Further analysis of the possible progenitor of SN 2008ax in NGC 4490

Details Further analysis of the possible progenitor of SN 2008ax in NGC 4490 Further analysis of the possible progenitor of SN 2008ax in NGC 4490

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1433....1l&link_type=abstract

The Astronomer's Telegram, #1433

Astronomy and Astrophysics

Astronomy

1

Optical, Novae, Supernovae, Transients

Scientific paper

W. Li, A. V. Filippenko, University of California, Berkeley, and S. D. Van Dyk, Spitzer Science Center, California Institute of Technology, on behalf of a larger team, report: We have analyzed the available HST/WFPC2 images of the field of SN 2008ax in NGC 4490, and derive the following photometry for the possible supernova progenitor star as previously reported in CBET 1290, CBET 1298, and ATEL 1417: F450W = 23.55 +/- 0.09, F606W = 23.64 +/- 0.13, and F814W = 22.58 +/- 0.08.

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