THE 2023 RELEASE OF Cloudy-Reference-Cited by-同舟云学术

THE 2023 RELEASE OF Cloudy

Published:2023-10-01 Issue:2 Volume:59 Page:327-343
ISSN:0185-1101
Container-title:Revista Mexicana de Astronomía y Astrofísica
language:
Short-container-title:RMxAA

Author:

Chatzikos Marios¹,Bianchi Stefano²,Camilloni Francesco³,Chakraborty Priyanka⁴,Gunasekera Chamani M.⁵,Guzmán Francisco⁶,Milby Jonathan S.⁷,Sarkar Arnab⁸,Shaw Gargi⁹,van Hoof Peter A. M.¹⁰,Ferland Gary J.¹

Affiliation:

1. Physics & Astronomy, University of Kentucky, Lexington, Kentucky, USA

2. Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, via della Vasca Navale 84, 00146 Roma, Italy.

3. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany.

4. Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA.

5. Physics & Astronomy, University of Kentucky, Lexington, Kentucky, USA.

6. 1. Physics & Astronomy, University of Kentucky, Lexington, Kentucky, USA. 2. Now at Physics & Astronomy, University of North Georgia, Dahlonega, Georgia, USA

7. Arts & Sciences Hive, University of Kentucky, Lexington, Kentucky, USA.

8. Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 70 Vassar St, Cambridge, MA, USA.

9. Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Mumbai 400005, India.

10. Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium

Abstract

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 control system. This change alone led us to adopt an annual release scheme, accompanied by a short release paper, the present being the inaugural. Significant changes to our atomic and molecular data have improved the accuracy of Cloudy predictions: we have upgraded our instance of the Chianti database from version 7 to 10; our H- and He-like collisional rates to improved theoretical values; our molecular data to the most recent LAMDA database, and several chemical reaction rates to their most recent UDfA and KiDA values. Finally, we describe our progress on upgrading Cloudy's capabilities to meet the requirements of the X-ray microcalorimeters aboard the upcoming XRISM and Athena missions, and outline future developments that will make Cloudy of use to the X-ray community.

Publisher

Universidad Nacional Autonoma de Mexico

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.astroscu.unam.mx/rmaa/RMxAA..59-2/PDF/RMxAA..59-2_mchatzikos-XII.pdf

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