Suzaku Observation : 501082010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '501082010' / Observation identification string
OBSERVER= 'Q. DANIEL WANG' / Principal Investigator
OBJECT = 'SNR G93.3+6.9 S3' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 313.2708 / planned target R.A.(deg)
DEC_OBJ = 55.2361 / planned target DEC.(deg)
RA_NOM = 3.131710000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 5.528010000000000E+01 / Declination of target (deci. deg)
PA_NOM = 40.0152 / nominal position angle from north to DETY(deg)
MEAN_EA1= 313.170962565651 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 34.719946750901 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 49.984817685928 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2006-06-20T10:19:16' / Start date of observations
DATE-END= '2006-06-20T17:26:19' / End date of observations
TSTART = 2.041139623473006E+08 / time start
TSTOP = 2.041389390000000E+08 / time stop
TELAPSE = 2.497665269935131E+04 / elapsed time
ONTIME = 1.635865269935131E+04 / On-source time
EXPOSURE= 1.635865269935131E+04 / Exposure time
MJD-OBS = 5.390643086263079E+04 / MJD of data start time
FILIN001= 'ae501082010xi0_0_3x3n000a_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae501082010xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN003= 'ae501082010xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN004= 'ae501082010xi3_0_3x3n000a_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 high-latitude supernova remnant G93.3+6.9 (DA 530), with a well-defined shell-like radio morphology and an exceptionally small ratio of X-ray to radio luminosities, evolves in a very low density medium. We propose Suzaku raster observations to map out the remnant. We will examine the type of the supernova and the X-ray radiation mechanism as well as the thermal, chemical and ionization states of the remnant. We will also spectroscopically characterize an extended hard X-ray emission feature, detected in a Chandra observation and spatially coincident with a radio peak near the remnant center, to test the hypothesis that it is a pulsar wind nebula. This study will facilitate an unprecedented test of our understanding of supernova remnants in a very low density environment.