Suzaku Observation : 803039010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '803039010' / Observation identification string
OBSERVER= 'DAVID K STRICKLAND' / Principal Investigator
OBJECT = 'NGC 3079' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 150.4908 / planned target R.A.(deg)
DEC_OBJ = 55.6798 / planned target DEC.(deg)
RA_NOM = 1.504440000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 5.561630000000000E+01 / Declination of target (deci. deg)
PA_NOM = 294.1052 / nominal position angle from north to DETY(deg)
MEAN_EA1= 150.444039114183 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 34.383702481102 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 155.894756161856 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-05-04T17:50:16' / Start date of observations
DATE-END= '2008-05-05T02:45:17' / End date of observations
TSTART = 2.632408120000000E+08 / time start
TSTOP = 2.632707014379909E+08 / time stop
TELAPSE = 2.988943799093366E+04 / elapsed time
ONTIME = 1.440831707254052E+04 / On-source time
EXPOSURE= 1.440831707254052E+04 / Exposure time
MJD-OBS = 5.459076940027778E+04 / MJD of data start time
FILIN001= 'ae803039010xi0_0_3x3n066a_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= 'ae803039010xi0_0_5x5n066a_cl.evt.gz' / Input file name
FILIN003= 'ae803039010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae803039010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae803039010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae803039010xi3_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 will determine whether AGN can drive galactic-scale winds by observing NGC 3079, the best nearby candidate for such a wind. The edge-on spiral NGC 3079 hosts a Compton-thick AGN and is surrounded by a 40 kpc-scale soft X-ray nebula, the largest manifestation of outflow activity also seen in the optical and radio. Proving the outflow is AGN-driven requires Suzaku's unique abilities. We will measure the AGN luminosity using the HXD in the 15-40 keV range and the 2-10 keV band reflection spectrum to assess whether the AGN can radiatively-or-mechanically power the observed superwind. We will determine the origin of the soft X-ray nebula using the relative elemental abundances in the plasma. We can also detect any significant starburst through the 6.7 keV line emission it would create.