From tmatheso@salmo.harvard.edu Wed Jan 17 19:23:33 2001 Return-Path: Received: from cfa.harvard.edu (cfa.harvard.edu [131.142.10.1]) by phyast.nhn.ou.edu (8.10.2/8.10.2) with ESMTP id f0I1NWp24586 for ; Wed, 17 Jan 2001 19:23:32 -0600 Received: from salmo.harvard.edu (salmo [131.142.24.159]) by cfa.harvard.edu (8.9.2/8.9.2/cfunix M-S 0.1) with ESMTP id UAA03345 for ; Wed, 17 Jan 2001 20:23:31 -0500 (EST) Received: (from tmatheso@localhost) by salmo.harvard.edu (8.9.2/8.9.2/cfunix S 0.5) id UAA21430 for branch@phyast.nhn.ou.edu; Wed, 17 Jan 2001 20:23:31 -0500 (EST) Date: Wed, 17 Jan 2001 20:23:31 -0500 (EST) From: Thomas Matheson Message-Id: <200101180123.UAA21430@salmo.harvard.edu> To: branch@mail.nhn.ou.edu Status: R Content-Length: 882 David, I'm glad you're having fun with the spectra. It would be great to get more out of these. I've put all the 1984L spectra on our ftp site. ftp flipper.berkeley.edu login (anonymous) cd pub/matheson/sn1984l I put both the observed and deredshifted spectra in the directory (the -z.flm are deredshifted). This is all the spectra that we have. They are in f-lambda format. That is interesting about the narrow lines in 98T. The reduction shouldn't do that, and the two spectra were reduced by two different people (Doug Leonard and myself). Both spectra were obtained at Keck, so maybe there is something about the chip in LRIS and bright emission lines. I see a few dips on the blue side of some lines. (There is Na D absorption to the red of the 5876 line.) This is something to think about. Tom %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%