Hostname: page-component-7bb8b95d7b-lvwk9 Total loading time: 0 Render date: 2024-09-18T20:52:30.295Z Has data issue: false hasContentIssue false
  • English
  • Français

The $K$-band luminosity functions of galaxies in high-redshift clusters

Published online by Cambridge University Press:  06 October 2004

Simon Ellis  and
Laurence Jones
Simon Ellis
Affiliation:
Anglo-Australian Observatory, PO Box 196, Epping, NSW, Australia email: [email protected]
Laurence Jones
Affiliation:
University of Birmingham, UK email: [email protected]
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.

$K$ band luminosity functions (LFs) of three, massive, high redshift clusters of galaxies are presented. The evolution of $K^{*}$, the characteristic magnitude of the LF, is consistent with purely passive evolution, and a redshift of formation $z_{{\rm f}} \approx 1.5-2$.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 435 - 437
Copyright
© 2004 International Astronomical Union