Suzaku Observation : 509070010

QL FITS Image

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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '509070010'          / Observation identification string
OBSERVER= 'JACCO VINK'         / Principal Investigator
OBJECT  = '3C400.2 SE'         / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             294.8250 / planned target R.A.(deg)
DEC_OBJ =              17.1111 / planned target DEC.(deg)
RA_NOM  = 2.948215000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 1.712130000000000E+01 / Declination of target (deci. deg)
PA_NOM  =              81.5889 / nominal position angle from north to DETY(deg)
MEAN_EA1=     294.821474629620 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      72.878691495081 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=       8.411148883802 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-04-23T22:36:02' / Start date of observations
DATE-END= '2014-04-24T11:25:13' / End date of observations
TSTART  = 4.516077738283070E+08 / time start
TSTOP   = 4.516532414353706E+08 / time stop
TELAPSE = 4.546760706359148E+04 / elapsed time
ONTIME  = 2.496270705461502E+04 / On-source time
EXPOSURE= 2.496270705461502E+04 / Exposure time
MJD-OBS = 5.677094256958688E+04 / MJD of data start time
FILIN001= 'ae509070010xi0_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= 'ae509070010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae509070010xi3_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:

Mixed morphology supernova remnants are an important, but peculiar class of supernova remnants. They have a shell-type morphology in the radio, but the X-ray emission is centrally dominated. X-ray spectroscopy of several of these supernova remnants, indicate that their central plasma is often over-ionised and have enhanced abundances. Here we propose to study a typical member of this class, which has so far not received much attention, despite being bright and only mildly absorbed: 3C400.2. The remnant can be covered with four pointings, and is bright enough for imaging spectroscopy on the scale of the Suzaku PSF. This will enable us to study spectroscopic variation, confirm the preliminary detection of an RRC and map its distribution, and study the abundances.