AST 221 problem set 1, links to models
The discovery of the planetary mass candidate companion to a young
solar analog is described in Lafrenière, Jayawardhana, and Van
Kerkwijk, 2008, Astrophys. J. (Letters), submitted
(see arXiv:0809.1424 and the
Gemini press release).
For problem set 1, you will need the
DUSTY models
(link
to original) from Chabrier et al.,
2000, Astrophys. J., 542,
464 and the COND models
(link
to original) from Baraffe et al.,
2003, Astron. &
Astroph., 402, 701.