Extragalactic abstracts - IRSA - California Institute of Technology

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Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 239/742 Spitzer Space Telescope − Directors Discretionary Time Proposal #196 Great Observatories Origins Deep Survey (GOODS) Validation Observations Principal Investigator: Mark Dickinson Institution: NOAO Technical Contact: Peter Eisenhardt, JPL Co−Investigators: The GOODS Team , Science Category: high−z galaxies (z>0.5) Observing Modes: IracMap MipsPhot Hours Approved: 10.0 Abstract: Validation observations of the Great Observatories Origins Deep Survey (GOODS). Spitzer_Approved_Extragalactic Printed_by_SSC Mar 25, 10 16:24 Page 240/742 Spitzer Space Telescope − Legacy General Observer Proposal #30948 A Deep−Wide Far−Infrared Survey of Cosmological Star Formation and AGN Activity Principal Investigator: Mark Dickinson Institution: NOAO Technical Contact: David Frayer, SSC/Caltech Co−Investigators: David Frayer, Spitzer Science Center David Alexander, Cambridge University Eric Bell, Max−Planck−Institute for Astronomy, Heidelberg Niel Brandt, Penn State University Daniela Calzetti, Space Telescope Science Institute Scott Chapman, California Institute of Technology Stefano Casertano, Space Telescope Science Institute Ranga−Ram Chary, Spitzer Science Center Emanuele Daddi, National Optical Astronomy Observatory Mark Davis, University of California, Berkeley Hervé Dole, Institut d’Astrophysique Spatiale, Université Pari James Dunlop, University of Edinburgh Peter Eisenhardt, Jet Propulsion Laboratory David Elbaz, CEA Saclay Sandra Faber, University of California Santa Cruz Giovanni Fazio, Smithsonian Astrophysical Observatory Henry Ferguson, Space Telescope Science Institute Mauro Giavalisco, Space Telescope Science Institute Mark Halpern, University of British Columbia Jiasheng Huang, Smithsonian Astrophysical Observatory Minh Huynh, Spitzer Science Center Rob Ivison, Royal Observatory Edinburgh Anton Koekemoer, Space Telescope Science Institute Emeric Le Floc’h, University of Arizona Glenn Morrison, Canada France Hawaii Telescope Leonidas Moustakas, Jet Propulsion Laboratory Casey Papovich, University of Arizona Alexandra Pope, University of British Columbia Alvio Renzini, Padova University George Rieke, University of Arizona Hans−Walter Rix, Max−Planck−Institute for Astronomy, Heidelberg Douglas Scott, University of British Columbia Ian Smail, Durham University Haojing Yan, Spitzer Science Center Pieter van Dokkum, Yale University Paul van der Werf, Leiden Observatory Science Category: high−z galaxies (z>0.5) Observing Modes: MipsPhot MipsScan Hours Approved: 397.0 Abstract: Spitzer is creating a vast legacy of 24 micron imaging, with hundreds of thousands of sources detected at cosmological distances. In principle, 24 micron data are the most sensitive probe of dust−enshrouded star formation and distant active galactic nuclei. In practice, at z > 1, they sample mid−infrared wavelengths complex in structure (PAH emission and silicate absorption) and physics (PAH excitation, metallicity dependence, extinction, warm dust and hidden AGN). Other data are needed to understand MIR emission, to calibrate its relation to star formation, to establish its dependence on other galaxy properties, to measure how many atypical objects there are, and to learn how to account for them in conclusions drawn from deep surveys. We propose a program of very deep MIPS imaging geared toward 70 micron detection of 1000 "normal" IR−luminous galaxies at 0.5 < z < 2.5 at wavelengths which trace thermal dust emission which more directly correlates with physical properties of interest such as star formation rates. We will survey 2200 square arcmin in three premier deep survey fields using far−infrared, radio and submillimeter data to measure bolometric luminosities, dust temperatures and masses, to quantify the Thursday March 25, 2010 xgal_covers.txt 120/371
Mar 25, 10 16:24 Spitzer_Approved_Extragalactic Page 241/742 population of Compton−obscured AGN, and to calibrate the use of 24 micron data for studying high redshift galaxy evolution. Spitzer_Approved_Extragalactic Printed_by_SSC Mar 25, 10 16:24 Page 242/742 Spitzer Space Telescope − General Observer Proposal #30823 Pushing the Far−IR Capability of Spitzer in the Study of High−Redshift ULIRGs Principal Investigator: Charles Dowell Institution: Jet Propulsion Laboratory Technical Contact: Charles Dowell, Jet Propulsion Laboratory Co−Investigators: Colin Borys, University of Toronto (Canada) Eiichi Egami, University of Arizona Michael Zemcov, Cardiff University (UK) Science Category: high−z galaxies (z>0.5) Observing Modes: MipsPhot Hours Approved: 60.4 Abstract: We propose deep MIPS 70 and 160 micron observations of a sample of submillimeter−selected high−redshift ultraluminous infrared galaxies (ULIRGs). For the first time, we will explore the diversity of their far−infrared spectral distributions −− in particular, on the Wien side of the graybody peak −− and measure accurately the integrated infrared luminosity. The targets are drawn from a sample of 850 micron sources at z > 1 amplified by foreground galaxy clusters, where the lensing allows us to measure galaxies which would otherwise be too faint for detection and may also lower the confusion noise. Our program is complemented by ground−based 350 micron imaging, which quantifies the graybody spectrum. Thursday March 25, 2010 xgal_covers.txt 121/371
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