XMM-Newton Proposal 02026219

Details XMM-Newton Proposal 02026219 XMM-Newton Proposal 02026219

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..137n&link_type=abstract

XMM-Newton Proposal ID #02026219

Physics

3C 279, 1H 0323+022, 1H 0414+009, 1Es 0647+250, Pks 0829+046, Pks 0558-504, H 2356-309, 1Es 1426+428, 1Es 1028+511, 3C 279, 1H 0323+022, 1H 0414+009, 1Es 0647+250, Pks 0829+046, Pks 0558-504, H 2356-309, 1Es 1426+428, 1Es 1028+511, Xmm-Newton Proposal 02026219

Scientific paper

We propose to extend our XMM-Newton-AO2 TOO program to the 3rd XMM-Newton cycle, to observe a moderate redshift blazar (z > 0.1) in an exceptionally high state with the XMM-Newton RGS for an exposure time of 200 ks. We shall study the ``warm'', low-redshift, phase of the intergalactic medium, where most of the baryonic matter of the local (z < 1-2) Universe is believed to hide.

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