Suzaku Observation : 404019010

QL FITS Image

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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '404019010'          / Observation identification string
OBSERVER= 'ATSUSHI HARAYAMA'   / Principal Investigator
OBJECT  = 'EUVE J0317-85.5'    / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =              49.2692 / planned target R.A.(deg)
DEC_OBJ =             -85.5431 / planned target DEC.(deg)
RA_NOM  = 4.898640000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -8.550030000000000E+01 / Declination of target (deci. deg)
PA_NOM  =              65.4600 / nominal position angle from north to DETY(deg)
MEAN_EA1=      48.986381565768 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=     175.500341597568 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=      24.540019624643 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2009-07-16T14:26:31' / Start date of observations
DATE-END= '2009-07-18T03:30:16' / End date of observations
TSTART  = 3.010697180000000E+08 / time start
TSTOP   = 3.012011294020281E+08 / time stop
TELAPSE = 1.314114020281434E+05 / elapsed time
ONTIME  = 6.308434964108467E+04 / On-source time
EXPOSURE= 6.308434964108467E+04 / Exposure time
MJD-OBS = 5.502860396046296E+04 / MJD of data start time
FILIN001= 'ae404019010xi0_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= 'ae404019010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae404019010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae404019010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae404019010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae404019010xi3_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:

Where is the particle acceleration site in the universe? The Cosmic-ray origin is the long standing mystery for near 100 years. The first discovery of "the white dwarf pulsar" in the AE Aquarii system with Suzaku is one of the most important step in this study, because Suzaku demonstrated the possibility of particle acceleration in white dwarfs. The next important step is to search for the sign of non-thermal emission from a NORMAL white dwarf. Here, we propose the Suzaku observation of an isolated white dwarf EUVE J0317-85.5, which has very high magnetic field strength of 450 MG and very fast rotation period 725 sec among this type of objects.