Suzaku Observation : 401092010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '401092010' / Observation identification string
OBSERVER= 'SANDRO MEREGHETTI' / Principal Investigator
OBJECT = 'SGR 1806-20' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 272.1638 / planned target R.A.(deg)
DEC_OBJ = -20.4110 / planned target DEC.(deg)
RA_NOM = 2.721660000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -2.047290000000000E+01 / Declination of target (deci. deg)
PA_NOM = 269.9473 / nominal position angle from north to DETY(deg)
MEAN_EA1= 272.165951745218 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 110.472893305201 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 180.052726445039 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2006-09-09T22:13:43' / Start date of observations
DATE-END= '2006-09-11T04:00:14' / End date of observations
TSTART = 2.111586250212495E+08 / time start
TSTOP = 2.112623950014531E+08 / time stop
TELAPSE = 1.037699802035987E+05 / elapsed time
ONTIME = 4.893152961161733E+04 / On-source time
EXPOSURE= 4.893152961161733E+04 / Exposure time
MJD-OBS = 5.398796631024594E+04 / MJD of data start time
FILIN001= 'ae401092010xi0_0_3x3n000a_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae401092010xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN003= 'ae401092010xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN004= 'ae401092010xi3_0_3x3n000a_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 soft gamma-ray repeater SGR 1806-20 has recently emitted the most powerful giant flare ever observed from these sources. This probably involved a large scale restructuring of the magnetosphere, leading to observable variations in the properties of its persistent emission, from IR to hard X-rays. We propose to observe SGR 1806-20 with Suzaku considering the unique opportunity offered by this satellite to study the spectrum of this source simultaneously both in the soft and hard X-ray bands. We also suggest to coordinate this observation with a simultaneous XMM-Newton one, in order to obtain a significantly better determination of the broad band spectral parameters.