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Spectral Energy Distribution Fitting with Markov Chain Monte Carlo: Methodology and Application to z = 3.1 Lyα-emitting Galaxies
(2011)
We 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, ...
The non-thermal broadband spectral energy distribution of radio galaxies
(Cambridge University Press, 2012)
I present a model for the non-thermal production of electromagnetic radiation in the jets of radio galaxies. The model goes far beyond the simple one-zone models usually applied to these sources. The transport equation is ...
The Accretion History of AGN: The Spectral Energy Distributions of X-Ray-luminous Active Galactic Nuclei
(2023)
Spectral energy distributions (SEDs) from X-ray to far-infrared (FIR) wavelengths are presented for a sample of 1246 X-ray-luminous active galactic nuclei (AGNs; L0.5–10 keV > 1043 erg s−1), with zspec < 1.2, selected from ...
New insights on the empirical predictability of spectral indicators for PV performance
(Pontificia Universidad Católica del PerúPE, 2023)
Modeling the spectral energy distribution of ULIRGs I: the radio spectra
(Astronomy and Astrophysics, 2008)
Modeling the spectral energy distribution of ULIRGs I: the radio spectra
(Astronomy and Astrophysics, 2008)