X-ray follow-up observations of known transient INTEGRAL sources

Details X-ray follow-up observations of known transient INTEGRAL sources X-ray follow-up observations of known transient INTEGRAL sources

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..193s&link_type=abstract

XMM-Newton Proposal ID #04051818

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Igr J11215-5952, Igr J11305-6256, Igr J11321-5311, Igr J16316-4028, Igr J16418-4532, Igr J17091-3624, Igr J17098-3628, Igr J17269-4737, Igr J17285-2922, Igr J17407-2808, Igr J16493-4348, Igr J18325-0756, Igr J18406-0539, Igr J18539+0727, Igr J05009-7044, Igr J05319-6601, Igr J05346-5759, Igr J06239-6052, Xmm-Newton Proposal 04051818

Scientific paper

We propose to trigger a maximum of 5 XMM follow-up observations on known transient sources discovered with INTEGRAL Observatory,if they undergo a new outburst during AO5. We ask for 20 ks per observation,usign EPIC PN as primary instrument, in order to get a high-quality X-ray spectrum.XMM spectral and spatial capabilities are essential in unveiling their nature (still unknown for the select targets), and in refining their sky positions, enabling multiwavelength follow-up observations.

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