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Astron. Astrophys. 361, 63-67 (2000)

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Research Note

The Type Ia SN 1999by in NGC 2841: near-maximum BV(RI)c photometry and the multicolor light-curve shape (MLCS) method

I. Toth and R. Szabó

Konkoly Observatory, P.O. Box 67, 1525 Budapest, Hungary (tothi@konkoly.hu; rszabo@konkoly.hu)

Received 5 April 2000 / Accepted 27 June 2000

Abstract

Results of [FORMULA] CCD photometry of the bright supernova SN 1999by in the flocculent galaxy NGC 2841 are presented. The Multicolor Light-Curve Shape (MLCS) method is applied to fit the observed V lightcurve around its maximum-light period. The reddening and the luminosity correction parameters were estimated.

Key words: stars: supernovae: individual: SN 1999by – stars: supernovae: general – galaxies: individual: NGC 2841 – techniques: photometric

Send offprint requests to: I. Toth

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© European Southern Observatory (ESO) 2000

Online publication: September 5, 2000
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