Extragalactic abstracts - IRSA - California Institute of Technology

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Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 503/742 Spitzer Space Telescope − General Observer Proposal #3726 The symbiosis of AGN activity and galaxy formation Principal Investigator: Jonathan Mittaz Institution: University of Alabama at Huntsville Technical Contact: Jonathan Mittaz, University of Alabama at Huntsville Co−Investigators: Mathew Page, MSSL, University College London Jason Stevens, Astronomy Technology Centre, ROE Francisco Carrera, IFCA, University of Cantabria, Spain Rob Ivison, Astronomy Technology Centre, ROE Ian Smail, Institute for Computational Cosmology, University Science Category: AGN/quasars/radio galaxies Observing Modes: IracMap MipsPhot Hours Approved: 6.0 Abstract: According to galaxy formation models, cluster ellipticals formed in high density regions through hierarchical merging of gas rich sub−components. In local ellipticals, the strong correlation observed between black hole and bulge mass implies that galaxy formation is inextricably linked to the build up of supermassive black holes. We have found 6 high redshift, X−ray luminous, but heavily absorbed AGN, embedded in strong bursts of star formation revealed in the submillimetre. Our SCUBA survey shows that the immediate vicinities of these objects contain large overdensities of ultraluminous star−forming galaxies which will evolve to form clusters. Here we propose to use SPITZER to measure the stellar masses of the companion galaxies, search for buried AGN, and thereby determine the sequence in which the cluster ellipticals are assembled, form their stars, and grow their massive black holes. Spitzer_Approved_Extragalactic Printed_by_SSC Mar 25, 10 16:24 Page 504/742 Spitzer Space Telescope − General Observer Proposal #41023 The Evolution of Faint AGN at High Redshift Principal Investigator: Kirpal Nandra Institution: Imperial College London Technical Contact: Kirpal Nandra, Imperial College London Co−Investigators: James Aird, Imperial College London Pauline Barmby, SAO Mark Davis, UC Berkeley Mark Dickinson, NOAO Sandra Faber, UC Santa Cruz Giovanni Fazio, Harvard University Antonis Georgakakis, Imperial College London Puragra Guhathakurta, UC Santa Cruz Jiasheng Huang, SAO Rob Ivison, University of Edinburgh David Koo, UC Santa Cruz Shinae Park, SAO Ranga Ram−Chary, Caltech David Frayer, IPAC/Caltech Science Category: AGN/Quasars/Radio Galaxies Observing Modes: IracMap Hours Approved: 46.0 Abstract: We propose a very deep (total 800ks/field) Chandra survey of 0.25 deg2 covering 3 contiguous fields in the Extended Groth Strip, which have exceptional multiwaveband coverage obtained by the AEGIS project. These data, in combination with the CDF North and South, will provide a definitive measurement of the evolution of faint, X−ray selected AGN from z=3−4, where the optical number counts start to drop dramatically. In combination with ultradeep Spitzer data in the same region, this survey will also provide a crucial step forward towards a more complete census of AGN activity and the importance of Compton thick AGN at high z, with associated implications for the total accretion budget of the universe. Thursday March 25, 2010 xgal_covers.txt 252/371
Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 505/742 Spitzer Space Telescope − General Observer Proposal #20142 Spectroscopy of the Dusty Torus in PG Quasars Principal Investigator: Patrick Ogle Institution: Caltech Technical Contact: Patrick Ogle, Caltech Co−Investigators: Robert Antonucci, University of California, Santa Barbara David Whysong, University of California, Santa Barbara Science Category: AGN/quasars/radio galaxies Observing Modes: IrsStare Hours Approved: 30.5 Abstract: We propose IRS SL+LL spectroscopic observations of the dusty tori in the complete sample of UV−color selected PG quasars with redshift z
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