Suzaku Observation : 402061010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '402061010' / Observation identification string
OBSERVER= 'DAVID MILES SMITH' / Principal Investigator
OBJECT = 'IGR J17544-2619' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 268.6071 / planned target R.A.(deg)
DEC_OBJ = -26.3328 / planned target DEC.(deg)
RA_NOM = 2.686038000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.633140000000000E+01 / Declination of target (deci. deg)
PA_NOM = 84.5765 / nominal position angle from north to DETY(deg)
MEAN_EA1= 268.603831157807 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 116.331409045445 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 5.423537351230 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-03-19T12:37:56' / Start date of observations
DATE-END= '2008-03-22T06:20:14' / End date of observations
TSTART = 2.592455319685283E+08 / time start
TSTOP = 2.594820039494441E+08 / time stop
TELAPSE = 2.364719809157848E+05 / elapsed time
ONTIME = 1.038332575907409E+05 / On-source time
EXPOSURE= 1.038332575907409E+05 / Exposure time
MJD-OBS = 5.454452773324685E+04 / MJD of data start time
FILIN001= 'ae402061010xi0_0_3x3n090a_cl.evt.gz' / Input file name
SEQPNUM = 2 / Number of times this dataset processed
PROCVER = '3.0.22.43' / Processing script version
MK1STVER= 'mk1stfits20120530' / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20151005_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae402061010xi0_0_5x5n090a_cl.evt.gz' / Input file name
FILIN003= 'ae402061010xi1_0_3x3n091b_cl.evt.gz' / Input file name
FILIN004= 'ae402061010xi1_0_5x5n091b_cl.evt.gz' / Input file name
FILIN005= 'ae402061010xi3_0_3x3n092a_cl.evt.gz' / Input file name
FILIN006= 'ae402061010xi3_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:
Supergiant Fast X-ray Transients are a newly-discovered class of x-ray binary with short outbursts and late O to early B supergiant companions. They are not persistently bright, but the nature of their low-level variability is not well known. Similarly short outbursts are also seen in bright HMXBs with supergiant companions such as Cyg X-1 and Vel X-1. The mechanism of these outbursts is unknown in all cases. We propose long pointings to the two best-studied SFXTs and a third object, XTE J1743-363, which seems to be transitional between SFXTs and persistent supergiant HMXBs. We will characterize their variability at low flux levels, both to understand the accretion mechanism and to enable surveys of archival data for new SFXTs.