From: Michael Wood-Vasey (wmwood-vasey@lbl.gov)
Date: Wed Nov 13 2002 - 00:14:29 PST
Dear Tony, Saul, and Peter,
I think things are fine w.r.t the lightcurves. Binning by day mislead
us into thinking we could tell more from the lightcurves than we
really can.
Specifically, SuF02-060 has one high point that pulls up the binned
value for the first night.
Perhaps it will be more helpful to look at the plots for all of the
images from each night. I had been plotting the binned data at Rob's
suggestion, but I've now provide both for all of the candidates in
question:
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-007-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-012-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-017-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-060-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-061-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-065-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-071-i_all.eps
http://supernova.lbl.gov/~wwoodvas/f2002/SuF02-081-i_all.eps
[and if I've missed any this time in the above list, I assume you
can figure out the pattern, '*i.eps' for binned-by-day plots,
'*i_all.eps' for plots with the value in each indivicual image given.]
These plots give a much better idea about how uncertain we are about
the measured fluxes.
- Michael
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