Discovery of four SN candidates as a part of A Survey for Supernovae in Massive High-Redshift Clusters

Details Discovery of four SN candidates as a part of A Survey for Supernovae in Massive High-Redshift Clusters Discovery of four SN candidates as a part of A Survey for Supernovae in Massive High-Redshift Clusters

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..723....1s&link_type=abstract

The Astronomer's Telegram, #723

Astronomy and Astrophysics

Astronomy

2

Optical, Novae, Supernovae

Scientific paper

K. Sharon (Tel Aviv U.), A. Gal-Yam (Caltech), and D. Maoz (Tel Aviv U.) report for a larger collaboration, including M. Donahue (MSU), H. Ebeling (IfA), R. Ellis (Caltech), A. Filippenko (UCB), R. Foley (UCB), W. Freedman (OCIW), J.-P. Kneib (Marseille), R. Kirshner (CfA), T. Matheson (NOAO), J. Mulchaey (OCIW), M. Phillips (OCIW), V. Sarajedini (UF) and M. Voit (MSU) (http://www.astro.caltech.edu/~avishay/hst.html): We have used the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST), to image the galaxy clusters CL1226+3332 (z=0.888) and MACS 0647+7015 (z=0.584) for one orbit each (2209s and 2584s respectively) with the F814W filter, as part of our cycle 14 survey for SNe in galaxy clusters (GO 10493, PI Gal-Yam).

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