001= 'ae505087010xi0_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= 'ae505087010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae505087010xi3_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.