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CfA3: 185 Type Ia Supernova Light Curves from the CfA

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Figure

Table 1 SN Ia Discovery Data
Figure 2. Histograms of time of first observation in the rest frame, relative to maximum light in B, as calculated by MLCS2k2
Figure 5. Synthesized natural system Keplercam BV r  i  passbands (solid curves) with Bessell (1990) BV and SDSS r  i  overplotted (dashed curves).
Figure 6. Nine of the better CfA3 SN Ia light curves. Error bars are smaller than the symbols in most cases
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