SN 2005cs one-year photometry (Pastorello+, 2009)

Astronomy and Astrophysics – Astronomy

Scientific paper

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Supernovae, Photometry: Ubvri, Photometry: Infrared

Scientific paper

The systematic photometric monitoring of SN 2005cs began on 2005 June 30, 3d after the SN discovery. However, earlier unfiltered images obtained by amateur astronomers were also collected. These data are particularly important because they show the light-curve evolution soon after the shock breakout. There is no evidence of the SN presence in images obtained on 2005 June 26, but the SN was clearly visible the subsequent day. The SN was then followed for one year (until 2006 July) in the optical bands, and until 2006 December in the NIR. A few optical observations obtained in 2007 show no trace of the SN.
(3 data files).

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