Suzaku Observation : 806007010

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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '806007010'          / Observation identification string
OBSERVER= 'KENTARO SOMEYA'     / Principal Investigator
OBJECT  = 'SNR B0532-675'      / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =              83.1000 / planned target R.A.(deg)
DEC_OBJ =             -67.5300 / planned target DEC.(deg)
RA_NOM  = 8.307660000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -6.753500000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             140.0497 / nominal position angle from north to DETY(deg)
MEAN_EA1=      83.076584734276 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     157.535035529671 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     309.950290866740 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-11-06T15:06:34' / Start date of observations
DATE-END= '2011-11-09T03:46:10' / End date of observations
TSTART  = 3.739072790000000E+08 / time start
TSTOP   = 3.741249750000000E+08 / time stop
TELAPSE = 2.176960000000000E+05 / elapsed time
ONTIME  = 8.249086666774750E+04 / On-source time
EXPOSURE= 8.249086666774750E+04 / Exposure time
MJD-OBS = 5.587163128685185E+04 / MJD of data start time
FILIN001= 'ae806007010xi0_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= 'ae806007010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae806007010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae806007010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae806007010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae806007010xi3_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:

Interstellar medium (ISM) heated by a forward shock of supernova remnants (SNRs) gives us a unique opportunity to study local metal abundance and density. Systematic study of the shock-heated ISM in a galaxy unveils its overall metal distribution and provides a key to understand its chemical evolution. On the basis of this idea, we have performed observations of SNRs in the Large Magellanic Cloud (LMC). We here propose to observe the LMC SNR B0532-675 for 80 ks. Since it locates near the star formation region LH76, we expect that we can study the process of metal diffusion from a star forming region by utilizing the result from another SNR DEM L241 near LH76 already observed.