Suzaku Observation : 706030050
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '706030050' / Observation identification string
OBSERVER= 'JOSEPH NEILSEN' / Principal Investigator
OBJECT = 'SMC X-1 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 19.2715 / planned target R.A.(deg)
DEC_OBJ = -73.4433 / planned target DEC.(deg)
RA_NOM = 1.928280000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -7.344950000000000E+01 / Declination of target (deci. deg)
PA_NOM = 39.2778 / nominal position angle from north to DETY(deg)
MEAN_EA1= 19.282814129724 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 163.449496311528 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 50.722224668429 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-05-25T02:02:40' / Start date of observations
DATE-END= '2011-05-25T16:11:24' / End date of observations
TSTART = 3.596071050000000E+08 / time start
TSTOP = 3.596550732910339E+08 / time stop
TELAPSE = 4.796829103392363E+04 / elapsed time
ONTIME = 1.818228924894333E+04 / On-source time
EXPOSURE= 1.818228924894333E+04 / Exposure time
MJD-OBS = 5.570612001370370E+04 / MJD of data start time
FILIN001= 'ae706030050xi0_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= 'ae706030050xi0_0_5x5n090l_cl.evt.gz' / Input file name
FILIN003= 'ae706030050xi1_0_3x3n091b_cl.evt.gz' / Input file name
FILIN004= 'ae706030050xi1_0_5x5n091b_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 a sequence of 10 18-ks observations of the wind-fed accreting X-ray pulsar SMC X-1. Distributed throughout the orbital and super-orbital period of this high-mass X-ray binary, our proposed observations will reveal the influence of wind accretion on the structure and evolution of accretion disks via three independent methods: (1) mapping the geometry of the accretion flow through soft X-ray emission line variability and ionization studies, (2) tracing the structure of the accretion disk corona with hard X-ray scattering studies, and (3) tracking the evolution of the neutron star spin period and pulse profile for comparison to changes in the warped, precessing accretion disk.