Suzaku Observation : 100027050
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '100027050' / Observation identification string
OBSERVER= 'Suzaku SWG' / Principal Investigator
OBJECT = '1E1743.1-2843(GC_BGD_3)' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 266.5900 / planned target R.A.(deg)
DEC_OBJ = -28.6510 / planned target DEC.(deg)
RA_NOM = 2.665920000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.865160000000000E+01 / Declination of target (deci. deg)
PA_NOM = 264.8800 / nominal position angle from north to DETY(deg)
MEAN_EA1= 266.592024773211 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 118.651628180264 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 185.119973408217 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2005-09-25T17:29:12' / Start date of observations
DATE-END= '2005-09-25T19:02:19' / End date of observations
TSTART = 1.809867370000000E+08 / time start
TSTOP = 1.809900466392940E+08 / time stop
TELAPSE = 3.309639294028282E+03 / elapsed time
ONTIME = 1.984639294028282E+03 / On-source time
EXPOSURE= 1.984639294028282E+03 / Exposure time
MJD-OBS = 5.363875464333333E+04 / MJD of data start time
FILIN001= 'ae100027050xi0_0_3x3n000a_cl.evt.gz' / Input file name
SEQPNUM = 4 / 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= 'ae100027050xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN003= 'ae100027050xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN004= 'ae100027050xi3_0_3x3n000a_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 obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin.