Suzaku Observation : 508038010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '508038010' / Observation identification string
OBSERVER= 'HIDETOSHI SANO' / Principal Investigator
OBJECT = 'VELA JR WEST3' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 131.7800 / planned target R.A.(deg)
DEC_OBJ = -46.2700 / planned target DEC.(deg)
RA_NOM = 1.317730000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -4.627430000000000E+01 / Declination of target (deci. deg)
PA_NOM = 116.2100 / nominal position angle from north to DETY(deg)
MEAN_EA1= 131.772978946348 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 136.274276311613 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 333.790021410238 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-11-24T01:55:54' / Start date of observations
DATE-END= '2013-11-24T17:34:13' / End date of observations
TSTART = 4.385733608852087E+08 / time start
TSTOP = 4.386296364876051E+08 / time stop
TELAPSE = 5.627560239636898E+04 / elapsed time
ONTIME = 3.499111798763275E+04 / On-source time
EXPOSURE= 3.499111798763275E+04 / Exposure time
MJD-OBS = 5.662008130867140E+04 / MJD of data start time
FILIN001= 'ae508038010xi0_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= 'ae508038010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae508038010xi3_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 toward West-rim of the SNR Vela Jr (RX J0852.0-4622). Recent our CO and HI data have revealed a dense interaction between SNR shock wave and the interstellar gas. Particularly, we found the synchrotron X-ray enhancement around the molecular core in the West-rim. This results indicate an efficient particle acceleration cased by shock-cloud interaction. This further observation allow us to investigate a more detail spectrum analysis comparable for the molecular core distribution.