Suzaku Observation : 405038010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '405038010' / Observation identification string
OBSERVER= 'YASUNOBU UCHIYAMA' / Principal Investigator
OBJECT = 'PSR B1259-63' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 195.6970 / planned target R.A.(deg)
DEC_OBJ = -63.8360 / planned target DEC.(deg)
RA_NOM = 1.956913000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -6.383560000000000E+01 / Declination of target (deci. deg)
PA_NOM = 117.5773 / nominal position angle from north to DETY(deg)
MEAN_EA1= 195.691308631263 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 153.835632357632 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 332.422650798712 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-02-02T04:37:35' / Start date of observations
DATE-END= '2011-02-02T10:46:14' / End date of observations
TSTART = 3.499372623762855E+08 / time start
TSTOP = 3.499587564976717E+08 / time stop
TELAPSE = 2.149412138622999E+04 / elapsed time
ONTIME = 2.149412138622999E+04 / On-source time
EXPOSURE= 2.149412138622999E+04 / Exposure time
MJD-OBS = 5.559420053889219E+04 / MJD of data start time
FILIN001= 'ae405038010xi0_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= 'ae405038010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae405038010xi3_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 a gamma-ray binary PSR B1259-63 during the pulsar's second disk crossing after periastron passage. PSR B1259-63 is a young radio pulsar orbiting around a B2e star with a highly eccentric 3.4 yr orbit. Suzaku XIS+HXD measurements of the hard continuum emission from the binary system allow us to investigate particle acceleration in a highly variable environment as a result of interactions between the relativistic wind of the pulsar and the circumstellar disk of the Be star. With the advent of the Fermi Gamma-ray Space Telescope, we will be able to simultaneously observe X-rays and GeV gamma-rays during the disk transit for the first time. The observations of PSR B1259-63 will give us a unique opportunity to study the physics of pulsar winds on AU-scale.