From: Robert A. Knop Jr. (robert.a.knop@vanderbilt.edu)
Date: Mon Apr 05 2004 - 14:01:49 PDT
Report from Rob and Rachel:
Summary: we missed a bunch of them because they are very low percent
increase. At least three were near the middle of brightish spiral
galaxies.
I have saved a candidate for each of Adam's that we missed.
Specifics:
> tile 24
>
> 1) Pele
> 12:36:25.94
> +62:09:37.44
This is our acs04-176, and is on our list of things to watch.
> 2) Adu
> 12:36:20.8, 62:10:19.7
This is our acs04-177, and is on our list of things to watch.
> 3) Beckenbauer
> 12:36:41.1, 62:11:41.3
This is off in the corner of the "canted" field, and was not in the
region that we subtracted.
> 4) Cobi
> host: 12:36:06.4, 62:12:53.35
We're not sure where we have identified this one yet. Our software
didn't pick it up, and there's no obvious residual in the area that
could be this candidate. There is a big galaxy here, and there is a
*faint*, almost candidate (that was not identified by our software) that
is saved as acs04-192 which is a coincidence of cosmic ray.s
> 5) Maradona
> 12:36:19.86
> 62:13:48.09
In the middle of a galaxy, %INC was 15, which was below our cut of 25.
Saved as acs04-193.
> 6) Chinalia
> 12:36:27.06
> 62:15:09.70
This one had a %INC of 19.5 and so got thrown out. I saved it as
acs04-194.
> 7) Salas
> ra=12:38:03.64, dec=62:17:11.9
This one had %INC of 18, and is in the middle of a bright galaxy.
There's a spot there from a year ago. Type II in a giant HII region?
> 8) Zamorano
> host: 12:37:09.42, 62:22:14.75
We found this as acs04-076
> 9) pine
> 12:37:06.7, 62:21:17.75
This one was missed as 15%INC. We have saved it as acs04-196.
> 10) Mahogany
> 12:37:22.7, 62:09:35.75
This is acs04-096.
> 11) Teak
> 12:37:21.33 62:09:35.24
This was missed completely by our software. It's weird; it's on a
galaxy that has a bright spot right next to it, and the candidate is
right next to the spot. I don't know why our software missed it; it
didn't even get picked up to fail the cuts. I have saved it as
acs04-197.
-Rob & Rachel
-- --Prof. Robert Knop Department of Physics & Astronomy, Vanderbilt University robert.a.knop@vanderbilt.edu
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