Suzaku Observation : 405026010

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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '405026010'          / Observation identification string
OBSERVER= 'YASUYUKI TANAKA'    / Principal Investigator
OBJECT  = 'EMS1150 '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             263.0865 / planned target R.A.(deg)
DEC_OBJ =             -32.7295 / planned target DEC.(deg)
RA_NOM  = 2.630830000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -3.272120000000000E+01 / Declination of target (deci. deg)
PA_NOM  =              91.2452 / nominal position angle from north to DETY(deg)
MEAN_EA1=     263.082954350110 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     122.721229410397 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     358.754760947092 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-02-19T23:54:57' / Start date of observations
DATE-END= '2011-02-20T16:43:24' / End date of observations
TSTART  = 3.514749570000000E+08 / time start
TSTOP   = 3.515342522871428E+08 / time stop
TELAPSE = 5.929528714275360E+04 / elapsed time
ONTIME  = 2.091857487183809E+04 / On-source time
EXPOSURE= 2.091857487183809E+04 / Exposure time
MJD-OBS = 5.561199793037037E+04 / MJD of data start time
FILIN001= 'ae405026010xi0_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= 'ae405026010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae405026010xi3_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:

Fermi discovered a lot of unidentified GeV sources in the Galactic plane. Among them, some of the low-latitude unIDs show "pulsar-like" cutoff power-law spectra with the cutoff energy of 1-5 GeV. We propose to search for X-ray counterparts of these unIDs. Using an X-ray spectral shape and a time variability, we would be able to identify these objects as pulsars. In addition, we search for diffuse X-ray emission around the targets. Finally, we investigate acceleration mechanisms which work in pulsars based on a broadband spectrum from X-ray to GeV.