Keck spectroscopy ofz= 1–3 ULIRGs from the Spitzer SWIRE survey

2007/03/09 by S. Berta, Carol J. Lonsdale, C. J. Lonsdale +13 · 3 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066795

published as Astron.Astrophys.467:565-584,2007 · Accepted for publications on Astronomy and Astrophysics (acceprance date March 8th, 2007). 33 pages. The quality of some figures have been degraded

arxiv created 2007/03/09 · openalex publication_date 2007/03/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context. High-redshift ultra luminous infrared galaxies contribute the bulk of the cosmic IR background and are the best candidates for very massive galaxies in formation at .

Citations

• Classification parameters for the emission-line spectra of extragalactic objects
• SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey
• Star Formation in Galaxies Along the Hubble Sequence

Cited by

• The ESO-Spitzer Imaging extragalactic Survey (ESIS)
• Photometric redshifts in the SWIRE Survey
• Mid-infrared spectroscopy of infrared-luminous galaxies atz∼ 0.5-3