<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>

COPY SCRIPT

For further information contact us at helpdesk@openaire.eu

Supernovae in Galaxy Clusters

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2005Embargo end date: 01 Jan 2003 English Publisher:Springer Science and Business Media LLCJournal:International Astronomical Union Colloquium, volume 192, pages 367-371 (issn: 0252-9211,

Authors: Alexei V. Filippenko; Keren Sharon; Avishay Gal-Yam; Dan Maoz; Puragra Guhathakurta; Francisco Prada;

doi: 10.1007/3-540-26633-x_51 , 10.1017/s025292110000943x , 10.48550/arxiv.astro-ph/0307520

arXiv: http://arxiv.org/abs/astro-ph/0307520

Supernovae in Galaxy Clusters

- Summary
- Subjects
- Metrics

Abstract

SummaryWe present the results of several surveys for supernovae (SNe) in galaxy clusters. SNe discovered in deep, archival HST images were used to measure the cluster SN Ia rate to z = 1. A search for SNe in nearby (0.06 ≤ z ≤ 0.2) Abell galaxy clusters yielded 15 SNe, 12 of which were spectroscopically confirmed. Of these, 7 are cluster SNe Ia, which we will use to measure the SN Ia rate in nearby clusters. This search has also discovered the first convincing examples of intergalactic SNe. We conclude with a brief description of ongoing and future cluster SN surveys.

Related Organizations

University of California, Berkeley
United States
Tel Aviv University
Israel
Herzberg Institute of Astrophysics
Canada
National Research Council Canada
Canada

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	1
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average