Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources

Details Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop..158r&link_type=abstract

XMM-Newton Proposal ID #06057002

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Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Gev J1907+0557

Scientific paper

There are several likely gamma-ray pulsars in EGRET error boxes which are probably associated with known TeV sources, but radio searches have failed to detect pulsations from them. Direct searches for gamma-ray pulsations of the brightest EGRET sources using Fermi are proving quite successful. However, to understand the emission mechanisms, pulsations at other wavelengths are critical. Here we propose XMM-Newton studies of two such sources: GeV J1825-1310 (the Eel) and GeV J1907+0557, with the primary goal of detecting X-ray pulsations using the PN in small window mode. Both have extended X-ray nebula whose spatial and spectral properties will be studied using the MOS imagers.

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