Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-02T18:46:48.782Z Has data issue: false hasContentIssue false
  • English
  • Français

News from z≲6-10 galaxy candidates found behind gravitational lensing clusters

Published online by Cambridge University Press:  01 December 2006

D. Schaerer ,
A. Hempel ,
R. Pelló ,
E. Egami  and
J. Richard
D. Schaerer
Affiliation:
Geneva Observatory, Ch. des Maillettes 51, CH-1290 Sauverny, Switzerland email: [email protected] Observatoire Midi-Pyréneés, 14 Avenue E. Belin, F-31400Toulouse, France
A. Hempel
Affiliation:
Geneva Observatory, Ch. des Maillettes 51, CH-1290 Sauverny, Switzerland email: [email protected]
R. Pelló
Affiliation:
Observatoire Midi-Pyréneés, 14 Avenue E. Belin, F-31400Toulouse, France
E. Egami
Affiliation:
Caltech Astronomy, MC105-24, Pasadena, CA 91125, USA
J. Richard
Affiliation:
Observatoire Midi-Pyréneés, 14 Avenue E. Belin, F-31400Toulouse, France Steward Observatory, University Arizona, AZ 85721, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We summarise the current status of our project to identify and classify ~ 6-10 galaxies thanks to strong gravitational lensing. Building on the detailed work by Richard et al. (2006), we present results from new follow-up observations undertaken with the ACS/HST and the Spitzer space telescope and compare our results with findings from the Hubble Ultra-Deep Field (UDF).

Keywords

galaxieshigh-redshiftgravitational lensing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 571 - 572
Copyright
Copyright © International Astronomical Union 2007

References

Bouwens, et al. 2004, ApJ, 616, L79CrossRefGoogle Scholar
Bouwens, et al. 2005, ApJ, 624, L5CrossRefGoogle Scholar
Hempel, et al. 2007, to be submittedCrossRefGoogle Scholar
Richard, et al. 2006, A&A 456, 861Google Scholar
Schaerer, et al. 2006, The Messenger, 125, 20Google Scholar