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Supernovae in Galaxy Clusters

Published online by Cambridge University Press:  19 September 2016

A. Gal-Yam ,
D. Maoz ,
K. Sharon ,
F. Prada ,
P. Guhathakurta  and
A.V. Filippenko
K. Sharon
Affiliation:
School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel; avishay@wise.tau.ac.il
F. Prada
Affiliation:
Instituto de AstrofÃ-sica de Canarias and The Isaac Newton Group, Spain
P. Guhathakurta
Affiliation:
Herzberg Institute of Astrophysics, National Research Council, Canada
A.V. Filippenko
Affiliation:
Department of Astronomy, University of California, Berkeley, CA, USA

Summary

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We 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.

Information

Type
Part V Supernovae: Searches/Statistics
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 367 - 371
Copyright
Copyright © Springer-Verlag 2005

References

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