Image Details
Caption: Fig. 9.
BVRI and near‐infrared photometry of SN 2000bk. Left: MLCS v/2.0 fits using Δ = +0.43. Right : BVI fits based on templates from the Δm15(B) method of Phillips et al. (1999). The B, R, I, J, and H data have been offset vertically by +1, −1, −2, −4, and −5 mag, respectively. Most of the J‐band photometry was actually obtained with a Js filter.
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.