Suzaku Observation : 809001100
QL FITS Image
HTTP dir
for public data including pipe-line products
SUZAKU MASTER for master database
UDON2 to quickly extract spectrum and light-curve
JUDO2 to show the pointing position and compare with other data
Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '809001100' / Observation identification string
OBSERVER= 'YOSHIHIRO UEDA' / Principal Investigator
OBJECT = 'THE MOON' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 17.8708 / planned target R.A.(deg)
DEC_OBJ = 7.6666 / planned target DEC.(deg)
RA_NOM = 1.786780000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = 7.668500000000000E+00 / Declination of target (deci. deg)
PA_NOM = 73.8004 / nominal position angle from north to DETY(deg)
MEAN_EA1= 17.867789504783 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 82.331483286920 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 16.199621801642 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2014-07-18T11:36:56' / Start date of observations
DATE-END= '2014-07-18T15:45:23' / End date of observations
TSTART = 4.590001930000000E+08 / time start
TSTOP = 4.590135101583762E+08 / time stop
TELAPSE = 1.331715837621689E+04 / elapsed time
ONTIME = 8.264158376216888E+03 / On-source time
EXPOSURE= 8.264158376216888E+03 / Exposure time
MJD-OBS = 5.685650297666666E+04 / MJD of data start time
FILIN001= 'ae809001100xi0_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= 'ae809001100xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae809001100xi3_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:
The Cosmic X-ray Background (CXB) was discovered almost 50 years ago. Despite many attempts to measure its spectrum, the normalization of the spectrum of the CXB in the 2-10 keV band has considerable uncertainty, of the order of 30% or more. The CXB represents an important integral of the total accretion power of supermassive black holes. We propose to use the dark side of the Moon as a shutter, thereby enabling a clear and unambiguous measurement of the CXB to be made with Suzaku. The motion of the Moon during a 45 ks observation extends over 5 deg, so by tracking the Moon we shall obtain an angle-averaged spectrum. Data from the Moon itself will be analysed and mosaicked to form an X-ray colour image highlighting different fluorescent lines from the bright side.