XMM-Newton Proposal 03028810

Details XMM-Newton Proposal 03028810 XMM-Newton Proposal 03028810

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..107w&link_type=abstract

XMM-Newton Proposal ID #03028810

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White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Gc-1, Gc-2, Gc-3, Gc-7, Gc-8, Gc-9, Gc-10, Xmm-Newton Proposal 03028810

Scientific paper

We propose a monitoring campaign using XMM-Newton and Chandra of a 2 by 1 degree region centered on the Galactic Center. We will be able to detect transients which occur near the Galactic Center with a peak luminosity of 1E33-1E35 ergs/s, 10 to 1000 times more sensitive than what is possible with other satellites (i.e., RXTE and INTEGRAL). This allows us to observe a very poorly studied group of X-ray transients and to follow the luminosity behavior of weak (less than 1E36 ergs/s) persistent sources.

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