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K‐Corrections and Spectral Templates of Type Ia Supernovae

  • Authors: E. Y. Hsiao, A. Conley, D. A. Howell, M. Sullivan, C. J. Pritchet, R. G. Carlberg, P. E. Nugent, and M. M. Phillips

Hsiao et al. 2007 The Astrophysical Journal 663 1187.

  • Provider: AAS Journals

Caption: Fig. 10.

Location of the observed filters at redshifts ﹩z=0.36﹩ (top) and ﹩z=0.54﹩ (bottom). We consider the same example of ﹩K﹩‐correction as in Fig. 9. The solid curves represent the rest‐frame ﹩B﹩ band, while the dotted curves represent the observed ﹩g_{\mathrm{M}\,}﹩, ﹩r_{\mathrm{M}\,}﹩, and ﹩i_{\mathrm{M}\,}﹩ bands. At redshifts where the observed and rest‐frame filter bands are misaligned, the observed color that straddles the rest‐frame filter band (highlighted for each plot) is the most important.

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