Suzaku Observation : 507035010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '507035010' / Observation identification string
OBSERVER= 'AYA BAMBA' / Principal Investigator
OBJECT = 'G32.8-0.1 NORTH' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 282.8400 / planned target R.A.(deg)
DEC_OBJ = -0.0600 / planned target DEC.(deg)
RA_NOM = 2.828355000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -5.110000000000000E-02 / Declination of target (deci. deg)
PA_NOM = 74.4992 / nominal position angle from north to DETY(deg)
MEAN_EA1= 282.835500768549 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 90.051141994157 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 15.500775460376 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-04-20T14:38:27' / Start date of observations
DATE-END= '2012-04-21T18:57:16' / End date of observations
TSTART = 3.882484370000000E+08 / time start
TSTOP = 3.883493290000000E+08 / time stop
TELAPSE = 1.008920000000000E+05 / elapsed time
ONTIME = 5.514745990812778E+04 / On-source time
EXPOSURE= 5.514745990812778E+04 / Exposure time
MJD-OBS = 5.603761691185185E+04 / MJD of data start time
FILIN001= 'ae507035010xi0_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= 'ae507035010xi0_0_5x5n066h_cl.evt.gz' / Input file name
FILIN003= 'ae507035010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN004= 'ae507035010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN005= 'ae507035010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN006= 'ae507035010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN007= 'ae507035010xi3_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:
A key element to untangle the Galactic origin of the cosmic-ray is the acceleration of high energy particles that occurs in the shocks of the supernova remnants (SNRs). Recent Fermi surveys revealed that particles are more efficiently escaping from the acceleration system when the SNRs get older. However what is still unknown is the plasma condition environment that makes the mechanism more efficient. X-ray observations are an excellent tool to understand the plasma condition but there has not been a systematic X-ray follow-up observations of these Fermi SNRs. The Suzaku Observatory is ideal for such X-ray systematic study because of his low background. We propose here X-ray observations of 4 SNRs detected by Fermi to solve cosmic-ray escape problem.