K. Smith
- Astronomy and Astrophysics top 2%
- Gamma-ray bursts and supernovae 26
- Stellar, planetary, and galactic studies 13
- Astro and Planetary Science 10
- Pulsars and Gravitational Waves Research 8
- Astrophysical Phenomena and Observations 7
- Instrumentation top 5%
- Astronomy and Astrophysical Research 6
- Nuclear and High Energy Physics top 10%
- Computational Mechanics top 10%
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- graph theory and CDMA systems 16
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- Coding theory and cryptography 13
K. Smith
62 papers receiving 1.2k citations
Hit Papers
Peers
Comparison fields: 5 of 91
- Astronomy and Astrophysics 1.0k
- Instrumentation 205
- Nuclear and High Energy Physics 229
- Discrete Mathematics and Combinatorics 35
- Computational Mechanics 80
Countries citing papers authored by K. Smith
This map shows the geographic impact of K. 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 K. Smith with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. Smith more than expected).
Fields of papers citing papers by K. Smith
This network shows the impact of papers produced by K. 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 K. Smith. The network helps show where K. Smith may publish in the future.
Co-authorship network
The 25 scholars most cited alongside K. Smith, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2025 | 0 | |
| 2 | 2025 | 0 | |
| 3 | 2025 | 0 | |
| 4 | 2025 | 3 | |
| 5 | 2024 | 4 | |
| 6 | 2024 | 3 | |
| 7 | 2024 | 5 | |
| 8 | 2024 | 5 | |
| 9 | 2024 | 1 | |
| 10 | 2024 | 1 | |
| 11 | 2023 | 12 | |
| 12 | 2023 | 7 | |
| 13 | 2021 | 3 | |
| 14 | 2018 | 13 | |
| 15 | 2017 | 30 | |
| 16 | 2013 | 13 | |
| 17 | Supernova 2013L in ESO 216-39 = Psn J11452955-5035531 | 2013 | 2 |
| 18 | First observations of the reappearance of SN 2009ip with PESSTO | 2013 | 1 |
| 19 | 2012 | 6 | |
| 20 | Discovery two new supernovae in the Pan-STARRS1 3Pi faint galaxy supernova survey | 2010 | 1 |
About K. Smith
K. Smith is a scholar working on Discrete Mathematics and Combinatorics, Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics and Artificial Intelligence, having authored 73 papers that have together received 1.4k indexed citations. Recurring topics across this work include Gamma-ray bursts and supernovae (26 papers), graph theory and CDMA systems (16 papers), Coding theory and cryptography (13 papers), Stellar, planetary, and galactic studies (13 papers), Astro and Planetary Science (10 papers), Pulsars and Gravitational Waves Research (8 papers), Astrophysical Phenomena and Observations (7 papers) and Astronomy and Astrophysical Research (6 papers). The work is most often cited by research in Astronomy and Astrophysics (1.0k citations), Instrumentation (205 citations), Nuclear and High Energy Physics (229 citations), Discrete Mathematics and Combinatorics (35 citations) and Computational Mechanics (80 citations). K. Smith has collaborated with scholars based in United States, United Kingdom and Australia. Frequent co-authors include S. J. Smartt, A. Rest, J. Tonry, L. Denneau, B. Stalder, H. Weiland, A. Heinze, C. W. Stubbs, H. Flewelling and D. R. Young. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, Journal of Combinatorial Theory Series A, The Planetary Science Journal, The Electronic Journal of Combinatorics and The Astrophysical Journal Letters.
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.