L. A. Nelson

1.8k total citations
34 papers, 1.0k citations indexed

About

L. A. Nelson is a scholar working on Astronomy and Astrophysics, Instrumentation and Oceanography. According to data from OpenAlex, L. A. Nelson has authored 34 papers receiving a total of 1.0k indexed citations (citations by other indexed papers that have themselves been cited), including 32 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 3 papers in Oceanography. Recurrent topics in L. A. Nelson's work include Stellar, planetary, and galactic studies (23 papers), Astro and Planetary Science (12 papers) and Gamma-ray bursts and supernovae (11 papers). L. A. Nelson is often cited by papers focused on Stellar, planetary, and galactic studies (23 papers), Astro and Planetary Science (12 papers) and Gamma-ray bursts and supernovae (11 papers). L. A. Nelson collaborates with scholars based in Canada, United States and United Kingdom. L. A. Nelson's co-authors include S. Rappaport, P. C. Joss, Keith A. MacCannell, S. Rappaport, W. Y. Chau, Eugene Chiang, Bill Paxton, Philipp Podsiadlowski, B. Kalomeni and Ben Dorman and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

L. A. Nelson

33 papers receiving 988 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
L. A. Nelson Canada 17 985 213 120 78 36 34 1.0k
T. Y. Steiman-Cameron United States 16 717 0.7× 132 0.6× 47 0.4× 106 1.4× 21 0.6× 47 772
Ryan M. O’Leary United States 13 1.1k 1.1× 94 0.4× 50 0.4× 219 2.8× 25 0.7× 15 1.1k
Peter Tamblyn United States 14 928 0.9× 254 1.2× 31 0.3× 73 0.9× 24 0.7× 38 960
R. P. S. Stone United States 16 907 0.9× 265 1.2× 30 0.3× 124 1.6× 24 0.7× 41 962
J. P. D. Mittaz United Kingdom 14 982 1.0× 119 0.6× 55 0.5× 320 4.1× 12 0.3× 22 1.1k
M. A. Hausman United States 13 445 0.5× 119 0.6× 79 0.7× 57 0.7× 35 1.0× 25 495
Patricia T. Boyd United States 14 434 0.4× 51 0.2× 45 0.4× 122 1.6× 53 1.5× 46 526
J. A. de Freitas Pacheco France 19 923 0.9× 220 1.0× 41 0.3× 302 3.9× 59 1.6× 122 1.0k
B. Klein United States 12 1.0k 1.1× 190 0.9× 69 0.6× 164 2.1× 22 0.6× 22 1.1k
Steven M. Crawford South Africa 15 1.1k 1.1× 263 1.2× 29 0.2× 337 4.3× 33 0.9× 53 1.2k

Countries citing papers authored by L. A. Nelson

Since Specialization
Citations

This map shows the geographic impact of L. A. Nelson'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 L. A. Nelson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. A. Nelson more than expected).

Fields of papers citing papers by L. A. Nelson

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by L. A. Nelson. 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 L. A. Nelson. The network helps show where L. A. Nelson may publish in the future.

