LumFunc: Luminosity Function Modeling

Details LumFunc: Luminosity Function Modeling LumFunc: Luminosity Function Modeling

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ascl.soft01016c&link_type=abstract

Astrophysics Source Code Library, record ascl:1201.016

Astronomy and Astrophysics

Astrophysics

Scientific paper

LumFunc is a numerical code to model the Luminosity Function based on central galaxy luminosity-halo mass and total galaxy luminosity-halo mass relations. The code can handle rest b_J-band (2dFGRS), r'-band (SDSS), and K-band luminosities, and any redshift with redshift dependences specified by the user. It separates the luminosity function (LF) to conditional luminosity functions, LF as a function of halo mass, and also to galaxy types. By specifying a narrow mass range, the code will return the conditional luminosity functions. The code returns luminosity functions for galaxy types as well (broadly divided to early-type and late-type). The code also models the cluster luminosity function, either mass averaged or for individual clusters.

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