Suzaku Observation : 707043010

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UDON2 to quickly extract spectrum and light-curve
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Fits Header

TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '707043010'          / Observation identification string
OBSERVER= 'SVETLANA G. JORSTAD' / Principal Investigator
OBJECT  = '3C345   '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             250.7450 / planned target R.A.(deg)
DEC_OBJ =              39.8103 / planned target DEC.(deg)
RA_NOM  = 2.507487000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.979450000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             267.7320 / nominal position angle from north to DETY(deg)
MEAN_EA1=     250.748693669677 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      50.205461342276 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     182.268048903313 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-09-11T06:28:26' / Start date of observations
DATE-END= '2012-09-11T11:27:13' / End date of observations
TSTART  = 4.006601450000000E+08 / time start
TSTOP   = 4.006780207891829E+08 / time stop
TELAPSE = 1.787578918290138E+04 / elapsed time
ONTIME  = 1.271678918290138E+04 / On-source time
EXPOSURE= 1.271678918290138E+04 / Exposure time
MJD-OBS = 5.618127093962963E+04 / MJD of data start time
FILIN001= 'ae707043010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM =                    2 / Number of times this dataset processed
PROCVER = '3.0.22.44'          / Processing script version
MK1STVER= 'mk1stfits20120530'  / Version of mk1stfits used
SOFTVER = 'Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22' / Version of HEADAS used
CALDBVER= 'hxd20110913_xis20160607_xrt20110630_xrs20060410' / Version of CALDB u
FILIN002= 'ae707043010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae707043010xi3_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 to perform two 2-week multi-frequency campaigns of observations of a sample of gamma-ray blazars during Fermi Cycle 5. The campaigns will involve: (1) gamma-ray monitoring with the Fermi LAT, (2) VLBA total and polarized intensity imaging at 43 GHz 3 times per campaign, (3) daily optical photometric B, V, R, and I measurements, (4) R-band polarimetric observations, (5) X-ray observations with Suzaku and Swift; (6) mid-IR measurements with IRTF; and (7) near-IR photometric J, H, and K observations. The research aims i) to search for correlated variability on short timescales; ii) to compile SEDs at different states of gamma-ray and radio jet activitiy; and iii) to explore mechanisms of high energy production and locations of gamma-ray emission regions in blazars.