Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'501'711
Articles rated: 2609

20 April 2024
 
  » arxiv » astro-ph/0412574

 Article overview


The Rest-Frame Optical Properties of SCUBA Galaxies
Ian Smail ; S.C. Chapman ; A.W. Blain ; R.J. Ivison ;
Date 21 Dec 2004
Journal Astrophys.J. 616 (2004) 71
Subject astro-ph
AbstractWe present optical and near-IR photometry of 96 dusty, far-IR luminous galaxies. We have precise spectroscopic redshifts for all these galaxies yielding a median redshift of z=2.2. The majority, 78, are submm-detected galaxies lying at z=0.2-3.6, while the remaining 18 are optically-faint uJy radio galaxies at z=0.9-3.4 which are proposed to be similarly luminous, dusty galaxies whose dust emission is too hot to be detected in the submm. We compare the photometric and morphological properties of these distant, ultraluminous galaxies to local samples. We confirm that spectroscopically-identified far-IR luminous galaxies at z>1 display a wide variety in their optical-near-IR and near-IR colors, with only a modest proportion red enough to classify as unusually red. We show that on average luminous, high-z dusty galaxies are both brighter and redder in restframe optical passbands than UV-selected star-forming galaxies at similar z. HST ACS imaging of 20 sources demonstrates both indications of mergers and interactions, which may have triggered their activity, and structured dust within these galaxies. We derive a near-IR Hubble diagram for far-IR luminous galaxies, showing that they are typically fainter than high luminosity radio galaxies at similar z and exhibit more scatter in their K-band magnitudes. The typical extinction-corrected optical luminosity of the high-z population, assuming passive evolution, provides a good fit to the bright end of the luminosity function of luminous spheroidal galaxies seen in rich clusters at z<1. This adds to the growing evidence that these high z, far-infrared luminous sources identify star-formation and AGN fueling events in the early life of massive galaxies. [Abridged]
Source arXiv, astro-ph/0412574
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica