relative lightcurves

From: Greg Aldering (aldering@panisse.lbl.gov)
Date: Sat Mar 15 2003 - 17:43:29 PST

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    Hi Rob,

    I haven't located a description of what you did in the following
    areas:

     1) How did you set the relative B and V stretches?

        For P99 we performed independent B and V fits to the Hamuy
        data and then plotted s_V versus s_B and chose a ratio
        for s_V/s_B from that. This was a matter of some discussion,
        and not entirely trivial. You must have determined an initial
        ratio and then renormalized the templates to have s_V/s_B = 1,
        but how did you determine the ratio in the first place?

        We know that there is real scatter in this ratio, so the value
        used must be based on an ensemble of well-measured SNe in order to
        get the best (albeit approximate) value.

        Since you perform joint BV fits, this is probably even more
        important (esp. for low-z SNe) than it was for P99. Moreover,
        it would be preferable to eliminate this as a difference in
        your reanalysis if at all possible - that is, if you don't have
        any better choice than in P99 we should try to use the P99
        choice.

     2) How did you establish t_Bmax - t_Vmax with your new templates?
        Again, we know that this value is not really constant between
        SNe, but we treat it as such in SNminuit. Thus, it can't be determined
        from just one well-measure SN.

    These same questions apply to U-band and R-band as well, although the
    choice affects fewer SNe and has less impact of the comparison between
    your current fits and those from P99.

    Thanks,

    Greg



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