Completing the X-ray survey of HESS~J1614-518

Details Completing the X-ray survey of HESS~J1614-518 Completing the X-ray survey of HESS~J1614-518

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..170h&link_type=abstract

XMM-Newton Proposal ID #05556601

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Hess J1614-518S, Xmm-Newton Proposal Id #05556601

Scientific paper

We propose to observe for the first time the south-eastern part of the unidentified very high energy E>100 GeV gamma-ray source HESS J1614-518. In a recent XMM-Newton observation (36 ksec) of the north-eastern part of this source, extended (FWHM 8'),non-thermal X-ray emission has been detected with an energy flux $f(2-10) 1.5x10^{-12}cgs. The morphology of the X-ray emitting region is similar to the morphology of HESS J1614-518.With the proposed observation of 40 ksec of the south-eastern part of HESS J1614-518 which has so far not beeen covered by X-ray observations, we want to search for X-ray emission from this region of HESS J1614-518 which would clearly establish the close connection between X-ray and VHE emission.

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