Suzaku Observation : 402003010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '402003010' / Observation identification string
OBSERVER= 'HIDEYUKI MORI' / Principal Investigator
OBJECT = '1RXSJ174459.5-172640' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 266.2479 / planned target R.A.(deg)
DEC_OBJ = -17.4444 / planned target DEC.(deg)
RA_NOM = 2.662467000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -1.744060000000000E+01 / Declination of target (deci. deg)
PA_NOM = 101.0461 / nominal position angle from north to DETY(deg)
MEAN_EA1= 266.246652089732 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 107.440611394472 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 348.953920729151 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-03-30T15:07:47' / Start date of observations
DATE-END= '2008-03-31T14:00:14' / End date of observations
TSTART = 2.602048782283870E+08 / time start
TSTOP = 2.602871978404041E+08 / time stop
TELAPSE = 8.231961201703548E+04 / elapsed time
ONTIME = 4.360325359794497E+04 / On-source time
EXPOSURE= 4.360325359794497E+04 / Exposure time
MJD-OBS = 5.455563127792114E+04 / MJD of data start time
FILIN001= 'ae402003010xi0_0_3x3n066a_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= 'ae402003010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae402003010xi3_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 study wide-band X-ray properties of 5 unidentified sources with luminosities of ~10^35 erg/s, which were detected in the ROSAT All Sky Survey. These sources are a part of the complete X-ray sample in the luminosity range > 10^34 erg/s in the Galactic bulge constructed by Mori (2005). Our goal is to obtain, for the first time, a clear picture about X-ray populations in the bulge, by utilizing the Suzaku fine spectra together with optical identifications. This is a new step toward understanding the formation history of the bulge. Furthermore, because the luminosity range we observe corresponds to a "missing link" region ever studied for a neutron star or black-hole X-ray binary, our results are also unique to test acrretion disk theories at intermediate mass accretion rates.