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
Received 5 April 2000 / Accepted 27 June 2000
Results of 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
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© European Southern Observatory (ESO) 2000
Online publication: September 5, 2000