Deep Lens Survey Transient Detections
The DLS imaged each piece of sky in its footprint 20 different times in each filter. In addition to our main data products, which are stacks of these images (and corresponding catalogs), we differenced the images in real time to find transient objects: supernova, asteroids, etc. Here is an archive of our discoveries. For a summary and analysis, see the Becker et al paper.
KPNO, March 24 - 28, 2004     | CTIO, March 18 - 23, 2004 |
CTIO, Jan 2004     | KPNO, Oct 2003     |
CTIO, Apr 2003 |
CTIO, Feb27-Mar5 2003, and KPNO, Mar6-Mar9 2003 (1000 numbered series) |
KPNO, Jan 2003 | KPNO, Nov 2002     |
CTIO, Apr 2002     | CTIO, Feb 2002 |
CTIO, Jan 2002     | KPNO, Dec 2001     |
KPNO, Nov 2001 | CTIO, Mar 2001     |
CTIO, Feb 2001     | CTIO, Jan 2001 |
KPNO, Dec 2000     | KPNO, Nov 2000     |
CTIO, Apr 2000 | CTIO, Mar 2000     |
KPNO, Jan 2000     | KPNO, Dec 1999 |