The survey, in a nutshell:
1 square degree,
3 filters (Sloan-like g'r'i')
3 seasons
33 epochs
We use image subtraction to detect variability. We have found 36000
variable objects, and we have over 80000 light curves.
We use
DAOPHOT to extract fluxes. There are roughly 2.5 million sources
detected in each passband. We have point source photometry for 4.7
million different sources; about 1 million sources detected in all 3
filters.
WARNING:
The photometry is not
yet calibrated. We provide "semi-instrumental" magnitudes. We used a
constant zero point (provided by the observatory) for all images.
From one chip to another, there can be differences of a few tenths of
a magnitude.
You can also check out some cool movies, made by Joel Hartman .
The files are publicly available and you can do whatever you want with
the data. It is nice to let us know what you do though (dfb AT'
astro 'DOT' livjm 'DOT' ac 'DOT' uk).
There are two different groups of variables. One is for stars that
have a counterpart in the deep reference image (most "regular"
variables like Cepheids, Miras, LBVs, red giants, etc.). Download the
summary file and the light curves (gzipped, 30 Mb).
The other group is for stars that do not have a counterpart
(one-off things, possible novae, fast microlensing events, etc.).
Download the summary file and
the light curves (gzipped, 23
Mb).
Papers
Here is a list of links to papers based
on these data. Some of the papers have been written by other groups
making use of the data.
If you want your paper to be listed here, let me know (dfb AT'
astro 'DOT' livjm 'DOT' ac 'DOT' uk).
This is the whole galaxy, with the movie region highlighted [Credit:
T.A.Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) and M.Hanna
(NOAO/AURA/NSF)]:

Here is the
movie
for this region.
Zooming in on a sub-region .
Last update on Oct 23 2006 ![]()
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