Suzaku Observation : 501091010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '501091010' / Observation identification string
OBSERVER= 'ROSA MURPHY WILLIAMS' / Principal Investigator
OBJECT = 'N11 SB ' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 74.2125 / planned target R.A.(deg)
DEC_OBJ = -66.4067 / planned target DEC.(deg)
RA_NOM = 7.418230000000000E+01 / Right Ascension of target (deci. deg)
DEC_NOM = -6.641200000000001E+01 / Declination of target (deci. deg)
PA_NOM = 146.4320 / nominal position angle from north to DETY(deg)
MEAN_EA1= 74.182301079043 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 156.412045535146 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 303.568046215913 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2006-11-07T10:34:39' / Start date of observations
DATE-END= '2006-11-08T05:34:08' / End date of observations
TSTART = 2.162126183025770E+08 / time start
TSTOP = 2.162791240000000E+08 / time stop
TELAPSE = 6.650569742301106E+04 / elapsed time
ONTIME = 3.045204986763000E+04 / On-source time
EXPOSURE= 3.045204986763000E+04 / Exposure time
MJD-OBS = 5.404646160285390E+04 / MJD of data start time
FILIN001= 'ae501091010xi0_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= 'ae501091010xi0_0_5x5n000a_cl.evt.gz' / Input file name
FILIN003= 'ae501091010xi1_0_3x3n001b_cl.evt.gz' / Input file name
FILIN004= 'ae501091010xi1_0_5x5n001b_cl.evt.gz' / Input file name
FILIN005= 'ae501091010xi2_0_3x3n000a_cl.evt.gz' / Input file name
FILIN006= 'ae501091010xi2_0_5x5n000a_cl.evt.gz' / Input file name
FILIN007= 'ae501091010xi3_0_3x3n000a_cl.evt.gz' / Input file name
FILIN008= 'ae501091010xi3_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:
Clusters of massive stars, through their stellar winds and supernovae, form large diffuse structures known as superbubbles (SBs), which play an essential role in shaping the local interstellar medium. Most SB models indicate that these objects should be dominated by thermal plasma processes. However, observations of 2 SBs have detected significant nonthermal contributions to their X-ray emission, which raises many questions. Is it generated by synchrotron, inverse-Compton, or nonthermal Bremsstrahlung processes? Are colliding stellar winds or internal supernova remnants responsible? We therefore propose to examine the X-ray emission from 4 X-ray bright SBs, to search for nonthermal X-ray emission, and if possible place strong constraints on the source of this emission.