Suzaku Observation : 407088010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '407088010' / Observation identification string
OBSERVER= 'VICTOR DOROSHENKO' / Principal Investigator
OBJECT = '4U 0352+30' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 58.8462 / planned target R.A.(deg)
DEC_OBJ = 31.0458 / planned target DEC.(deg)
RA_NOM = 5.884270000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 3.104940000000000E+01 / Declination of target (deci. deg)
PA_NOM = 77.7002 / nominal position angle from north to DETY(deg)
MEAN_EA1= 58.842691024676 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 58.950636315078 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 12.299775612706 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-08-27T08:38:37' / Start date of observations
DATE-END= '2012-08-31T02:21:09' / End date of observations
TSTART = 3.993734480000000E+08 / time start
TSTOP = 3.996923950000000E+08 / time stop
TELAPSE = 3.189470000000000E+05 / elapsed time
ONTIME = 1.534893130773902E+05 / On-source time
EXPOSURE= 1.534893130773902E+05 / Exposure time
MJD-OBS = 5.616637861324074E+04 / MJD of data start time
FILIN001= 'ae407088010xi0_0_3x3n090l_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= 'ae407088010xi0_0_5x5n090l_cl.evt.gz' / Input file name
FILIN003= 'ae407088010xi1_0_3x3n140b_cl.evt.gz' / Input file name
FILIN004= 'ae407088010xi1_0_5x5n140b_cl.evt.gz' / Input file name
FILIN005= 'ae407088010xi3_0_3x3n092a_cl.evt.gz' / Input file name
FILIN006= 'ae407088010xi3_0_5x5n092a_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:
After 40 years of studies, surprisingly little is known about accreting pulsars at low-luminosities, yet these may be the most numerous class of neutron star binaries in the Galaxy. Upcoming large-scale surveys will likely reveal many such objects, but to identify them it is crucial to fully understand their properties. X Per, the archetypal source of this class, at 1 kpc from Earth is ideal target for detailed studies. In spite of that X Per is still puzzling. With the proposed program we aim to study X Per in detail, constrain its X-ray spectrum also as a function of the spin phase. Our study will be key to characterize the properties of low-luminosity X-ray pulsars population and will help to identify it in upcoming surveys.