Suzaku Observation : 508059010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '508059010' / Observation identification string
OBSERVER= 'TAKESHI GO TSURU' / Principal Investigator
OBJECT = 'G359.0-0.9 S' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 266.8720 / planned target R.A.(deg)
DEC_OBJ = -30.3137 / planned target DEC.(deg)
RA_NOM = 2.668698000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -3.031160000000000E+01 / Declination of target (deci. deg)
PA_NOM = 101.9997 / nominal position angle from north to DETY(deg)
MEAN_EA1= 266.869783840619 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 120.311635133016 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 348.000319602287 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-03-08T19:36:03' / Start date of observations
DATE-END= '2014-03-10T01:30:23' / End date of observations
TSTART = 4.476225698188115E+08 / time start
TSTOP = 4.477302104059693E+08 / time stop
TELAPSE = 1.076405871577263E+05 / elapsed time
ONTIME = 5.353507842439413E+04 / On-source time
EXPOSURE= 5.353507842439413E+04 / Exposure time
MJD-OBS = 5.672481752318069E+04 / MJD of data start time
FILIN001= 'ae508059010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae508059010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae508059010xi3_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 detected X-ray emission along the radio shell of G359.0-0.9 located toward the Galactic Center region. The spectral structure shows strong emission like structures at H-like Mg Ly alpha, H-like Si Ly alpha, He-like Ne RRC and He-like Mg RRC. This is the first hint for over ionized plasma in a shell-type SNR. We make three pointing observations with XIS covering the whole of G359.0-0.9 and obtain firm evidence for the ionized plasma.