Suzaku Observation : 504076010


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UDON2 to quickly extract spectrum and light-curve
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Fits Header
TELESCOP= 'SUZAKU  '           / Telescope (mission) name
OBS_ID  = '504076010'          / Observation identification string
OBSERVER= 'STEVEN L SNOWDEN'   / Principal Investigator
OBJECT  = 'NEP #4  '           / Name of observed object
OBS_REM = '        '           / remark on observation
RA_OBJ  =             270.0000 / planned target R.A.(deg)
DEC_OBJ =              66.5700 / planned target DEC.(deg)
RA_NOM  = 2.700449000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 6.657880000000000E+01 / Declination of target (deci. deg)
PA_NOM  =             165.3654 / nominal position angle from north to DETY(deg)
MEAN_EA1=     270.044893452039 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2=      23.421209460980 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3=     284.634550300347 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2009-12-28T09:57:09' / Start date of observations
DATE-END= '2009-12-29T10:59:24' / End date of observations
TSTART  = 3.153110680000000E+08 / time start
TSTOP   = 3.153995442296321E+08 / time stop
TELAPSE = 8.847622963213921E+04 / elapsed time
ONTIME  = 4.985712610733509E+04 / On-source time
EXPOSURE= 4.985712610733509E+04 / Exposure time
MJD-OBS = 5.519343440027777E+04 / MJD of data start time
FILIN001= 'ae504076010xi0_0_3x3n066l_cl.evt.gz' / Input file name
SEQPNUM =                    2 / Number of times this dataset processed
PROCVER = ''          / 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= 'ae504076010xi0_0_5x5n066l_cl.evt.gz' / Input file name
FILIN003= 'ae504076010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN004= 'ae504076010xi1_0_5x5n069b_cl.evt.gz' / Input file name
FILIN005= 'ae504076010xi3_0_3x3n066a_cl.evt.gz' / Input file name
FILIN006= 'ae504076010xi3_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


We propose a series of four coupled north and south ecliptic pole pointings to observe solar wind charge exchange (SWCX) emission from the interplanetary density enhancement of the He focusing cone. The purpose of the observations is to test, verify, and calibrate models for diffuse X-ray emission from the heliosphere, the source of both a significant contamination for observations of extended structures in the cosmic diffuse X-ray background as well as a source of diagnostic information for the solar wind and structure within the solar system. A well-calibrated model for heliospheric SWCX emission can be used to untangle the very local and more distant components of the observed soft X-ray background affecting our understanding of the Milky Way and the local universe.