Suzaku Observation : 507041010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '507041010' / Observation identification string
OBSERVER= 'TSUNEFUMI MIZUNO' / Principal Investigator
OBJECT = 'CYG_BGD1' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 306.6375 / planned target R.A.(deg)
DEC_OBJ = 39.4925 / planned target DEC.(deg)
RA_NOM = 3.066527000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = 3.948560000000000E+01 / Declination of target (deci. deg)
PA_NOM = 218.9004 / nominal position angle from north to DETY(deg)
MEAN_EA1= 306.652738918199 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 50.514354075406 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 231.099637580346 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-12-19T04:00:00' / Start date of observations
DATE-END= '2012-12-19T15:05:15' / End date of observations
TSTART = 4.092048136402285E+08 / time start
TSTOP = 4.092446992555858E+08 / time stop
TELAPSE = 3.988561535733938E+04 / elapsed time
ONTIME = 2.694835923892260E+04 / On-source time
EXPOSURE= 2.694835923892260E+04 / Exposure time
MJD-OBS = 5.628016756741005E+04 / MJD of data start time
FILIN001= 'ae507041010xi0_0_3x3n066l_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= 'ae507041010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae507041010xi3_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:
The long-standing questions on the origin of Galactic cosmic-rays (GCR) is still not settled, and star-forming regions are promising sites for the production of GCR. We propose deep observation of nearby star-forming region Cygnus X, aiming at GeV gamma-ray excess revealed by Fermi. By utilizing the high sensitivity of Suzaku XIS, particularly for diffuse X-rays, we can identify particle species (electrons or protons) and evaluate the cosmic-ray energy density in this important object.