R. C. Smith

27.7k citations
263 papers · 20.0k · 10 hit papers · h-index 73

Impact in

    • Astronomy and Astrophysical Research
    • Galaxies: Formation, Evolution, Phenomena
    • Cosmology and Gravitation Theories
    • Gamma-ray bursts and supernovae
    • Stellar, planetary, and galactic studies
    • Astrophysical Phenomena and Observations

Papers in

    • Galaxies: Formation, Evolution, Phenomena 124
    • Gamma-ray bursts and supernovae 78
    • Stellar, planetary, and galactic studies 53
    • Cosmology and Gravitation Theories 52
    • Astrophysics and Star Formation Studies 21
    • Astrophysical Phenomena and Observations 20
    • Astronomy and Astrophysical Research 77

R. C. Smith

254 papers receiving 19.1k citations

R. C. Smith's Hit Papers

Euclid 2024 · 348 citations
3480+8+17Years since publication4008001.2k

Peers

R. C. Smith
Comparison fields: 5 of 173
  • Instrumentation 4.8k
  • Astronomy and Astrophysics 17.9k
  • Nuclear and High Energy Physics 6.1k
  • Statistical and Nonlinear Physics 740
  • Oceanography 341
Replace Knud Jahnke with:
Knud Jahnke Germany
Masao Sako United States
J.‐L. Puget France
Steven Allen United States
H. R. Butcher United States
Gary Bernstein United States
Andrea Ferrara Italy
Zheng Zheng United States
Andrew W. Howard United States
Matthias R. Schreiber Chile
R. C. Smith relative to Knud Jahnke Germany Knud Jahnke's profile →
Citations per field
00.5×1.5×2.0×
Knud Jahnke · 1×
Citations per year

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-authors

The 25 scholars most cited alongside R. C. Smith, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with R. C. Smith Line = papers co-authored together R. C. Smith links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown

Showing the 20 most-cited of 263 papers — load more, or switch the sort, to bring in the rest.

#Work
1
Stable clustering, the halo model and non-linear cosmological power spectra
Hit paper breakdown →
20031444
2
Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
Hit paper breakdown →
2018911
3
Halo occupation numbers and galaxy bias
Hit paper breakdown →
2000712
4
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
Hit paper breakdown →
2017683
5
Observational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
Hit paper breakdown →
2007586
6
Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
Hit paper breakdown →
2018484
7 1998467
8 2001423
9
EIGHT NEW MILKY WAY COMPANIONS DISCOVERED IN FIRST-YEAR DARK ENERGY SURVEY DATA
Hit paper breakdown →
2015406
10
The James Webb Space Telescope Mission
Hit paper breakdown →
2023404
11 2007381
12
Euclid
Hit paper breakdown →
2024348
13
4MOST: Project overview and information for the First Call for Proposals
Hit paper breakdown →
2019275
14 2016267
15 2013234
16 1978232
17 2010224
18 2012221
19 2002218
20 2018215

About R. C. Smith

R. C. Smith is a scholar working on Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Statistical and Nonlinear Physics and Electrical and Electronic Engineering, having authored 263 papers that have together received 20.0k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (124 papers), Gamma-ray bursts and supernovae (78 papers), Astronomy and Astrophysical Research (77 papers), Stellar, planetary, and galactic studies (53 papers), Cosmology and Gravitation Theories (52 papers), Astrophysics and Cosmic Phenomena (34 papers), Astrophysics and Star Formation Studies (21 papers) and Astrophysical Phenomena and Observations (20 papers). The work is most often cited by research in Instrumentation (4.8k citations), Astronomy and Astrophysics (17.9k citations), Nuclear and High Energy Physics (6.1k citations), Statistical and Nonlinear Physics (740 citations) and Oceanography (341 citations). R. C. Smith has collaborated with scholars based in United States, United Kingdom and Germany. Frequent co-authors include John A. Peacock, Frazer R. Pearce, Uroš Seljak, Tobias Baldauf, Román Scoccimarro, H. M. P. Couchman, Carlos Silvestre Frenk, Adrian R. Jenkins, Simon D. M. White and P. Thomas. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, The Astronomical Journal, The Astrophysical Journal Supplement Series and Physical review. D.

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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