Suzaku Observation : 502051010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '502051010' / Observation identification string
OBSERVER= 'KATSUJI KOYAMA' / Principal Investigator
OBJECT = 'GC_G0.9+0.1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 266.9350 / planned target R.A.(deg)
DEC_OBJ = -28.1500 / planned target DEC.(deg)
RA_NOM = 2.669332000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.814740000000000E+01 / Declination of target (deci. deg)
PA_NOM = 105.8953 / nominal position angle from north to DETY(deg)
MEAN_EA1= 266.933206666612 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 118.147429500700 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 344.104733300870 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-03-11T06:19:45' / Start date of observations
DATE-END= '2008-03-15T05:30:18' / End date of observations
TSTART = 2.585327100517101E+08 / time start
TSTOP = 2.588730020000000E+08 / time stop
TELAPSE = 3.402919482898712E+05 / elapsed time
ONTIME = 1.387614350353181E+05 / On-source time
EXPOSURE= 1.387614350353181E+05 / Exposure time
MJD-OBS = 5.453627747957998E+04 / MJD of data start time
FILIN001= 'ae502051010xi0_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= 'ae502051010xi0_0_5x5n066a_cl.evt.gz' / Input file name
FILIN003= 'ae502051010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae502051010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae502051010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae502051010xi3_0_5x5n066a_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:
The Suzaku PV observations found that the diffuse X-rays (6.7 and 6.9 keV-lines) from the GC region can well be explained by a thermal emission from hot plasma (6-7 keV). The most plausible energy injection source is multiple SNe. The huge thermal energy (10^54 ergs) and short timescale (10^5 yr) of the hot plasma suggest that the GC region harbors at least 10 young SNRs. To confirm this scenario, we propose to observe the shell of G0.9+0.1 and the connecting region of Sgr B and D. The first objective is to detect a thermal emission from the shell of G0.9+0.1 and the second is to discover new SNRs.