This page contains information about the software pipeline used to analyze the physical properties of star clusters in the LEGUS
The software pipeline is hosted on bitbucket
. It can be downloaded via git by doing
git clone https://bitbucket.org/krumholz/legus-cluster-pipeline.git
The libraries for use with the pipeline can be downloaded from the Data Products
page, or from the list below:
The naming convention for these files is TRACKS_IMF_EXCURVE_*, where TRACKS is the set of stellar evolution tracks used (Padova Z = 0.02, Padova Z = 0.04, Padova Z = 0.08, or Geneva Z = 0.014 non-rotating), IMF is the initial mass function (kroupalim = Kroupa (2001), chabrier = Chabrier (2005)), and EXCURVE is the extinction curve shape (Milky Way or starburst). See Krumholz et al., 2015, submitted to ApJ for details.