Suzaku Observation : 504066010

QL FITS Image

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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '504066010'          / Observation identification string
OBSERVER= 'HIDEAKI KATAGIRI'   / Principal Investigator
OBJECT  = 'W51NW   '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             290.6843 / planned target R.A.(deg)
DEC_OBJ =              14.2018 / planned target DEC.(deg)
RA_NOM  = 2.906858000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 1.421330000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             105.4558 / nominal position angle from north to DETY(deg)
MEAN_EA1=     290.685819569302 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      75.786745585260 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     344.544153958807 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-03-28T11:44:41' / Start date of observations
DATE-END= '2010-03-29T13:19:12' / End date of observations
TSTART  = 3.230919354818952E+08 / time start
TSTOP   = 3.231839354699814E+08 / time stop
TELAPSE = 9.199998808616400E+04 / elapsed time
ONTIME  = 4.412048795497417E+04 / On-source time
EXPOSURE= 4.412048795497417E+04 / Exposure time
MJD-OBS = 5.528349073687378E+04 / MJD of data start time
FILIN001= 'ae504066010xi0_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= 'ae504066010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae504066010xi3_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:

We propose to observe the supernova remnant (SNR) W51C with Suzaku XIS. The thermal energy of plasma in W51C, ~3x10^51ergs, is much larger than typical kinetic energy of supernova and can give a large amount of energy to cosmic-ray acceleration. The SNR interactes with the giant molecler cloud and is expected to emit gamma-rays from cosmic-ray interaction. We search for non-thermal X-ray diffuse emission from electron bremsstrahlung or synchrotron emission of secondary electrons produced by decaying charged pions created by p-p interaction.