Suzaku Observation : 703023020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '703023020' / Observation identification string
OBSERVER= 'TRACEY JANE TURNER' / Principal Investigator
OBJECT = 'NGC 4051' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 180.7901 / planned target R.A.(deg)
DEC_OBJ = 44.5313 / planned target DEC.(deg)
RA_NOM = 1.807952000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 4.453930000000000E+01 / Declination of target (deci. deg)
PA_NOM = 126.4079 / nominal position angle from north to DETY(deg)
MEAN_EA1= 180.795212862195 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 45.460712209940 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 323.592073638248 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2008-11-23T16:48:00' / Start date of observations
DATE-END= '2008-11-25T13:43:43' / End date of observations
TSTART = 2.807741194807228E+08 / time start
TSTOP = 2.809358150000000E+08 / time stop
TELAPSE = 1.616955192771554E+05 / elapsed time
ONTIME = 7.839388047373295E+04 / On-source time
EXPOSURE= 7.839388047373295E+04 / Exposure time
MJD-OBS = 5.479370119982318E+04 / MJD of data start time
FILIN001= 'ae703023020xi0_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= 'ae703023020xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae703023020xi3_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 powerful combination of Principal Components Analysis with time-resolved X-ray spectroscopy of Seyfert AGN has shown strong evidence that changes in a complex absorber are the origin of much of observed AGN spectral and flux variability. Large column, high ionization layers of gas may arise in a disk wind, representing a significant new, and possibly dominant, component, responsible for shaping the X-ray spectrum of AGN. The broad bandpass of Suzaku gives us a unique opportunity to model primary and reflected continua and the effects of variable absorbing zones, and test wind and other models. We propose a long 340 ks exposure on the NLSy1 NGC 4051 whose large amplitude of variability and well-studied complex absorption will test those models to the limit