From: Andy Howell (howell@astro.utoronto.ca)
Date: Mon Mar 01 2004 - 08:11:40 PST
On Mon, 1 Mar 2004, Serena Nobili wrote:
> >I can give you an example of where the chi_sq minimum value is not used.
> >When Andy determines the SN epoch, he takes the average of the best five(?)
> >fits. I've cc'ed this e-mail to Andy so he can explain to us why
> >he chooses this method of analysis.
> >
>
> As I said above, I think this is due to the fact that the chisq is not a
> good indicator for the goodness of the fit of SN spectra. This depends on
> the signal-to-noise but also on the differences in the spectral features.
> I hope Andy agrees with me about this point.
Hi,
It will take me a little longer to digest all of the comments here, but I
can reply immediately to this question of how I calculate a date from SN
spectroscopy fits. I calculate a weighted average based on the best 5
fits to a SN spectrum. The weights are the inverse of the square of the
goodness-of-fit parameter. The goodness of fit parameter is like a
chi-sq, but without the errors. So if "S" is the goodness of fit
parameter, and "D" is the date I determined from that fit, then the
average date is:
5
__ Di/Si^2
Dav= \ _________
/
__ 1/Si^2
i=1
Thus if the best fit is much better than the rest, it dominates the date
determination. However, allowing the other fits to have some influence
gets around the discreteness problem. Dates are only good to +/- 1 day on
SN spectra (if that). Since different SNe have differnt distributions of
elements, what looks like day 15 on one SN may well be day 17 on another
SN. By averaging you beat down some of this scatter. At the same time,
by doing a weighted average, you ensure that the best fits drive the
average. I have done tests on the effects of different indicators of the
date, e.g. (a) just the best fit date, (b) the median of the top five, (c)
the weighted average. The weighted average gave the least dispersion in
spectroscopic day vs photometric day plots.
-Andy
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