R. C. Smith

25.3k total citations · 2 hit papers
157 papers, 7.0k citations indexed

About

R. C. Smith is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, R. C. Smith has authored 157 papers receiving a total of 7.0k indexed citations (citations by other indexed papers that have themselves been cited), including 104 papers in Astronomy and Astrophysics, 34 papers in Instrumentation and 27 papers in Nuclear and High Energy Physics. Recurrent topics in R. C. Smith's work include Galaxies: Formation, Evolution, Phenomena (58 papers), Astronomy and Astrophysical Research (34 papers) and Cosmology and Gravitation Theories (31 papers). R. C. Smith is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (58 papers), Astronomy and Astrophysical Research (34 papers) and Cosmology and Gravitation Theories (31 papers). R. C. Smith collaborates with scholars based in United States, United Kingdom and Germany. R. C. Smith's co-authors include J. A. Peacock, F. R. Pearce, Uroš Seljak, Tobias Baldauf, Román Scoccimarro, G. Efstathiou, Simon D. M. White, H. M. P. Couchman, Adrian Jenkins and P. Thomas and has published in prestigious journals such as Nature, The Lancet and The Journal of Chemical Physics.

In The Last Decade

R. C. Smith

147 papers receiving 6.8k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Stable clustering, the halo model and non-linear cosmological power spectra

2003 1.2k citations R. C. Smith, J. A. Peacock et al. Monthly Notices of the Royal Astronomical Society profile →
Halo occupation numbers and galaxy bias

2000 632 citations J. A. Peacock, R. C. Smith Monthly Notices of the Royal Astronomical Society profile →

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
R. C. Smith United States	40	5.8k	1.9k	1.6k	414	275	157	7.0k
Xiaohui Fan United States	64	13.6k 2.3×	3.1k 1.6×	4.2k 2.6×	253 0.6×	397 1.4×	345	15.3k
Hsiao‐Wen Chen United States	48	4.9k 0.8×	959 0.5×	1.8k 1.1×	102 0.2×	228 0.8×	179	7.1k
Christian Wolf United Kingdom	38	5.3k 0.9×	556 0.3×	3.0k 1.9×	169 0.4×	163 0.6×	191	5.8k
S. Ortolani Italy	51	7.0k 1.2×	1.9k 1.0×	3.2k 2.0×	64 0.2×	400 1.5×	355	11.1k
Oliver Hahn Germany	37	3.3k 0.6×	1.2k 0.6×	1.3k 0.8×	382 0.9×	59 0.2×	110	4.6k
G. M. Bernstein United States	35	2.6k 0.4×	414 0.2×	904 0.6×	198 0.5×	204 0.7×	99	5.1k
M. Allen United States	39	3.7k 0.6×	1.7k 0.9×	295 0.2×	68 0.2×	189 0.7×	173	6.7k
C. Mendes de Oliveira Brazil	31	2.7k 0.5×	253 0.1×	1.7k 1.0×	161 0.4×	116 0.4×	206	4.4k
Yue Shen United States	37	5.3k 0.9×	1.1k 0.6×	1.4k 0.8×	73 0.2×	164 0.6×	177	5.8k
Shuang‐Nan Zhang China	35	3.9k 0.7×	1.8k 0.9×	132 0.1×	210 0.5×	211 0.8×	383	4.7k

Countries citing papers authored by R. C. Smith

Since Specialization

Citations

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

Fields of papers citing papers by R. C. Smith

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by R. C. 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 R. C. Smith. The network helps show where R. C. Smith may publish in the future.

Co-authorship network of co-authors of R. C. Smith

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

1.

Gastol, Dominika, Jean E. Marshall, Claire E. T. Mitchell, et al.. (2022). Reclaimed and Up‐Cycled Cathodes for Lithium‐Ion Batteries. SHILAP Revista de lepidopterología. 6(12). 2200046–2200046. 25 indexed citations

2.

Winther, Hans A., Fabian Schmidt, Alexandre Barreira, et al.. (2015). Modified gravityN-body code comparison project. Monthly Notices of the Royal Astronomical Society. 454(4). 4208–4234. 93 indexed citations

3.

Peacock, J. A. & R. C. Smith. (2014). HALOFIT: nonlinear distribution of cosmological mass and galaxies. Sussex Research Online (University of Sussex). 5 indexed citations

4.

Smith, R. C.. (2012). How covariant is the galaxy luminosity function?. Monthly Notices of the Royal Astronomical Society. 426(1). 531–548. 15 indexed citations

5.

Cano, Z. & R. C. Smith. (2010). Does the RR Lyrae variable DY And show the Blazhko effect. Observatory. 130(1). 11–16. 1 indexed citations

6.

Smith, R. C., Román Scoccimarro, & Ravi K. Sheth. (2008). Motion of the acoustic peak in the correlation function. Physical review. D. Particles, fields, gravitation, and cosmology. 77(4). 94 indexed citations

7.

Smith, R. C. & Peter Watts. (2005). Triaxial haloes, intrinsic alignments and the dark matter power spectrum. Monthly Notices of the Royal Astronomical Society. 360(1). 203–215. 35 indexed citations

8.

Suntzeff, N. B., et al.. (2001). Supernova 2001M in NGC 3240. IAUC. 7576. 5. 1 indexed citations

9.

Smith, R. C., et al.. (2001). Light curve and physical parameters of the Algol-type binary TW Cas. Observatory. 121. 308–315. 5 indexed citations

10.

Smith, R. C., et al.. (2000). SY Cancri: A hot ligt secondary?. New Astronomy Reviews. 44. 31. 1 indexed citations

11.

Gal‐Yam, A., D. Maoz, Louis-Gregory Strolger, et al.. (1999). Supernovae 1999au, 1999av, 1999aw, 1999ax, 1999ay. IAUC. 7130. 1.

12.

Williams, R., You‐Hua Chu, John R. Dickel, et al.. (1996). DEM L 316: a Pair of Colliding Supernova Remnants. Bulletin of the American Astronomical Society. 188(2). 924.

13.

Smith, R. C., et al.. (1991). Post-partum Anovulation in Nursing Mothers. Journal of Tropical Pediatrics. 37(6). 286–292. 3 indexed citations

14.

Smith, R. C.. (1984). The theory of contact binaries. Quarterly journal of the Royal Astronomical Society. 25(4). 405–420. 1 indexed citations

15.

Smith, R. C. & G. S. West. (1983). Space and Planetary Environment Criteria Guidelines for Use in Space Vehicle Development, 1982 Revision (volume I). 1 indexed citations

16.

Smith, R. C., et al.. (1983). The theoretical spread of the main sequence due to stellar rotation. Observatory. 103. 8–12. 2 indexed citations

17.

Smith, R. C. & G. S. West. (1983). Space and planetary environment criteria guidelines for use in space vehicle development. Volume 1: 1982 revision. NASA STI/Recon Technical Report N. 83. 18816. 23 indexed citations

18.

Smith, R. C.. (1983). An empirical stellar mass-luminosity relationship. Observatory. 103. 29–31. 18 indexed citations

19.

Clark, D. H., P. J. Andrews, & R. C. Smith. (1981). Are we overdue for a galactic supernova. Observatory. 101. 203–205. 1 indexed citations

20.

Smith, R. C., et al.. (1971). Hepatoma in a Bengal Tiger. Journal of the American Veterinary Medical Association. 159(5). 617–619. 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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