Suzaku Observation : 707042010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '707042010' / Observation identification string
OBSERVER= 'SVETLANA G. JORSTAD' / Principal Investigator
OBJECT = '0836+710' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 130.3517 / planned target R.A.(deg)
DEC_OBJ = 70.8951 / planned target DEC.(deg)
RA_NOM = 1.303582000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 7.090910000000000E+01 / Declination of target (deci. deg)
PA_NOM = 111.9979 / nominal position angle from north to DETY(deg)
MEAN_EA1= 130.358229858659 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 19.090906181165 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 338.002140737807 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-10-13T14:28:26' / Start date of observations
DATE-END= '2012-10-13T19:44:13' / End date of observations
TSTART = 4.034567460000000E+08 / time start
TSTOP = 4.034720400000000E+08 / time stop
TELAPSE = 1.529400000000000E+04 / elapsed time
ONTIME = 1.061300000000000E+04 / On-source time
EXPOSURE= 1.061300000000000E+04 / Exposure time
MJD-OBS = 5.621363900675926E+04 / MJD of data start time
FILIN001= 'ae707042010xi0_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= 'ae707042010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae707042010xi3_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.