XMM-Newton Proposal 02044008

Details XMM-Newton Proposal 02044008 XMM-Newton Proposal 02044008

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..234a&link_type=abstract

XMM-Newton Proposal ID #02044008

Computer Science

6C1232+39, 4C23.56, 8C1435+635, Tx1243+036, 3C239, 4C60.07, 4C28.58, Mg2141+192, Xmm-Newton Proposal 02044008

Scientific paper

We have completed a sub-mm survey of powerful high redshift radio galaxies. This revealed strong evolution in the mean sub-mm luminosity with redshift, with a particularly wide variance in sub-mm properties beyond z3. This range of evolutionary states may reflect the formation epoch of the host spheroids. Here we seek XMM-Newton observations of a carefully chosen sample to investigate whether the most luminous sub-mm sources contain the most heavily absorbed AGN. This will test the popular evolutionary models for the early stages of massive galaxy formation (Silk & Rees 1998, Fabian 1999), which predict a transition from sub-mm source (with a hidden AGN) to a visible quasar. A secondary goal is to search for hot gas associated with early proto-cluster environments.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 02044008 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with XMM-Newton Proposal 02044008, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 02044008 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1172836