Suzaku Observation : 506059010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '506059010' / Observation identification string
OBSERVER= 'KATSUJI KOYAMA' / Principal Investigator
OBJECT = 'KES 79 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 283.2000 / planned target R.A.(deg)
DEC_OBJ = 0.6861 / planned target DEC.(deg)
RA_NOM = 2.831953000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 6.959000000000000E-01 / Declination of target (deci. deg)
PA_NOM = 73.5801 / nominal position angle from north to DETY(deg)
MEAN_EA1= 283.195291582689 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 89.304148785711 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 16.419875037690 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-04-23T22:38:57' / Start date of observations
DATE-END= '2011-04-25T11:19:13' / End date of observations
TSTART = 3.569157316208298E+08 / time start
TSTOP = 3.570444830000000E+08 / time stop
TELAPSE = 1.287513791702390E+05 / elapsed time
ONTIME = 5.089697206181288E+04 / On-source time
EXPOSURE= 5.089697206181288E+04 / Exposure time
MJD-OBS = 5.567496985885219E+04 / MJD of data start time
FILIN001= 'ae506059010xi0_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= 'ae506059010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae506059010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae506059010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae506059010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae506059010xi3_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:
Suzaku found recombining plasma (RP) from the mixed-morphology SNRs (MM-SNRs). Since the standard evolution of SNR does not predict RP, the Suzaku discovery requires a dramatic change on the scenario of SNR dynamics and evolution. Suggestive facts are that all RP detected SNRs have OH masers and all RP-detected SNRs have TeV/GeV emissions. The most important issue at this stage, however, is not model making, but systematic and comprehensive observations to study which kind of SNRs, and/or which circum SN conditions, are responsible to RP. This is our primary objective. The second aim of this proposal is to provide path-finding data for the Astro-H science.