Extragalactic abstracts - IRSA - California Institute of Technology

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Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 243/742 Spitzer Space Telescope − Legacy General Observer Proposal #40021 A Spitzer Public Legacy survey of the UKIDSS Ultra Deep Survey Principal Investigator: James Dunlop Institution: Institute for Astronomy, Royal Obs. Edinburgh Technical Contact: Duncan Farrah, Cornell University Co−Investigators: Duncan Farrah, Cornell University Masami Ouchi, Space Telescope Science Institute Ross McLure, Institute for Astronomy, Royal Obs. Edinburgh Eiichi Egami, University of Arizona Angela Mortier, Institute for Astronomy, Royal Obs. Edinburgh Harry Ferguson, Space Telescope Science Institute George Rieke, University of Arizona Omar Almaini, University of Nottingham Chris Simpson, Liverpool John Moores University Andy Lawrence, Institute for Astronomy, Royal Obs. Edinburgh Rob Ivison, Royal Observatory Edinburgh Eduardo Ibar, Institute for Astronomy, Royal Obs. Edinburgh Michael Fall, Space Telescope Science Institute Andrea Cimatti, Osservatorio Astrofisico di Arcetri Malcolm Bremer, University of Bristol Stephen Serjeant, Open University Masayuki Akiyama, National Astronomical Obs of Japan (NAOJ), Subaru Hisanori Furusawa, National Astronomical Observatory of Japan (NAOJ) Kazuhiro Sekiguchi, National Astronomical Obs of Japan (NAOJ), Subaru Ian Smail, University of Durham Michele Cirasuolo, Institute for Astronomy, Royal Obs. Edinburgh Mike Watson, University of Leicester Alexis Finoguenov, University of Maryland Baltimore County Christopher Conselice, University of Nottingham David Alexander, University of Durham Gavin Dalton, University of Oxford Matt Jarvis, University of Oxford Sebastien Foucaud, University of Nottingham Steve Eales, University of Wales, College of Cardiff (UWCC) Simon Dye, University of Wales, College of Cardiff (UWCC) Steve Rawlings, University of Oxford Seb Oliver, University of Sussex Mathew Page, Mullard Space Science Laboratory Steve Maddox, University of Nottingham Toru Yamada, National Astronomical Observatory of Japan (NAOJ) Loretta Dunne, University of Nottingham Kristen Coppin, University of Durham Alastair Edge, University of Durham Colin Borys, University of Toronto Lee Clewley, University of Oxford Elizabeth Stanway, University of Bristol Caroline van Breukelen, University of Oxford Andy Taylor, Institute for Astronomy, Royal Obs. Edinburgh Marijn Franx, Leiden University Rik Williams, Leiden University Maaike Damen, Leiden University Pieter van Dokkum, Yale University Ivo Labbe, Carnegie Observatories, Pasadena Jiasheng Huang, CfA, Harvard University Rychard Bouwens, UC Santa Cruz Garth Illingworth, UC Santa Cruz Ryan Quadri, Yale University Casey Papovich, University of Arizona David Schiminovich, Columbia University Science Category: high−z galaxies (z>0.5) Observing Modes: IracMap MipsScan Hours Approved: 292.0 Mar 25, 10 16:24 Spitzer_Approved_Extragalactic Printed_by_SSC Page 244/742 Abstract: We propose a public legacy program of Spitzer IRAC+MIPS imaging of the ~1 square degree UKIDSS Ultra Deep Survey (UDS). The UDS is by far the largest, deep near−infrared (JHK) survey in existence, and the first capable of sampling truly representative cosmological volumes (100x100 Mpc) out to the highest redshifts (z>6). The UDS is an uniquely powerful resource for studying galaxy formation and evolution and already contains ~100,000 galaxies (>20,000 at z>2). However, the key to unlocking the full potential of the UDS lies in combining the ground− based near−infrared data with appropriately deep Spitzer imaging. The proposed Spitzer data will be invaluable for providing robust measurements of both stellar mass and starformation rates, and will allow the