From: Robert A. Knop Jr. (robert.a.knop@vanderbilt.edu)
Date: Tue Apr 15 2003 - 07:30:09 PDT
We asserted in P99 that we used CMB redshifts, rather than heliocentric
redshifts. And, indeed, some of the low-z redshifts in the
latest_sne.dat file that I think we used for fits in that paper are
slightly different from the heliocentric redshifts values in the
supernovae.dat file I inherited from (I think) Don.
However, they are *also* different from the CMB redshfit values in the
Gnumeric spreadsheet Alex C. sent me.
Clearly something is wrong somewhere. Do we really know how fast our
galaxy is moving relative to the CMB that much better now than we did
four years ago? (That would mightily surprise me.) Were the CMB
calculations used in P99 wrong? Or are Alex's calculations on his
spreadsheet wrong?
This needs to get resolved (along with the issue in the previous E-mail)
soon.
-Rob
-- --Prof. Robert Knop Department of Physics & Astronomy, Vanderbilt University robert.a.knop@vanderbilt.edu
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