Suzaku Observation : 401032010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '401032010' / Observation identification string
OBSERVER= 'PAOLA TESTA' / Principal Investigator
OBJECT = 'HR 9024 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 357.4207 / planned target R.A.(deg)
DEC_OBJ = 36.4253 / planned target DEC.(deg)
RA_NOM = 3.574125000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.643080000000000E+01 / Declination of target (deci. deg)
PA_NOM = 49.8624 / nominal position angle from north to DETY(deg)
MEAN_EA1= 357.412460454207 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 53.569212633267 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 40.137645235790 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2006-07-23T01:28:49' / Start date of observations
DATE-END= '2006-07-24T14:26:19' / End date of observations
TSTART = 2.069334128677882E+08 / time start
TSTOP = 2.070663635843918E+08 / time stop
TELAPSE = 1.329507166036367E+05 / elapsed time
ONTIME = 5.879970548886061E+04 / On-source time
EXPOSURE= 5.879970548886061E+04 / Exposure time
MJD-OBS = 5.393906339180310E+04 / MJD of data start time
FILIN001= 'ae401032010xi0_0_3x3n000a_cl.evt.gz' / Input file name
SEQPNUM = 3 / 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= 'ae401032010xi0_0_5x5n000a_cl.evt.gz' / Input file name
FILIN003= 'ae401032010xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN004= 'ae401032010xi1_0_5x5n001b_cl.evt.gz' / Input file name
FILIN005= 'ae401032010xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN006= 'ae401032010xi2_0_5x5n000a_cl.evt.gz' / Input file name
FILIN007= 'ae401032010xi3_0_3x3n000a_cl.evt.gz' / Input file name
FILIN008= 'ae401032010xi3_0_5x5n000a_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:
Suzaku-XIS is the best available instrument to study the Fe fluorescence emission from late-type evolved stars. Fe fluorescence is produced by illumination of the photosphere by ionizing coronal X-rays and its intensity depends on the height of the X-ray source. We propose to observe Fe fluorescence in the single G-type giant HR 9024 and in the active RS CVn system II Peg to obtain a direct geometrical constraint on the scale height of their coronal structures. These two stars have the brightest Fe fluorescence features of all the late-type stars observed by the Chandra-HETGS and their different stellar parameters (stellar radius, gravity, multiplicity,..) and evolutionary stage will allow us to probe the typical coronal scale for significantly different conditions.