Suzaku Observation : 405036010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '405036010' / Observation identification string
OBSERVER= 'MARINA ORIO' / Principal Investigator
OBJECT = 'V2491 CYG' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 295.7582 / planned target R.A.(deg)
DEC_OBJ = 32.3205 / planned target DEC.(deg)
RA_NOM = 2.957679000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.230680000000000E+01 / Declination of target (deci. deg)
PA_NOM = 253.6206 / nominal position angle from north to DETY(deg)
MEAN_EA1= 295.767872345858 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 57.693228850047 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 196.379418737159 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-11-03T10:32:11' / Start date of observations
DATE-END= '2010-11-05T06:30:13' / End date of observations
TSTART = 3.420965130000000E+08 / time start
TSTOP = 3.422536110000000E+08 / time stop
TELAPSE = 1.570980000000000E+05 / elapsed time
ONTIME = 7.440042289531231E+04 / On-source time
EXPOSURE= 7.440042289531231E+04 / Exposure time
MJD-OBS = 5.550345112481481E+04 / MJD of data start time
FILIN001= 'ae405036010xi0_0_3x3n066l_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= 'ae405036010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae405036010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae405036010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae405036010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae405036010xi3_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:
We propose to observe again one of the most luminous and intriguing classical novae of the last two years, after it has returned to quiescence. The goala are to understand how accretion is re-estabilished, investigate the claim that the white dwarf an intermediate polar (IP), estimate mass accretion are and white dwarf mass. IP are a class of X-ray sources that Suzaku is ideally suited to study, and we want to study the influence of the magnetic field on the nova evolution.