activity
20152025
most citedImproved Fe II emission line models for AGN using new atomic datasets

46 citations · 176 across the 14 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2025

The 2025 Release of Cloudy

Chamani M. Gunasekera, Peter A. M. van Hoof, Maryam Dehghanian +6

We present the 2025 release of the spectral synthesis code Cloudy, highlighting significant enhancements to the scope and accuracy of the physics which have been made since the pre…

astro-ph.GA2025

H-, He-like recombination spectra -- V: On the dependence of the simulated line intensities on the number of electronic levels of the atoms

F. Guzmán, M. Chatzikos, G. Ferland

This paper presents a study of the dependence of the simulated intensities of recombination lines from hydrogen and helium atoms on the number of -resolved principal quantum…

astro-ph.GA2023

The 23.01 release of Cloudy

Chamani M. Gunasekera, Peter A. M. van Hoof, Marios Chatzikos +1

We announce the C23.01 update of Cloudy. This corrects a simple coding error, present since 1990, in one routine that required a conversion from the line-center to the mean…

astro-ph.GA20233 cited

The 2023 release of Cloudy

Marios Chatzikos, Stefano Bianchi, Francesco Camilloni +8

We describe the 2023 release of the spectral synthesis code Cloudy. Since the previous major release, migrations of our online services motivated us to adopt git as our version con…

astro-ph.GA2023

Revisiting the gas-phase chemical rate coefficients at high temperatures in CLOUDY

Gargi Shaw, Gary Ferland, M. Chatzikos

A two-body gas-phase reaction rate coefficient can be given by the usual Arrhenius-type formula which depends on temperature. The UMIST Database for Astrochemistry is a widely used…

astro-ph.GA202128 cited

High-ionization emission line ratios from quasar broad line regions: metallicity or density?

Matthew J. Temple, Gary J. Ferland, Amy L. Rankine +2

The flux ratios of high-ionization lines are commonly assumed to indicate the metallicity of the broad emission line region in luminous quasars. When accounting for the variation i…