LumFunc: Luminosity Function Modeling

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LumFunc: Luminosity Function Modeling

Post by owlice » Wed Feb 01, 2012 2:58 am

[c]LumFunc: Luminosity Function Modeling[/c][/b]
Abstract: 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.

Credit: Cooray, Asantha; Milosavljević, Miloš


Bibcode: 2012ascl.soft01016C

ID: ascl:1201.016
Last edited by Ada Coda on Sun Dec 23, 2018 8:12 pm, edited 1 time in total.
Reason: Updated code entry.
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