Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733608k&link_type=abstract
American Astronomical Society, AAS Meeting #217, #336.08; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
Motivated by a search to identify the x-ray counterpart of GeV emissions from pulsars detected by Femi-LAT, we have analyzed over forty pulsar observations from various x-ray missions. Among these missions are BeppoSax, SWIFT, and Chandra. Through our analysis we have been able to identify the X-ray counterpart, estimate the X-ray flux, and calculate the x-ray photon index for much of our sample. We have investigated the correlations between observed properties such as fluxes and photon indices in X-ray and GeV, as well as pulsar parameters such as the magnetic field strength, the rate of rotational energy loss and the spin down age for all of our sample in order to characterize each pulsar further.
Knoche Richard Aaron
Sakamoto Taka
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