Suzaku Observation : 710009010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '710009010' / Observation identification string
OBSERVER= 'HIROFUMI NODA' / Principal Investigator
OBJECT = 'NGC 3516' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 166.6979 / planned target R.A.(deg)
DEC_OBJ = 72.5685 / planned target DEC.(deg)
RA_NOM = 1.666817000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 7.255790000000000E+01 / Declination of target (deci. deg)
PA_NOM = 306.0068 / nominal position angle from north to DETY(deg)
MEAN_EA1= 166.681688601248 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 17.442074174831 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 143.993239884869 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2015-05-12T08:01:41' / Start date of observations
DATE-END= '2015-05-15T00:50:12' / End date of observations
TSTART = 4.847355550000000E+08 / time start
TSTOP = 4.849661954020591E+08 / time stop
TELAPSE = 2.306404020591378E+05 / elapsed time
ONTIME = 1.247632091977000E+05 / On-source time
EXPOSURE= 1.247632091977000E+05 / Exposure time
MJD-OBS = 5.715436596277777E+04 / MJD of data start time
FILIN001= 'ae710009010xi0_0_3x3n066s_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae710009010xi0_0_5x5n066s_cl.evt.gz' / Input file name
FILIN003= 'ae710009010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN004= 'ae710009010xi1_0_5x5n130b_cl.evt.gz' / Input file name
FILIN005= 'ae710009010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae710009010xi3_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:
In the AO-8 cycle, we have proposed several X-ray and optical simultaneous observations of a type I Seyfert galaxy NGC 3516, and obtained a good correlation between those wavelengths in its faint phase. The result suggests that a hard primary X-ray continua found in NGC 3516 by Noda et al. (2013) is generated in a corona formed closely to an accretion disk, which is possibly a radiatively inefficient accretion flow. As a next step, we examine whether or not an X-ray variation is also correlated with that in optical, when NGC 3516 is in the bright phase, and the other primary X-ray continuum, also reported by Noda et al. (2013), is dominant. For it, we propose an X-ray and optical simultaneous observation of NGC 3516 with an exposure of 120 ksec, which is triggered by a Swift monitoring.