Suzaku Observation : 505072010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '505072010' / Observation identification string
OBSERVER= 'ESTER ALIU' / Principal Investigator
OBJECT = 'SNR G106.3+2.7 P2' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 336.9500 / planned target R.A.(deg)
DEC_OBJ = 60.9422 / planned target DEC.(deg)
RA_NOM = 3.369121000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 6.094390000000000E+01 / Declination of target (deci. deg)
PA_NOM = 12.2687 / nominal position angle from north to DETY(deg)
MEAN_EA1= 336.912068571978 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 29.056078418549 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 77.731336092260 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2010-08-15T10:09:14' / Start date of observations
DATE-END= '2010-08-16T00:30:13' / End date of observations
TSTART = 3.351822370000000E+08 / time start
TSTOP = 3.352337978826286E+08 / time stop
TELAPSE = 5.156088262856007E+04 / elapsed time
ONTIME = 2.457218886184692E+04 / On-source time
EXPOSURE= 2.457218886184692E+04 / Exposure time
MJD-OBS = 5.542342478222222E+04 / MJD of data start time
FILIN001= 'ae505072010xi0_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= 'ae505072010xi1_0_3x3n069b_cl.evt.gz' / Input file name
FILIN003= 'ae505072010xi3_0_3x3n066a_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:
After two decades searching for the origin of the GeV emission from 3EG J2227+6122, it is now identified with PSR J2229+6114 and its PWN.~This highly energetic young pulsar lies within the arcmin diameter Boomerang radio nebula. Now, recently discovered nearby extended TeV emission suggest a second Vela-like "cocoon" feed by relic electrons from the PWN, blowing out the vast degree-scale radio feature.~Interactions of the SNR shock front with overlapping molecular cloud material can also contribute in the gamma-ray production.~An XIS mosaic will allow us to search for soft and hard X-ray emission similar to Vela's "Cocoon" and resolve the nature of the TeV emission and its connection to the Boomerang and the radio feature.