Galaxy and Mass Assembly (GAMA): Stellar-to-dynamical Mass Relation. I. Constraining the Precision of Stellar Mass Estimates

In this empirical work, we aim to quantify the systematic uncertainties in stellar-mass ( M _⋆ ) estimates made from spectral energy distribution (SED) fitting through stellar population synthesis (SPS) for galaxies in the local Universe by using the dynamical mass ( M _dyn ) estimator as an SED-ind...

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Autors principals:	M. Burak Dogruel, Edward N. Taylor, Michelle Cluver, Francesco D’Eugenio, Anna de Graaff, Matthew Colless, Alessandro Sonnenfeld
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2023-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Galaxy masses Galaxy properties Astronomy data modeling Astrostatistics strategies Galaxy stellar content
Accés en línia:	https://doi.org/10.3847/1538-4357/acde56
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