Re: Subaru data analysis spectra

From: Gerson Goldhaber (g_goldhaber@lbl.gov)
Date: Thu Nov 18 2004 - 10:42:18 PST

Next message: Danny Lennon: "[INGNEWS] First Announcement: Hot Subdwarf Stars and Related Objects"

Previous message: Tony Spadafora: "final review of I-band paper"
In reply to: Gerson Goldhaber: "Re: Latest Subaru data analysis Oct 04"
Messages sorted by: [ date ] [ thread ] [ subject ] [ author ] [ attachment ]

Gerson Goldhaber wrote:
> Hi Chris,
Yes I agree that we should request VLT time to get spectra.
Here I repeat the priority as to which SNe should be measured.

>
> Based on light curve fits I have also assigned approximate z values. We
> need actual z values for these. In order of priority I suggest:
> z > 1. : 051,057,J02,J01, and SXDS_1-a
> 0.8 < z < 1. : 004,034,058,079
> 0.7 < z < 0.8 : 056,SXDS_1-b,SXDS_2-9
> All these would correspond to the U-band.
> cheers Gerson
>

-- 
Gerson Goldhaber
LBNL MS 50R2008
Berkeley, CA 94720
Tel. (510) 486-6210
Fax  (510) 486-6738

Next message: Danny Lennon: "[INGNEWS] First Announcement: Hot Subdwarf Stars and Related Objects"
Previous message: Tony Spadafora: "final review of I-band paper"
In reply to: Gerson Goldhaber: "Re: Latest Subaru data analysis Oct 04"
Messages sorted by: [ date ] [ thread ] [ subject ] [ author ] [ attachment ]

This archive was generated by hypermail 2.1.4 : Thu Nov 18 2004 - 10:44:56 PST