Fig. 10 from Optical and Infrared Photometry of the Type Ia Supernovae 1999da, 1999dk, 1999gp, 2000bk, and 2000ce

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Optical and Infrared Photometry of the Type Ia Supernovae 1999da, 1999dk, 1999gp, 2000bk, and 2000ce

Authors: Kevin Krisciunas, Mark M. Phillips, Christopher Stubbs, Armin Rest, Gajus Miknaitis, Adam G. Riess, Nicholas B. Suntzeff, Miguel Roth, S. E. Persson, and Wendy L. Freedman

Krisciunas et al. 2001 The Astronomical Journal 122 1616.

Provider: AAS Journals

Caption: Fig. 10.

BVRI photometry of SN 2000ce. Left : MLCS v/2.0 fits using Δ = −0.26. Right : Two templates from the Δm₁₅(B) method of Phillips et al. (1999) that fit the data equally well. This implies a greater than normal uncertainty in the time of maximum light and the magnitudes at maximum. The B, R, I, J, H, and K data have been offset vertically by +1, −1, −2, −3, −4, and −5 mag, respectively.

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