Suzaku Observation : 505074010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '505074010' / Observation identification string
OBSERVER= 'JOSEPH DAVID GELFAND' / Principal Investigator
OBJECT = 'SNR G304.6+0.1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 196.4583 / planned target R.A.(deg)
DEC_OBJ = -62.6917 / planned target DEC.(deg)
RA_NOM = 1.964463000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -6.269510000000000E+01 / Declination of target (deci. deg)
PA_NOM = 321.0575 / nominal position angle from north to DETY(deg)
MEAN_EA1= 196.446277878663 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 152.695070516269 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 128.942518024337 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-09-03T21:54:15' / Start date of observations
DATE-END= '2010-09-06T12:51:23' / End date of observations
TSTART = 3.368709560000000E+08 / time start
TSTOP = 3.370926696301629E+08 / time stop
TELAPSE = 2.217136301628947E+05 / elapsed time
ONTIME = 9.962973729729652E+04 / On-source time
EXPOSURE= 9.962973729729652E+04 / Exposure time
MJD-OBS = 5.544297014101852E+04 / MJD of data start time
FILIN001= 'ae505074010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 2 / 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= 'ae505074010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae505074010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae505074010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae505074010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae505074010xi3_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:
Galactic supernova remnants are believed to be the primary source of cosmic rays below 10^15.5 eV even though the exact acceleration mechanism remains unknown. This uncertainty results from the lack of remnants with synchrotron X-ray and GeV emission, needed to distinguish accelerated electrons from protons using broadband spectral modeling. An analysis of recent XMM and Fermi data suggests SNR G304.6+0.1 is just the third remnant with both, but the observed hard X-ray excess is also consistent with bremsstrahlung emission. We request a deep Suzaku observation of this source to determine the nature of its hard X-ray emission - critical for identifying the underlying acceleration mechanism.