Suzaku Observation : 409016010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '409016010' / Observation identification string
OBSERVER= 'HIDEYUKI MORI' / Principal Investigator
OBJECT = '1RXSJ170856.9-235936' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 257.2371 / planned target R.A.(deg)
DEC_OBJ = -23.9933 / planned target DEC.(deg)
RA_NOM = 2.572347000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.399310000000000E+01 / Declination of target (deci. deg)
PA_NOM = 95.2085 / nominal position angle from north to DETY(deg)
MEAN_EA1= 257.234663723249 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 113.993069257063 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 354.791505327928 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2015-03-18T06:38:15' / Start date of observations
DATE-END= '2015-03-18T14:28:22' / End date of observations
TSTART = 4.799790270000000E+08 / time start
TSTOP = 4.800040858454822E+08 / time stop
TELAPSE = 2.505884548217058E+04 / elapsed time
ONTIME = 1.538484548217058E+04 / On-source time
EXPOSURE= 1.538484548217058E+04 / Exposure time
MJD-OBS = 5.709931355537037E+04 / MJD of data start time
FILIN001= 'ae409016010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae409016010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae409016010xi3_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 6 unidentified sources with luminosities of ~10^35 erg/s. These sources are a part of the first complete X-ray sample in the luminosity range > 10^34 erg/s in the Galactic bulge, that is constructed from the detected sources in the ROSAT All Sky Survey (Mori 2005, PhD. thesis). Our goal is to obtain, for the first time, a clear picture about X-ray populations in the bulge, by utilizing the fine Suzaku spectra together with follow-up optical identifications. This is a new step toward understanding the formation history of the bulge, and hence that of galaxies with various Hubble sequences in the universe.