Spectral Energy Distribution Fitting with Markov Chain Monte Carlo: Methodology and Application to z = 3.1 Lyα-emitting Galaxies

Astrophysical Journal

dc.creatorAcquaviva, V.
dc.creatorGuaita, L.
dc.date2020-03-11T20:36:47Z
dc.date2022-07-08T17:17:37Z
dc.date2020-03-11T20:36:47Z
dc.date2022-07-08T17:17:37Z
dc.date2011
dc.date.accessioned2023-08-22T01:28:32Z
dc.date.available2023-08-22T01:28:32Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/241094
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8306041
dc.descriptionWe present GalMC, a Markov Chain Monte Carlo (MCMC) algorithm designed to fit the spectral energy distributions (SEDs) of galaxies to infer physical properties such as age, stellar mass, dust reddening, metallicity, redshift, and star formation rate. We d
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/737/2/47
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleSpectral Energy Distribution Fitting with Markov Chain Monte Carlo: Methodology and Application to z = 3.1 Lyα-emitting Galaxies
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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