first statistical study of the evolution of the high−mass end of the galaxy mass function out to z=6. Moreover, the proposed Spitzer imaging will allow the evolution of starforming and passive galaxies to be studied separately, and help delineate the link between stellar mass assembly and starformation at high redshift. The UDS will continue to provide ever−increasing depth for the next 5 years, and will be the deepest, contiguous degree−scale infrared survey for the foreseeable future. This proposal is ideally timed to allow immediate and full exploitation of the first world−public UDS release in January 2008, but will also provide a uniquely powerful data−set of lasting legacy value for future exploitation with JWST and ALMA in the next decade. Thursday March 25, 2010 xgal_covers.txt 122/371
Spitzer_Approved_Extragalactic Mar 25, 10 16:24 Page 245/742 Spitzer Space Telescope − General Observer Proposal #41011 MIPS 24 um Snapshot Survey of Massive Galaxy Clusters Principal Investigator: Eiichi Egami Institution: University of Arizona Technical Contact: Eiichi Egami, University of Arizona Co−Investigators: Graham Smith, University of Birmingham Jean−Paul Kneib, OAMP, Marseille Daniel Schaerer, Geneva Observatory Roser Pello, Obs−MIP, France Johan Richard, Caltech Dario Fadda, IPAC/Caltech Frederic Boone, Obs−PM, France Science Category: high−z galaxies (z>0.5) Observing Modes: MipsPhot Hours Approved: 22.3 Abstract: Gravitatinoal lensing by massive clusters of galaxies offers a very powerful and yet cheap means to improve the sensitivity of a given telescope/instrument combination. The use of gravitational lensing is especially powerful in the infrared wavelengths because cluster cores are dominated by early−type galaxies, which usually emit very little in the infrared. Therefore, infrared sources detected in cluster cores are almost always background sources. Here, we propose to conduct a MIPS 24 $\\mu$m snapshot survey of massive galaxy clusters with the goal of more of such stongly−lensed high−redshift galaxies. We will also study infrared−luminous brightest cluster galaxies (BCGs). This survey should be able to supply many interesting targets to follow up with SCUBA2, Herschel, and ALMA. Spitzer_Approved_Extragalactic Printed_by_SSC Mar 25, 10 16:24 Page 246/742 Spitzer Space Telescope − Directors Discretionary Time Proposal #280 IRS Spectroscopy of a Typical Lyman Break Galaxy Principal Investigator: Richard Ellis Institution: Caltech Technical Contact: Brian Siana, Spitzer Science Center Co−Investigators: Johan Richard, Caltech Harry Teplitz, Caltech Ian Smail, Durham Jean−Paul Kneib, Caltech Mark Swinbank, Durham Alastair Edge, Durham Harald Ebeling, Institute for Astronomy Max Pettini, Cambridge Science Category: High−z Galaxies (z>0.5) Observing Modes: IracMap MipsPhot Hours Approved: 0.9 Abstract: We request Director’s discretionary time on the Spitzer Space Telescope (SST) to determine the restframe mid−infrared spectral properties of a typical L* Lyman break galaxy (LBG) at z=3.07. Our proposed SST study of this galaxy requests a total of 11 hrs integration: 2 hrs with IRAC and MIPS at 24/70 microns to obtain photometry of the source at restframe wavelengths of 0.8−17 microns and 9 hrs exposure with IRS in LL1/SL1 to probe the 3−8 micron PAH and the shape of the continuum emission. This study is only feasible because of a 30x boost to the light−gathering power of Spitzer provided by a foreground gravitational lens − allowing us to use these observations to address questions which are drivers of the James Webb Space Telescope (JWST) science case: yielding insights into the star formation properties of a normal, young galaxy seen 12 Gyrs ago. Thursday March 25, 2010 xgal_covers.txt 123/371
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