C. L. Doherty

1.5k total citations
35 papers, 953 citations indexed

About

C. L. Doherty is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, C. L. Doherty has authored 35 papers receiving a total of 953 indexed citations (citations by other indexed papers that have themselves been cited), including 31 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 7 papers in Nuclear and High Energy Physics. Recurrent topics in C. L. Doherty's work include Stellar, planetary, and galactic studies (29 papers), Astro and Planetary Science (18 papers) and Gamma-ray bursts and supernovae (13 papers). C. L. Doherty is often cited by papers focused on Stellar, planetary, and galactic studies (29 papers), Astro and Planetary Science (18 papers) and Gamma-ray bursts and supernovae (13 papers). C. L. Doherty collaborates with scholars based in Australia, Spain and Hungary. C. L. Doherty's co-authors include John C. Lattanzio, Pilar Gil-Pons, L. Siess, Herbert H. B. Lau, Maria Lugaro, S. W. Campbell, Amanda I. Karakas, Richard J. Stancliffe, Ross P. Church and M. Pignatari and has published in prestigious journals such as Science, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

C. L. Doherty

32 papers receiving 898 citations

Peers

C. L. Doherty

INSTR

NHEP

GEOPH

RADIA

B. J. McNamara United States

Dacheng Lin United States

Simone Scaringi United Kingdom

Alicia Soderberg United States

E. Glebbeek Netherlands

Dheeraj R. Pasham United States

J. S. Clark United Kingdom

Rachel Tunnicliffe United Kingdom

E. Romero‐Colmenero South Africa

N. Mouawad Germany

B. J. McNamara United States

C. L. Doherty

578 ×0.6

153 ×0.7

INSTR

90 ×0.4

NHEP

25 ×0.7

GEOPH

5 ×0.3

RADIA

Citations per year, relative to C. L. Doherty C. L. Doherty (= 1×) peers B. J. McNamara

Countries citing papers authored by C. L. Doherty

Since Specialization

Citations

This map shows the geographic impact of C. L. Doherty's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by C. L. Doherty with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. L. Doherty more than expected).

Fields of papers citing papers by C. L. Doherty

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. L. Doherty. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by C. L. Doherty. The network helps show where C. L. Doherty may publish in the future.

Co-authorship network of co-authors of C. L. Doherty

This figure shows the co-authorship network connecting the top 25 collaborators of C. L. Doherty. A scholar is included among the top collaborators of C. L. Doherty based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with C. L. Doherty. C. L. Doherty is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Gil-Pons, Pilar, et al.. (2025). An asymptotic giant branch star as the source of the abundance pattern of hyper-metal-poor star HE 1327-2326. Astronomy and Astrophysics. 703. A107–A107.

Volk, John, et al.. (2024). Incorporating model selection and uncertainty into forecasts of economic conditions in companion animal clinical veterinarian labor markets. Journal of the American Veterinary Medical Association. 263(2). 240–247. 3 indexed citations

Drout, M. R., B. M. Gaensler, C. S. Kochanek, et al.. (2023). Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II. Spectroscopic and Environmental Analysis of Thorne–Żytkow Object and Super-AGB Star Candidates. The Astrophysical Journal. 943(1). 18–18. 9 indexed citations

Doherty, C. L., et al.. (2023). Aluminium-26 from Massive Binary Stars. III. Binary Stars up to Core Collapse and Their Impact on the Early Solar System. The Astrophysical Journal. 951(2). 110–110. 11 indexed citations

Lugaro, Maria, Benoît Côté, M. Pignatari, et al.. (2022). The RADIOSTAR Project. Universe. 8(2). 130–130.

Gil-Pons, Pilar, et al.. (2022). Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars. Astronomy and Astrophysics. 668. A100–A100. 7 indexed citations

Diehl, R., Maria Lugaro, Alexander Heger, et al.. (2021). The radioactive nuclei and in the Cosmos and in the solar system. Publications of the Astronomical Society of Australia. 38. 31 indexed citations

García–Hernández, D. A., P. Ventura, C. L. Doherty, et al.. (2021). First models of the s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver. Astronomy and Astrophysics. 657. A28–A28. 3 indexed citations

Gil-Pons, Pilar, et al.. (2020). Nucleosynthetic yields of Z=1e-5 intermediate-mass stars. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 8 indexed citations

10.

Hartogh, J. W. den, Raphaël Hirschi, Maria Lugaro, et al.. (2019). The s process in rotating low-mass AGB stars. Astronomy and Astrophysics. 629. A123–A123. 15 indexed citations

11.

Doherty, C. L., et al.. (2019). Aluminium-26 from Massive Binary Stars. I. Nonrotating Models*. The Astrophysical Journal. 884(1). 38–38. 23 indexed citations

12.

Doherty, C. L., et al.. (2017). Partial mixing and the formation of 13C pockets in AGB stars: effects on the s-process elements. Monthly Notices of the Royal Astronomical Society. 471(1). 824–838. 18 indexed citations

13.

Bravo, Eduardo, et al.. (2016). Explosion of white dwarfs harboring hybrid CONe cores. Astronomy and Astrophysics. 589. A38–A38. 16 indexed citations

14.

Shingles, Luke J., C. L. Doherty, Amanda I. Karakas, et al.. (2015). Evolution and nucleosynthesis of helium-rich asymptotic giant branch models. Monthly Notices of the Royal Astronomical Society. 452(3). 2804–2821. 16 indexed citations

15.

Doherty, C. L., Pilar Gil-Pons, Herbert H. B. Lau, et al.. (2014). Super and massive AGB stars – III. Nucleosynthesis in metal-poor and very metal-poor stars – Z = 0.001 and 0.0001. Monthly Notices of the Royal Astronomical Society. 441(1). 582–598. 80 indexed citations

16.

Gil-Pons, Pilar, C. L. Doherty, Herbert H. B. Lau, et al.. (2013). Evolution and CNO yields ofZ= 10^-5stars and possible effects on carbon-enhanced metal-poor production. Astronomy and Astrophysics. 557. A106–A106. 27 indexed citations

17.

Doherty, C. L., Pilar Gil-Pons, Herbert H. B. Lau, John C. Lattanzio, & L. Siess. (2013). Super and massive AGB stars – II. Nucleosynthesis and yields – Z = 0.02, 0.008 and 0.004. Monthly Notices of the Royal Astronomical Society. 437(1). 195–214. 124 indexed citations

18.

Lau, Herbert H. B., Pilar Gil-Pons, C. L. Doherty, & John C. Lattanzio. (2012). The end of super AGB and massive AGB stars. Astronomy and Astrophysics. 542. A1–A1. 43 indexed citations

19.

Gil-Pons, Pilar & C. L. Doherty. (2010). The upper mass limit for the formation of TP-SAGB stars and the dredge-out phenomenon .. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 81(4). 974–979. 1 indexed citations

20.

Doherty, C. L. & John C. Lattanzio. (2006). Evolution and nucleosynthesis in super-AGB stars.. MmSAI. 77. 828. 2 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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