| Gary J. Ferland | |
| Birth Name: | Gary Joseph Ferland |
| Birth Date: | 10 May 1951 |
| Birth Place: | Washington D.C., US |
| Fields: | Astrophysics |
| Thesis Title: | Spectroscopic Observations of Nova V1500 Cygni |
| Thesis Year: | 1978 |
| Doctoral Advisor: | David L. Lambert Gregory Shields |
| Awards: | Catedratico de Excelencia Guillermo Haro, (2016) AAS Fellow AAAS Fellow RAS Fellow |
Gary Joseph Ferland (born May 10, 1951, in Washington D.C.) is an American astrophysicist. He is a professor of Physics and Astronomy at The University of Kentucky.[1] He is best known for developing the astrophysical simulation code Cloudy, for his work on physical processes in ionized plasmas, and investigations of the chemical evolution of the cosmos.
He joined the University of Texas Astronomy Department in 1973 wherehe received his Ph.D. in 1978, studying the 1975 explosion of V1500 Cygni atMcDonald Observatory.[2] From 1978 to 1980 he was at the Institute of Astronomy, Cambridgewhere he worked with Martin Rees on International Ultraviolet Explorer observations of radio galaxies.[3] He joined the faculty of the University of Kentucky in 1980. The American Astronomical Society'sAstronomy Genealogy Project[4] lists the 17 PhDs hehas supervised.[5]
Ferland is a Fellow of the American Astronomical Society,[6] and has served on their Governing Council in addition to their Publications Board.[7] He was named Fellow of the American Association for the Advancement of Science[8] in 2023 and is a Fellow of the Royal Astronomical Society. He is a long-time member of the International Astronomical Union[9] where he was on the Organizing Committee of Division VI (2003–2009)and Commission 34 (2006–2012) Interstellar Matter.
His research involves the interactions between light and matter, especially how the photons we receive can tell us about events at the edges of the Universe.[10] He has also studied such diverse environmentsas the interstellar medium, planetary nebulae, H II region, photodissociation regions, and Active Galactic Nuclei.His discovery of a tidal disruption event in the Seyfert galaxy NGC 548[11] was listed by Science News as one of the top ten discoveries in astronomy in 1986.[12]
He is best known as a developer of the open-source spectral simulation code Cloudy,[13] a project he started at Cambridge in 1978. The code uses large databases of atomic, molecular and interstellar grain cross sections and rate coefficients to determine the physical state of a non-equilibrium plasma, the emission or absorption properties of Interstellar clouds,and predict the observed spectrum. Cloudy helps to understand the emission and absorption spectra of plasmas and to interpret observational data from various astrophysical sources.Nature Astronomy named Cloudy their first Code of honour[14] in their Access Code[15] series.
He has edited two books in addition to more than 700 articles on astronomy and astrophysics.[16] He is a co-author on the influential[17] 2006 textbook Astrophysics of Gaseous Nebulae and Active Galactic Nuclei, written with Donald E. Osterbrock of Lick Observatory and the University of California at Santa Cruz.
As a science communicator, Ferland has given popular-leveltalks at the Smithsonian Institution, the Cleveland Museum of Natural History,and numerous clubs, organizations, and classes across the Bluegrass region.
Ferland was named as American Astronomical Society Fellow in 2021 and as Fellow of the American Association for the Advancement of Science in 2022.[18] Both cited his development of the Cloudy spectral simulation code. In 2016 he received Catedratico de Excelencia Guillermo Haro from the National Institute of Astrophysics, Optics and Electronics, (Tonantzintla, Puebla, Mexico). A Festschrift was held in his honor at National Autonomous University of Mexico, Mexico City in 2016.[19]
He has received many honorary visiting positions:
Ferland was the son of Andrew Joseph Ferland, a career officer in the United States Air Force, and Ida Marie Schneemann. He was raised in Washington D.C., the Panama Canal Zone, Alaska, Florida, and Texas, where he received a BS in Physics with Special Honors in 1972 at the University of Texas.[21]
He married Ann Elizabeth Clemmens (1952-) in 1983. They have two children, Peter Andrew (1987-) and Elizabeth Marie (1989-).