Suzaku Observation : 404075020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '404075020' / Observation identification string
OBSERVER= 'JON MILLER' / Principal Investigator
OBJECT = 'CYGNUS X-1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 299.5903 / planned target R.A.(deg)
DEC_OBJ = 35.2016 / planned target DEC.(deg)
RA_NOM = 2.995895000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.527210000000000E+01 / Declination of target (deci. deg)
PA_NOM = 91.3103 / nominal position angle from north to DETY(deg)
MEAN_EA1= 299.589482753647 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 54.727877568023 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 358.689744918317 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2009-04-08T06:09:03' / Start date of observations
DATE-END= '2009-04-08T19:44:19' / End date of observations
TSTART = 2.924864259692746E+08 / time start
TSTOP = 2.925334440000000E+08 / time stop
TELAPSE = 4.701803072541952E+04 / elapsed time
ONTIME = 5.332207102000713E+03 / On-source time
EXPOSURE= 5.332207102000713E+03 / Exposure time
MJD-OBS = 5.492926030269993E+04 / MJD of data start time
FILIN001= 'ae404075020xi0_0_2x2b104a_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= 'ae404075020xi0_0_3x3b104a_cl.evt.gz' / Input file name
FILIN003= 'ae404075020xi1_0_3x3b105b_cl.evt.gz' / Input file name
FILIN004= 'ae404075020xi3_0_2x2b106a_cl.evt.gz' / Input file name
FILIN005= 'ae404075020xi3_0_3x3b106a_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:
In both stellar-mass and supermassive black holes, connections between X-ray flux and radio flux hint at disk-jet connections expected theoretically. The next step in this work is to move beyond fluxes, and tie the physical parameters of the disk to radio jet emission. Cygnus X-1 is bright and highly variable in both X-rays and radio bands; moreover, it is the only black hole that always permits two measurements of the disk (through disk continuum and broad Fe K disk line/reflection). We propose to observe Cygnus X-1 on 20 occasions for 15 ksec (each) during AO-4, simultaneously with the updated Ryle radio telescope. This will form a modest Large Program with public data access, and an important legacy dataset for Suzaku. This project addresses NASA Beyond Einstein science goals.