Suzaku Observation : 705035010

QL FITS Image

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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '705035010'          / Observation identification string
OBSERVER= 'GRZEGORZ M MADEJSKI' / Principal Investigator
OBJECT  = 'CEN A S LOBE NO. 4' / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             196.7500 / planned target R.A.(deg)
DEC_OBJ =             -45.1360 / planned target DEC.(deg)
RA_NOM  = 1.967510000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -4.514360000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             288.0039 / nominal position angle from north to DETY(deg)
MEAN_EA1=     196.750954584406 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     135.143606688238 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     161.996093568924 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-08-13T08:21:01' / Start date of observations
DATE-END= '2010-08-13T16:10:12' / End date of observations
TSTART  = 3.350034770000000E+08 / time start
TSTOP   = 3.350309979095575E+08 / time stop
TELAPSE = 2.752090955746174E+04 / elapsed time
ONTIME  = 2.065799884933233E+04 / On-source time
EXPOSURE= 2.065799884933233E+04 / Exposure time
MJD-OBS = 5.542135580074074E+04 / MJD of data start time
FILIN001= 'ae705035010xi0_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= 'ae705035010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae705035010xi3_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 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).