From: Mamoru Doi (doi@ioa.s.u-tokyo.ac.jp)
Date: Sat May 11 2002 - 17:38:34 PDT
Hi,
The followings are the updated summary from Tokyo analysis.
(Saul, the same list as I sent you.)
In addition to Rob's list, I think S02-057 and S02-080
may be good candidates.
-Mamoru
SDF
name oldrank i' %inc
D S02-071 C 24.99 7.7 6.2 visible in Apr
D S02-072 D 24.32 8.4 8.6 0.5pixel off-center
D S02-073 D 23.75 8.7 8.8 almost at the center
B S02-074 C 23.83 72.5 49.9 seen in Apr
B S02-075 B 23.74 200.9 169.8 host seen in Apr
SDFw
name oldrank i' %inc
B S02-057 B 24.47 119.8 81.5 possible host seen in Apr
C S02-076 C 25.38 5.2 2.2 bright host, 0.5pixel off-center, AGN?
A S02-060 A 25.65 917.4 419.9 nothing seen in Apr
A S02-070 A 25.14 160.9 127.2 possible host seen in Apr
A S02-061 A 25.18 195.9 157.8 probable faint host seen in Apr
B S02-078 C 25.34 85.0 60.3 possible host seen in Apr
D S02-079 C 24.91 11.7 5.9 almost at the center, AGN?
C S02-080 B 25.38 10.2 5.3 0.5pixel off-center, AGN?
B S02-058 C 22.96 107.5 80.3 almost at the center, %inc is large
good targets for z=0.85: 075, 074, 058
good targets for z=1.2: 061, 070, 060, 057, 078
>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
Mamoru Doi
Institute of Astronomy
School of Science
Univ. of Tokyo
voice +81-422-34-5084
fax. +81-422-34-5041
doi@ioa.s.u-tokyo.ac.jp
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