The 2025 release of Cloudy

Chamani M. Gunasekera, Peter A.M. van Hoof, Maryam Dehghanian, Priyanka Chakraborty, Gargi Shaw, Stefano Bianchi, Marios Chatzikos, Masahiro Tsujimoto, Gary J. Ferland

Research output: Contribution to journalArticlepeer-review

Abstract

We present the 2025 release of the spectral synthesis code CLOUDY, highlighting the significant enhancements in the scope and accuracy of the physics that have been made since the previous release. This key development resolves the Lyman α line into ϳ-resolved fine-structure doublets, thereby making CLOUDY useful to the X-ray community. We also updated the inner-shell ionization line energies and incorporated the 1 keV feature that is commonly observed in X-ray binaries. In addition, we updated the Stout database for the carbon isoelectronic sequence, improving the CLOUDY microphysical calculations for all wavelengths. The molecular network has also been extended with new silicon-bearing species, titanium-related reactions, and phosphorus-containing molecules, enhancing CLOUDY’s ability to model the complex chemistry relevant to exoplanet atmospheres. Finally, we outline future developments aimed at maximizing scientific returns from current and upcoming generations of observatories.

Original languageEnglish
Pages (from-to)120-133
Number of pages14
JournalRevista Mexicana de Astronomia y Astrofisica
Volume61
Issue number3
DOIs
StatePublished - 2025

Bibliographical note

Publisher Copyright:
© 2025 Instituto de Astronomía, Universidad Nacional Autónoma de México.

Keywords

  • Active galaxies
  • Astronomy software
  • Atomic data
  • Computational methods
  • Galaxy clusters
  • Molecular data

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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