Co-authorship network of co-authors of L. A. Nelson

This figure shows the co-authorship network connecting the top 25 collaborators of L. A. Nelson. A scholar is included among the top collaborators of L. A. Nelson 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 L. A. Nelson. L. A. Nelson is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Jayaraman, Rahul, S. Rappaport, L. A. Nelson, et al.. (2022). TIC 5724661: A Long-period Binary with a Pulsating sdB Star and δ Scuti Variable. The Astrophysical Journal. 936(2). 123–123. 2 indexed citations
2.
Rappaport, S., D. W. Kurtz, G. Handler, et al.. (2021). A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020. Monthly Notices of the Royal Astronomical Society. 14 indexed citations
3.
Heinke, C. O., Eric W. Koch, Robert C. Andrews, et al.. (2020). The X-ray emissivity of low-density stellar populations. Monthly Notices of the Royal Astronomical Society. 492(4). 5684–5708. 12 indexed citations
4.
Thorstensen, J. R., S. Rappaport, Andrew W. Mann, et al.. (2019). A 9-h CV with one outburst in 4 yr of Kepler data. Monthly Notices of the Royal Astronomical Society. 489(1). 1023–1036. 12 indexed citations
5.
Borkovits, T., Simon Albrecht, S. Rappaport, et al.. (2018). EPIC 219217635: A Doubly Eclipsing Quadruple System Containing an Evolved Binary. Monthly Notices of the Royal Astronomical Society. 17 indexed citations
6.
Rappaport, S., Andrew Vanderburg, L. A. Nelson, et al.. (2017). WD 1202-024: the shortest-period pre-cataclysmic variable. Monthly Notices of the Royal Astronomical Society. 471(1). 948–961. 14 indexed citations
7.
Nelson, L. A., et al.. (2015). POPULATION SYNTHESIS OF CATACLYSMIC VARIABLES. I. INCLUSION OF DETAILED NUCLEAR EVOLUTION. The Astrophysical Journal. 809(1). 80–80. 65 indexed citations
8.
LaCourse, Daryll M., Kian J. Jek, Thomas L. Jacobs, et al.. (2015). Keplereclipsing binary stars – VI. Identification of eclipsing binaries in theK2Campaign 0 data set. Monthly Notices of the Royal Astronomical Society. 452(4). 3561–3592. 23 indexed citations
9.
Nelson, L. A., et al.. (2014). DISCOVERY OF TWO NEW THERMALLY BLOATED LOW-MASS WHITE DWARFS AMONG THE KEPLER BINARIES. DSpace@MIT (Massachusetts Institute of Technology). 23 indexed citations
10.
Chiang, Eugene, A. Levine, B. Kalomeni, et al.. (2012). POSSIBLE DISINTEGRATING SHORT-PERIOD SUPER-MERCURY ORBITING KIC 12557548. DSpace@MIT (Massachusetts Institute of Technology). 102 indexed citations
11.
Colberg, J. M., F. R. Pearce, Caroline Foster, et al.. (2008). The Aspen–Amsterdam void finder comparison project. Monthly Notices of the Royal Astronomical Society. 387(2). 933–944. 134 indexed citations
12.
Nelson, L. A., et al.. (2004). On the Properties of Galactic Novae and Their Orbital Period Distribution. The Astrophysical Journal. 602(2). 938–947. 13 indexed citations
13.
Nelson, L. A., et al.. (2004). Evolutionary Properties of Helium‐rich, Degenerate Dwarfs in Binaries Containing Compact Companions. The Astrophysical Journal. 616(2). 1124–1147. 52 indexed citations
14.
Nelson, L. A. & S. Rappaport. (2003). Theoretical Considerations on the Properties of Accreting Millisecond Pulsars. The Astrophysical Journal. 598(1). 431–445. 47 indexed citations
15.
Nelson, L. A., S. Rappaport, & P. C. Joss. (1993). The detectability of brown dwarfs - Predictions and uncertainties. The Astrophysical Journal. 404. 723–723. 10 indexed citations
16.
Lee, Hyung Mok & L. A. Nelson. (1988). Stellar encounters in the Galactic center - Formation of massive stars and close binaries. The Astrophysical Journal. 334. 688–688. 13 indexed citations
17.
Rappaport, S., et al.. (1987). The evolutionary status of 4U 1820-30. The Astrophysical Journal. 322. 842–842. 79 indexed citations
18.
Nelson, L. A., S. Rappaport, & P. C. Joss. (1986). The evolution of very low mass stars. The Astrophysical Journal. 311. 226–226. 25 indexed citations
19.
Nelson, L. A., W. Y. Chau, & Arnold Rosenblum. (1985). Evolution of rotationally and tidally distorted low-mass, close binary systems - Implications for the minimum orbital period of cataclysmic variables. The Astrophysical Journal. 299. 658–658. 9 indexed citations
20.
Chau, W. Y. & L. A. Nelson. (1983). Non-conservative evolution of low-mass, close binaries with gravitational radiation and systemic mass losses. Astrophysics and Space Science. 90(2). 245–260.

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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026