StarFISH is a suite of programs designed to determine the star formation history (SFH) of a stellar population, given multicolor stellar photometry and a library of theoretical isochrones. It constructs a library of synthetic color-magnitude diagrams from the isochrones, which includes the effects of extinction, photometric errors and completeness, and binarity. A minimization routine is then used to determine the linear combination of synthetic CMDs that best matches the observed photometry. The set of amplitudes modulating each synthetic CMD describes the star formation history of the observed stellar population.
References:
StarFISH in the Literature:
Some published work that has used StarFISH:
The latest version is 1.1-p1, which was released on 2 June 2004. There are two tarballs. Both contain the StarFISH source code and auxiliary programs and scripts, as well as the user manual. Both also include the latest Padua isochrones (note that StarFISH should work with nearly any modern isochrones). The full version adds a sample parsed isochrone library, and a sample synthetic CMD library.
I have created some message boards for the StarFISH community. Post early, post often!
This release fixes a number of bugs in SFH-1.1:
If you already have downloaded SFH-1.1, you can simply download this small patch file. Apply the patch like this:
Some of the new features include: