Suzaku Observation : 705032010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '705032010' / Observation identification string
OBSERVER= 'GRZEGORZ M MADEJSKI' / Principal Investigator
OBJECT = 'CEN A S LOBE NO. 1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 200.8667 / planned target R.A.(deg)
DEC_OBJ = -45.1514 / planned target DEC.(deg)
RA_NOM = 2.008664000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -4.516020000000000E+01 / Declination of target (deci. deg)
PA_NOM = 288.0039 / nominal position angle from north to DETY(deg)
MEAN_EA1= 200.866394380661 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 135.160239548333 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 161.996125723895 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-08-10T15:52:16' / Start date of observations
DATE-END= '2010-08-11T18:37:10' / End date of observations
TSTART = 3.347734750000000E+08 / time start
TSTOP = 3.348670139312091E+08 / time stop
TELAPSE = 9.353893120908737E+04 / elapsed time
ONTIME = 7.516537683343887E+04 / On-source time
EXPOSURE= 7.516537683343887E+04 / Exposure time
MJD-OBS = 5.541869374055555E+04 / MJD of data start time
FILIN001= 'ae705032010xi0_0_3x3n066l_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= 'ae705032010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae705032010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae705032010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae705032010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae705032010xi3_0_5x5n066a_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 a set of four pointings (200 ks), to study the X-ray emission from the Southern giant lobe of the radio galaxy Cen A. Those lobes clearly separated from the central source, have been detected as a source of diffuse gamma-ray emission by the Fermi Telescope. The goal of the Suzaku observations is two-fold: first, to measure the diffuse component of the non-thermal X-ray emission with both the XIS and the HXD in order to determine the details of the distribution of the radiating relativistic particles (and B field), and second, to measure the thermal emission from the lobes (using primarily the XIS), to determine temperature and density of the X-ray emitting plasma, which, via consideration of pressure balance, will determine the content of energetic protons (cosmic rays).