From: Serena Nobili (serena@lpnhep.in2p3.fr)
Date: Wed Oct 27 2004 - 07:43:11 PDT
Hi Greg,
I am sorry for the delay in answering your email.
I have already addressed all your comments in the most recent version of
the paper, apart from the ones on SN99Q, that as you know, keeps
changing. I copy here part of your comments or questions that need a
direct answer.
Cheers
Serena
G: Greg
S: Serena
G: You used the Lira method on the Riess'Sne?
S: Actually, Phillips et al. (1999) did it. I have used the same method
on the Jha data.
G: In Fig3 two Sne are as or more deviant than 98es and 99dq.
S: Yes, it is true. But the problem with 98es and 99dq is that they become
redder after extinction correction than before correction.
G. In Fig4 the deviant supernovae lack a second peak.
S: Although they show a less prominent second peak, there are others with
the same lightcurve shape (e.g. 92bc) but that are in the ballpark. Thus,
we cannot claim they are deviant because of this lightcurve property.
G: Caption of Table 4. Circle around the +- sign. "Double valued? Pick the
right one"
S: I don't understand your comment. The note to the table refers to the
last column in which you have a value +- its uncertainty, and the note
explain how the value and the uncertainty are computed.
----------------------------------------------------------------------
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