Suzaku Observation : 407094010
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Fits Header
TELESCOP= 'SUZAKU ' / Telescope (mission) name
OBS_ID = '407094010' / Observation identification string
OBSERVER= 'MARTINO MARELLI' / Principal Investigator
OBJECT = 'J1522-5734' / Name of observed object
OBS_REM = ' ' / remark on observation
RA_OBJ = 230.5223 / planned target R.A.(deg)
DEC_OBJ = -57.5831 / planned target DEC.(deg)
RA_NOM = 2.305286000000000E+02 / Right Ascension of target (deci. deg)
DEC_NOM = -5.758160000000000E+01 / Declination of target (deci. deg)
PA_NOM = 274.4971 / nominal position angle from north to DETY(deg)
MEAN_EA1= 230.528647113269 / mean of the 1st ZYZ-Euler angle (deg)
MEAN_EA2= 147.581628828566 / mean of the 2nd ZYZ-Euler angle (deg)
MEAN_EA3= 175.502926790351 / mean of the 3rd ZYZ-Euler angle (deg)
DATE-OBS= '2012-08-15T15:34:02' / Start date of observations
DATE-END= '2012-08-16T00:11:17' / End date of observations
TSTART = 3.983610160000000E+08 / time start
TSTOP = 3.983910614699782E+08 / time stop
TELAPSE = 3.004546997821331E+04 / elapsed time
ONTIME = 3.004546997821331E+04 / On-source time
EXPOSURE= 3.004546997821331E+04 / Exposure time
MJD-OBS = 5.615466065027777E+04 / MJD of data start time
FILIN001= 'ae407094010xi0_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= 'ae407094010xi1_0_3x3n130b_cl.evt.gz' / Input file name
FILIN003= 'ae407094010xi3_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 Large Area Telescope (LAT) on-board the Fermi mission is opening a new window on pulsar astrophysics, by unveiling more than 100 new gamma-ray pulsars, a third of which lacks detection at radio wavelengths despite very deep searches. For these pulsars, X-rays provide a powerful avenue for further high-energy studies. Here we propose 25ks Suzaku observations of the 9 radio-quiet gamma-ray pulsars which have no X-ray counterparts nor deep X-ray observations, in order to better understand this population's X-ray properties and to extract constraints on the crucial unknown distances.