Suzaku Observation : 507058010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '507058010' / Observation identification string
OBSERVER= 'JUNICHIRO KATSUTA' / Principal Investigator
OBJECT = 'SNR HB3 SE-C' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 36.0250 / planned target R.A.(deg)
DEC_OBJ = 62.4667 / planned target DEC.(deg)
RA_NOM = 3.603580000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 6.245780000000000E+01 / Declination of target (deci. deg)
PA_NOM = 247.4994 / nominal position angle from north to DETY(deg)
MEAN_EA1= 36.035819246721 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 27.542203494743 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 202.500635581793 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-01-31T18:31:12' / Start date of observations
DATE-END= '2013-02-01T03:48:19' / End date of observations
TSTART = 4.129722790201851E+08 / time start
TSTOP = 4.130056826414963E+08 / time stop
TELAPSE = 3.340362131118774E+04 / elapsed time
ONTIME = 2.416962185943127E+04 / On-source time
EXPOSURE= 2.416962185943127E+04 / Exposure time
MJD-OBS = 5.632377249078918E+04 / MJD of data start time
FILIN001= 'ae507058010xi0_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= 'ae507058010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae507058010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae507058010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae507058010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae507058010xi3_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:
We propose to study the large SNR HB3, which is classified as the mixed-morphology SNRs. The Fermi LAT revealed recently bright gamma-ray emissions adjacent to the southeastern shell of HB3, indicating the gamma rays originate in shocked molecular clouds associated with the nearby HII region W3/W4. However it is difficult to determine the gamma-ray origins since the HII regions are dominant in all energy bands except for X-ray. Our aim is to obtain the spatial structure and the temperature of thermal X-ray emissions at this site. These information will help us to understand whether HB3 interacts with molecular clouds. For this purpose, we require high sensitivities and the wide field of view to cover the southeastern shell. Suzaku is an ideal X-ray observatory to achieve this objective.