XMM-Newton observation of the bright atoll 4U 1735-444

Details XMM-Newton observation of the bright atoll 4U 1735-444 XMM-Newton observation of the bright atoll 4U 1735-444

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..167d&link_type=abstract

XMM-Newton Proposal ID #05556201

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, 4U 1735-44, Xmm-Newton Proposal Id #05556201

Scientific paper

We propose to observe the LMXB bursting source 4U 1755-44 with XMM-Newton for 40 ks. Our main scientific goal is to perform high resolution spectroscopic analysis in the broad RGS/EPIC X-ray range combined with the timing analysis. The source is enough bright and not so much absorbed, to allow a detailed analysis of the X-ray spectrum in the whole 0.3-15 keV range, still avoiding spectral distortions due to pile-up. We request the observation to be performed in the Modified Timing Mode configuration; this will allow a more efficient use of the instruments, eliminting data loss due to telemetry overflow and maximizing the S/N ratio in the Fe K region.

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