Suzaku Observation : 406010030
QL FITS Image
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '406010030' / Observation identification string
OBSERVER= 'KAZUTAKA YAMAOKA' / Principal Investigator
OBJECT = 'AQL X-1 ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 287.8169 / planned target R.A.(deg)
DEC_OBJ = 0.5849 / planned target DEC.(deg)
RA_NOM = 2.878278000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 5.718000000000000E-01 / Declination of target (deci. deg)
PA_NOM = 243.2618 / nominal position angle from north to DETY(deg)
MEAN_EA1= 287.827766586178 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 89.428190101150 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 206.738239396559 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2011-10-24T17:26:47' / Start date of observations
DATE-END= '2011-10-25T13:53:19' / End date of observations
TSTART = 3.727959430693279E+08 / time start
TSTOP = 3.728659755602395E+08 / time stop
TELAPSE = 7.003249091160297E+04 / elapsed time
ONTIME = 9.634404268383980E+03 / On-source time
EXPOSURE= 9.634404268383980E+03 / Exposure time
MJD-OBS = 5.585876860246907E+04 / MJD of data start time
FILIN001= 'ae406010030xi0_0_2x2b104l_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= 'ae406010030xi1_0_3x3b137b_cl.evt.gz' / Input file name
FILIN003= 'ae406010030xi3_0_2x2b106a_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 the neutron star binary Aql X-1 during the initial outburst phase with Suzaku ToO. The initial outburst phase is very important for studying the spectral state transition and jet ejections in the accretion physics. However, a detailed study of this phase has not been done much yet due to the insufficient sky coverage and sensitivity of the all-sky monitors. The current MAXI/GSC, Swift/BAT and RXTE/ASM+PCA survey has a very good sensitivity and sky coverage, which can promptly trigger the pointed X-ray observations. Suzaku high-sensitive broadband observations and possible radio coordinated observations will reveals us to establish the unified picture in accretion disks and jets in X-ray binaries, which are independent of the central object.