ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

MAGPHYS: Multi-wavelength Analysis of Galaxy Physical Proper

Discussion topics for individual codes
User avatar
owlice
Guardian of the Codes
Posts: 1102
Joined: Wed Aug 04, 2004 4:18 pm
Location: Washington, DC

MAGPHYS: Multi-wavelength Analysis of Galaxy Physical Properties

Postby owlice » Thu Jun 16, 2011 11:50 am

MAGPHYS: Multi-wavelength Analysis of Galaxy Physical Properties

Abstract: MAGPHYS is a self-contained, user-friendly model package to interpret observed spectral energy distributions of galaxies in terms of galaxy-wide physical parameters pertaining to the stars and the interstellar medium. MAGPHYS is optimized to derive statistical constraints of fundamental parameters related to star formation activity and dust content (e.g. star formation rate, stellar mass, dust attenuation, dust temperatures) of large samples of galaxies using a wide range of multi-wavelength observations. A Bayesian approach is used to interpret the SEDs all the way from the ultraviolet/optical to the far-infrared.

Credit: da Cunha, Elisabete; Charlot, Stéphane

Site: http://www.iap.fr/magphys/magphys/MAGPHYS.html
http://adsabs.harvard.edu/abs/2008MNRAS.388.1595D

Bibcode: 2011ascl.soft06010D

ID: ascl:1106.010
Last edited by Ada Coda on Sun Feb 28, 2016 12:38 pm, edited 1 time in total.
Reason: Updated code entry.
Code-seeking owl at your service

Return to “Astrophysics Source Code Library”

Who is online

Users browsing this forum: No registered users and 8 guests

cron