XMM-Newton Proposal 02018304

Details XMM-Newton Proposal 02018304 XMM-Newton Proposal 02018304

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...98m&link_type=abstract

XMM-Newton Proposal ID #02018304

Physics

Ngc 5506, Ngc 5506, Ngc 5506, Ngc 5506, Xmm-Newton Proposal 02018304

Scientific paper

We propose repeated observations with XMM-Newton of the bright Seyfert galaxy NGC 5506 which exhibits a complex Fe line emission profile, with at least two components, as revealed by previous XMM-Newton AO-1 observations. The source is also known to be highly variable on timescales of few days from extensive RXTE monitoring. The main goal of the proposed observations is to assess the location and physical state of the emitting media by measuring their profiles and EWs in different intensity states of the continuum. Our strategy will be to perform 4 logarithmically spaced observations, sampling time scales from a few days to a month.

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