activity
20052024
most citedThe 2013 Release of Cloudy

446 citations · 2k across the 32 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2024★ 1 cited

Recent Update of Gas-Phase Chemical Reactions and Molecular Lines of TiO in Cloudy

Gargi Shaw, Gary J. Ferland, Phillip Stancil +1

We present our current update on the gas-phase chemical reactions and spectral lines of TiO in the spectral synthesis code Cloudy. For this purpose, we have added 229 Ti-related re…

astro-ph.GA2017

The 2017 Release of Cloudy

G. J. Ferland, M. Chatzikos, F. Guzmán +8

We describe the 2017 release of the spectral synthesis code Cloudy. A major development since the previous release has been exporting the atomic data into external data files. This…

astro-ph.IM2015★ 36 cited

Stout: Cloudy's Atomic and Molecular Database

M. L. Lykins, G. J. Ferland, R. Kisielius +6

We describe a new atomic and molecular database we developed for use in the spectral synthesis code Cloudy. The design of Stout is driven by the data needs of Cloudy, which simulat…

astro-ph.SR2015★ 36 cited

The Abundances of Light Neutron-Capture Elements in Planetary Nebulae III. The Impact of New Atomic Data on Nebular Selenium and Krypton Abundance Determinations

N. C. Sterling, R. L. Porter, H. L. Dinerstein

The detection of neutron(n)-capture elements in several planetary nebulae (PNe) has provided a new means of investigating s-process nucleosynthesis in low-mass stars. However, a la…

astro-ph.HE2015★ 25 cited

Accurate determination of the free-free Gaunt factor. II - relativistic Gaunt factors

P. A. M. van Hoof, G. J. Ferland, R. J. R. Williams +4

When modelling an ionised plasma, all spectral synthesis codes need the thermally averaged free-free Gaunt factor defined over a very wide range of parameter space in order to prod…

astro-ph.GA2015★ 12 cited

Collisional excitation of [C II], [O I] and CO in Massive Galaxies

R. E. A. Canning, G. J. Ferland, A. C. Fabian +5

Many massive galaxies at the centres of relaxed galaxy clusters and groups have vast reservoirs of cool (~10,000 K) and cold (~100 K) gas. In many low redshift brightest group and…