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MIPS Class Coaddition of SWIRE High-Redshift Galaxies

Shupe, David L. and Lonsdale, Carol J. and Polletta, Mari and Lagache, Guilaine (2008) MIPS Class Coaddition of SWIRE High-Redshift Galaxies. In: The 2nd Spitzer Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series. No.381. Astronomical Society of the Pacific , pp. 235-238. ISBN 978-1-58381-325-6. https://resolver.caltech.edu/CaltechAUTHORS:20100802-104613039

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Abstract

The SWIRE survey encompasses the largest volume of the Spitzer extragalactic surveys, providing the best sensitivity for the detection of significant numbers of rare objects, including the most massive ULIRGs, and obscured AGN. These objects are detected and classified using Spitzer IRAC and MIPS-24 data, but are too faint to be detected individually in the 70 μm and 160 μm bands. We have applied a class coaddition technique to investigate far-infrared spectral energy distributions of these sources by redshift and spectral shape. The variation of far-IR-to-mid-IR colors of the ULIRGs with redshift generally tracks the predictions of template galaxies, and favors the lower-luminosity templates.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://www.aspbooks.org/a/volumes/article_details/?paper_id=28097PublisherArticle
ORCID:
AuthorORCID
Shupe, David L.0000-0003-4401-0430
Lonsdale, Carol J.0000-0003-0898-406X
Polletta, Mari0000-0001-7411-5386
Lagache, Guilaine0000-0003-1492-2519
Additional Information:© Astronomical Society of the Pacific. We are grateful to Hervé Dole for advice on estimating uncertainties using bootstrap resampling.
Group:Infrared Processing and Analysis Center (IPAC)
Series Name:ASP Conference Series
Issue or Number:381
Record Number:CaltechAUTHORS:20100802-104613039
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100802-104613039
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:19243
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:17 Aug 2010 21:41
Last Modified:09 Mar 2020 13:19

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