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Distance determination to 12 type II supernovae using the expanding photosphere method

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Figure

Figure 1. Optical light curves of four SNe during the first ∼120 days of their evolution
Figure 3. Optical light curves of four SNe during the first ∼120 days of their evolution
Figure 4. Dilution factors ζ as a function of the color temperature, computed at z = 0 from the E96 (blue dots) and D05 (red dots) atmosphere models for three different filter subsets ( {BV}, {BVI}, and {VI})
Figure 7. Line velocity evolution determined from the P Cygni absorption minima of four different features during ∼100 days after discovery
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