Suzaku Observation : 407015020
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '407015020' / Observation identification string
OBSERVER= 'SHINYA YAMADA' / Principal Investigator
OBJECT = 'CYG X-1 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 299.5907 / planned target R.A.(deg)
DEC_OBJ = 35.1892 / planned target DEC.(deg)
RA_NOM = 2.995787000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.520240000000000E+01 / Declination of target (deci. deg)
PA_NOM = 59.5691 / nominal position angle from north to DETY(deg)
MEAN_EA1= 299.578716833107 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 54.797645192622 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 30.430928648418 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2013-05-07T02:13:17' / Start date of observations
DATE-END= '2013-05-07T14:34:19' / End date of observations
TSTART = 4.212080830000000E+08 / time start
TSTOP = 4.212499649442136E+08 / time stop
TELAPSE = 4.188194421362877E+04 / elapsed time
ONTIME = 3.244213010132313E+03 / On-source time
EXPOSURE= 3.244213010132313E+03 / Exposure time
MJD-OBS = 5.641909429611111E+04 / MJD of data start time
FILIN001= 'ae407015020xi0_0_2x2b122l_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= 'ae407015020xi0_0_2x2n066l_cl.evt.gz' / Input file name
FILIN003= 'ae407015020xi1_0_3x3b120b_cl.evt.gz' / Input file name
FILIN004= 'ae407015020xi1_0_3x3n130b_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 Cyg X-1 for 85 ks, utilizing P-sum mode for XIS3. Our aim is to perform shot analysis, which is originally invented by Negoro et al. 1995 with Ginga, and obtain high-quality wide-band spectra for several phases in less than 1 sec; for example, 0.1 sec before the peak, +/- 0.05 sec at the peak, and after the peak. With these spectra, we will quantify changes in five spectral components: hard Comptonization, soft Comptonization, disk emission, Fe-K lines, and reflection. This will be a clue to know long-standing mystery on rapid variability in black holes.