Extragalactic abstracts - IRSA - California Institute of Technology
Extragalactic abstracts - IRSA - California Institute of Technology
Extragalactic abstracts - IRSA - California Institute of Technology
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Spitzer_Approved_<strong>Extragalactic</strong><br />
Mar 25, 10 16:24 Page 671/742<br />
Spitzer Space Telescope − General Observer Proposal #3672<br />
Spitzer Observations <strong>of</strong> a Complete Sample <strong>of</strong> Luminous Infrared Galaxies in the<br />
Local Universe<br />
Principal Investigator: Joseph Mazzarella<br />
Institution: <strong>California</strong> Instiute <strong>of</strong> <strong>Technology</strong><br />
Technical Contact: Joseph Mazzarella, <strong>California</strong> Instiute <strong>of</strong> <strong>Technology</strong><br />
Co−Investigators:<br />
Phil Appleton, Caltech , IPAC/SSC<br />
Lee Armus, Caltech, IPAC/SSC<br />
Aaron Evans, SUNY, Stony Brook<br />
David Frayer, Caltech, IPAC/SSC<br />
Catherine Ishida, Subaru<br />
Joseph Jensen, Gemini<br />
Sophia Khan, GSFC<br />
Dong−Chan Kim, University <strong>of</strong> Maryland<br />
Steven Lord, Caltech, IPAC/NHSC<br />
Barry Madore, OCIW & Caltech<br />
David Sanders, IfA, University <strong>of</strong> Hawaii<br />
Bernhard Schulz, IPAC, NHSC<br />
Jason Surace, Caltech, IPAC/SSC<br />
Sylvain Veilleux, University <strong>of</strong> Maryland<br />
Kevin Xu, Caltech, IPAC/GALAX<br />
Science Category: ULIRGS/LIRGS/HLIRGS<br />
Observing Modes: IracMap MipsPhot<br />
Hours Approved: 90.1<br />
Abstract:<br />
We propose Spitzer Space Telescope observations <strong>of</strong> all ~200 luminous infrared<br />
galaxies (LIRGs, L_ir > 10^{11} L_sun) and ultraluminous infrared galaxies<br />
(ULIRGs, L_ir > 10^{12} L_sun) in the IRAS Revised Bright Galaxy Sample, a<br />
complete flux−limited survey <strong>of</strong> all extragalactic objects with total 60um flux<br />
density greater than 5.24 Jy, covering the entire sky surveyed by IRAS at<br />
Galactic latitudes abs(b) > 5 degrees. The superb sensitivity <strong>of</strong> Spitzer<br />
provides a unique opportunity to survey the physical properties <strong>of</strong> star<br />
formation and the interstellar medium in a large, statistically complete,<br />
flux−limited sample <strong>of</strong> nearby LIRGs and ULIRGs. IRAC and MIPS will be used to<br />
image the infrared emission in individual galaxies within interacting/merging<br />
systems that were not resolved by IRAS or ISO. Problems to be addressed include:<br />
1) How do star formation rates and the spatial distribution <strong>of</strong> dust emitting<br />
regions vary with the stage <strong>of</strong> the interaction/merger, the mass ratio <strong>of</strong> the<br />
galaxies, the geometry <strong>of</strong> the encounter, and the properties <strong>of</strong> each galaxy known<br />
from optical, near−infrared, H I, CO, and radio continuum observations? 2) Which<br />
LIRGs most likely represent progenitors <strong>of</strong> ULIRGs and QSOs, and what<br />
characteristics <strong>of</strong> the galaxies and their merger geometries likely lead to dust<br />
heating dominated by AGNs rather than starbursts? 3) What are the relative<br />
amounts <strong>of</strong> cold (10 − 30 K), cool (30−50 K) and warm (T_d > 50 K) dust<br />
components in LIRGs and ULIRGs, and can this be used to age−date merger events?<br />
4) Are there regions with very hot dust (600 − 1000 K) in some <strong>of</strong> these objects?<br />
This survey will also provide an important archive <strong>of</strong> data for establishing<br />
links between the global infrared properties <strong>of</strong> high redshift infrared/sub−mm<br />
galaxies and structural details that can be well resolved only in local LIRGs.<br />
Spitzer_Approved_<strong>Extragalactic</strong><br />
Printed_by_SSC<br />
Mar 25, 10 16:24 Page 672/742<br />
Spitzer Space Telescope − General Observer Proposal #40682<br />
IRS Observation <strong>of</strong> Four Exceptionally Red 24 micron Sources<br />
Principal Investigator: Sebastian Oliver<br />
Institution: University <strong>of</strong> Sussex<br />
Technical Contact: Sebastian Oliver, University <strong>of</strong> Sussex<br />
Co−Investigators:<br />
Matthew Thomson, University <strong>of</strong> Sussex<br />
Duncan Farrah, Cornell<br />
Carol Lonsdale, University <strong>of</strong> <strong>California</strong>, San Diego<br />
Mari Polletta, University <strong>of</strong> <strong>California</strong>, San Diego<br />
David Shupe, IPAC<br />
Jason Surace, IPAC<br />
Science Category: ULIRGS/LIRGS/HLIRGS<br />
Observing Modes: IrsMap<br />
Hours Approved: 10.1<br />
Abstract:<br />
Four strong candidates for some <strong>of</strong> the most extreme objects observable with IRS<br />
have been identified using a technique for source extraction based on using the<br />
data from SWIRE 24 micron images taken at two epochs. These are highly reliable<br />
sources but which have no detection at IRAC wavebands. This suggests that they<br />
are the most extremely red sources. Our proposal is for an IRS observation <strong>of</strong><br />
these four objects in order to apply various SED models to attempt to find the<br />
nature <strong>of</strong> these objects.<br />
Thursday March 25, 2010 xgal_covers.txt<br />
336/371