A. M. S. Smith

8.4k total citations
54 papers, 1.2k citations indexed

About

A. M. S. Smith is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, A. M. S. Smith has authored 54 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 52 papers in Astronomy and Astrophysics, 19 papers in Instrumentation and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in A. M. S. Smith's work include Stellar, planetary, and galactic studies (48 papers), Astrophysics and Star Formation Studies (33 papers) and Astro and Planetary Science (33 papers). A. M. S. Smith is often cited by papers focused on Stellar, planetary, and galactic studies (48 papers), Astrophysics and Star Formation Studies (33 papers) and Astro and Planetary Science (33 papers). A. M. S. Smith collaborates with scholars based in United Kingdom, United States and Switzerland. A. M. S. Smith's co-authors include D. R. Anderson, A. Collier Cameron, C. Hellier, M. Gillon, D. Queloz, A. H. M. J. Triaud, P. F. L. Maxted, B. Smalley, R. G. West and S. Udry and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

A. M. S. Smith

52 papers receiving 1.1k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
A. M. S. Smith United Kingdom 22 1.1k 500 132 71 66 54 1.2k
F. Murgas Spain 19 876 0.8× 377 0.8× 102 0.8× 74 1.0× 50 0.8× 56 927
M. Lendl Switzerland 26 1.6k 1.5× 646 1.3× 176 1.3× 94 1.3× 83 1.3× 78 1.7k
Everett Schlawin United States 16 798 0.7× 310 0.6× 125 0.9× 57 0.8× 69 1.0× 41 892
A. S. Bonomo Italy 20 1.1k 0.9× 342 0.7× 96 0.7× 84 1.2× 34 0.5× 49 1.1k
P. Rojo Chile 18 805 0.7× 306 0.6× 86 0.7× 46 0.6× 43 0.7× 63 862
X. Delfosse France 16 1.3k 1.1× 482 1.0× 111 0.8× 71 1.0× 42 0.6× 20 1.3k
L. Delrez Belgium 16 907 0.8× 313 0.6× 152 1.2× 87 1.2× 52 0.8× 34 950
S. C. Marsden Australia 31 2.8k 2.5× 388 0.8× 110 0.8× 45 0.6× 75 1.1× 96 2.9k
Natalie M. Batalha United States 21 1.8k 1.6× 564 1.1× 87 0.7× 64 0.9× 81 1.2× 62 1.9k
Jessie L. Christiansen United States 21 1.2k 1.0× 444 0.9× 62 0.5× 35 0.5× 58 0.9× 70 1.2k

Countries citing papers authored by A. M. S. Smith

Since Specialization
Citations

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

Fields of papers citing papers by A. M. S. Smith

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by A. M. S. Smith. 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 A. M. S. Smith. The network helps show where A. M. S. Smith may publish in the future.

Co-authorship network of co-authors of A. M. S. Smith

This figure shows the co-authorship network connecting the top 25 collaborators of A. M. S. Smith. A scholar is included among the top collaborators of A. M. S. Smith 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 A. M. S. Smith. A. M. S. Smith 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.
Csizmadia, Sz., et al.. (2025). Characterising WASP-43b’s interior structure: Unveiling tidal decay and apsidal motion. Astronomy and Astrophysics. 694. A233–A233. 2 indexed citations
2.
Csizmadia, Sz., A. M. S. Smith, H. Rauer, et al.. (2024). Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system. Astronomy and Astrophysics. 684. A78–A78. 8 indexed citations
3.
Guenther, E. W., Elisa Goffo, Daniel Sebastian, et al.. (2024). A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c. Monthly Notices of the Royal Astronomical Society. 529(1). 141–154. 1 indexed citations
4.
Smith, A. M. S., et al.. (2023). The Orbit of Warm Jupiter WASP-106 b is Aligned with its Star. The Astronomical Journal. 166(4). 159–159. 5 indexed citations
5.
Wunderlich, Fabian, M. Godolt, John Lee Grenfell, et al.. (2019). Detectability of atmospheric features of Earth-like planets in the habitable zone around M dwarfs. Astronomy and Astrophysics. 624. A49–A49. 74 indexed citations
6.
Samadi, R., D. R. Reese, Emmanuel Grolleau, et al.. (2019). The PLATO Solar-like Light-curve Simulator. Astronomy and Astrophysics. 624. A117–A117. 12 indexed citations
7.
Greaves, J. S., A. Scaife, D. T. Frayer, et al.. (2018). Anomalous microwave emission from spinning nanodiamonds around stars. Nature Astronomy. 2(8). 662–667. 19 indexed citations
8.
Anderson, D. R., A. Collier Cameron, L. Delrez, et al.. (2017). The discoveries of WASP-91b, WASP-105b and WASP-107b: Two warm Jupiters and a planet in the transition region between ice giants and gas giants. Astronomy and Astrophysics. 604. A110–A110. 46 indexed citations
9.
Maxted, P. F. L., D. R. Anderson, A. Collier Cameron, et al.. (2016). Five transiting hot Jupiters discovered using WASP-South,Euler, and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b, and WASP-133 b. Astronomy and Astrophysics. 591. A55–A55. 19 indexed citations
10.
Essen, C. von, M. Mallonn, Simon Albrecht, et al.. (2015). A temperature inversion in WASP-33b?. Astronomy and Astrophysics. 584. A75–A75. 9 indexed citations
11.
Lendl, M., A. H. M. J. Triaud, D. R. Anderson, et al.. (2014). WASP-117b: a 10-day-period Saturn in an eccentric and misaligned orbit. Springer Link (Chiba Institute of Technology). 24 indexed citations
12.
Neveu-VanMalle, M., D. Queloz, D. R. Anderson, et al.. (2014). WASP-94 A and B planets: hot-Jupiter cousins in a twin-star system. Springer Link (Chiba Institute of Technology). 16 indexed citations
13.
Smith, A. M. S.. (2014). The SuperWASP exoplanet transit survey. 43(3). 500–512. 2 indexed citations
14.
Gillon, M., D. R. Anderson, A. Collier Cameron, et al.. (2014). WASP-103 b: a new planet at the edge of tidal disruption. Astronomy and Astrophysics. 562. L3–L3. 53 indexed citations
15.
Anderson, D. R., A. Collier Cameron, C. Hellier, et al.. (2014). WASP-20b and WASP-28b: a hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars. Astronomy and Astrophysics. 575. A61–A61. 26 indexed citations
16.
Beasley, Matthew, et al.. (2013). AsteroidZoo: A New Zooniverse project to detect asteroids and improve asteroid detection algorithms. AGU Fall Meeting Abstracts. 2013. 3 indexed citations
17.
Smalley, B., D. R. Anderson, A. Collier Cameron, et al.. (2012). WASP-78b and WASP-79b: two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus. Springer Link (Chiba Institute of Technology). 17 indexed citations
18.
Lendl, M., D. R. Anderson, A. Collier Cameron, et al.. (2012). WASP-42 b and WASP-49 b: two new transiting sub-Jupiters. Springer Link (Chiba Institute of Technology). 33 indexed citations
19.
Enoch, B., C. A. Haswell, A. J. Norton, et al.. (2012). Transit algorithm performance using real WASP data. Astronomy and Astrophysics. 548. A48–A48. 2 indexed citations
20.
Anderson, D. R., A. Collier Cameron, M. Gillon, et al.. (2011). WASP-43b: the closest-orbiting hot Jupiter. Springer Link (Chiba Institute of Technology). 53 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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