From: Robert A. Knop Jr. (robert.a.knop@vanderbilt.edu)
Date: Sat May 11 2002 - 17:18:30 PDT
> I'm working right now on trying to figure out tonight's plan for Keck
> and Gemini. I'm still trying to bring in some more info from the
> analysis teams in Berkeley, Tennessee, Hawaii (the French team) and
> Tokyo, since we don't yet have quite enough confirmed candidates in
> the key HST redshift range.
Er... what do you mean by confirmed? I thought that's what you were
there for. Also, for finding out the redshifts....
If you want high-probability dim candidates to blow all night on, then
consider:
S02-056 \
S02-061 | --> All found by both DeepIDL scanners and Naoki, prio 5
S02-070 /
S02-060 --> Found by both Naoki and DeepIDL scanners, prio 4
S02-080 --> Found only by Naoki; by tomorrow I should see what this
looks like on the DeepIDL subtractions
T02-015 --> Promising looking mag 24 candidate CTIO; the same
I-magnitude that Albinoni was when we found it
Plus there are several brighter ones which could use shorter spectra.
Already here, though, unless all of these wash out quickly, there's more
than a night's worth of 10m work.
-Rob
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