The nature of the high flux sources seen by the BeppoSAX WFC

Details The nature of the high flux sources seen by the BeppoSAX WFC The nature of the high flux sources seen by the BeppoSAX WFC

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..102c&link_type=abstract

XMM-Newton Proposal ID #05026706

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, 1Rxsj063656.7-0, Pks 0706-15, 1Rxsj081232.3-5, 1Rxsj153934.7-8, 1Rxsj160107.6-7, 1Rxsj202151.7+3, Xmm-Newton Proposal 05026706

Scientific paper

The combination of all data of the BeppoSAX Wide Filed Cameras has revealed the detection of a number of active galactic nuclei and galaxy clusters. Six bright sources, which are confirmations of ROSAT detections, are yet without a determined nature. We propose to carry out short exploratory observations with XMM-Newton of these objects, in order to determine their spectrum and short-term variability and identify possibly interesting features for follow up in future XMM-Newton or Chandra AOs.

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