Suzaku Observation : 509024010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '509024010' / Observation identification string
OBSERVER= 'AKIHIRO TAKATA' / Principal Investigator
OBJECT = 'G166.0+4.3_SE' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 81.6683 / planned target R.A.(deg)
DEC_OBJ = 42.6506 / planned target DEC.(deg)
RA_NOM = 8.166690000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 4.265370000000000E+01 / Declination of target (deci. deg)
PA_NOM = 85.0186 / nominal position angle from north to DETY(deg)
MEAN_EA1= 81.666913114927 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 47.346344770375 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 4.981360250640 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-09-21T05:46:00' / Start date of observations
DATE-END= '2014-09-22T00:30:11' / End date of observations
TSTART = 4.645935736839038E+08 / time start
TSTOP = 4.646609952823933E+08 / time stop
TELAPSE = 6.742159848946333E+04 / elapsed time
ONTIME = 3.427309418863058E+04 / On-source time
EXPOSURE= 3.427309418863058E+04 / Exposure time
MJD-OBS = 5.692124117902666E+04 / MJD of data start time
FILIN001= 'ae509024010xi0_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= 'ae509024010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae509024010xi3_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:
Rarefaction by a blow-out is an important candidate for the formation of recombining plasmas discovered recently in several SNRs. G166.0+4.3 (G166 hereafter) is a unique SNR with which we can examine it. The morphology suggests that the shell of G166 follows the normal evolutional scenario of SNR and the wing is formed by blow-out into cavity on the way of the evolution. Observing G166 with Suzaku as a laboratory of recombining plasma, 1) we examine if a recombining plasma in a SNR is created through rarefaction by blow-out. 2) We construct a model of creation of a recombining plasma in a SNR. Using the parameters of G166 such as age and SN energy obtained from the shell, we reconstruct the recombining plasma created by the blow-out in the wing and compare it with the observation.