Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ∼ 1 and z ∼ 2 in the Absence of Infrared Data

Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ∼ 1 and z ∼ 2 in the Absence of Infrared Data

Robust estimation of star formation rates (SFRs) at higher redshifts ( z ≳ 1) using UV–optical–near-infrared (NIR) photometry is contingent on the ability of spectral energy distribution (SED) fitting to constrain the dust attenuation, stellar metallicity, and star formation history (SFH) simultaneo...

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Bibliographic Details
Main Authors: Chandler Osborne, Samir Salim
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy formation
Galaxy evolution
Galaxy masses
Galaxy properties
Star formation
Spectral energy distribution
Online Access:https://doi.org/10.3847/1538-4357/ad17c8

Internet

https://doi.org/10.3847/1538-4357/ad17c8

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