M. L. N. Ashby
- Instrumentation top 0.5%
- Astronomy and Astrophysical Research 60
- Astronomy and Astrophysics top 0.5%
- Galaxies: Formation, Evolution, Phenomena 106
- Astrophysics and Star Formation Studies 48
- Stellar, planetary, and galactic studies 48
- Gamma-ray bursts and supernovae 35
- Astrophysical Phenomena and Observations 23
- Radio Astronomy Observations and Technology 13
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- Astrophysics and Cosmic Phenomena 15
- Atmospheric Science top 10%
- Spectroscopy top 5%
- Co-authors
- S. P. WillnerG. G. FazioM. A. PahreP. BarmbyJiasheng HuangM. BrodwinPeter EisenhardtDaniel Stern
- Partner nations
- United StatesUnited KingdomFrance
In The Last Decade
M. L. N. Ashby
127 papers receiving 4.1k citations
Hit Papers
Peers
Comparison fields: 5 of 84
- Instrumentation 1.6k
- Astronomy and Astrophysics 4.1k
- Nuclear and High Energy Physics 632
- Atmospheric Science 203
- Spectroscopy 189
Countries citing papers authored by M. L. N. Ashby
This map shows the geographic impact of M. L. N. Ashby'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 M. L. N. Ashby with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. L. N. Ashby more than expected).
Fields of papers citing papers by M. L. N. Ashby
This network shows the impact of papers produced by M. L. N. Ashby. 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 M. L. N. Ashby. The network helps show where M. L. N. Ashby may publish in the future.
Co-authorship network
The 25 scholars most cited alongside M. L. N. Ashby, 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 | 1 | |
| 2 | 2024 | 1 | |
| 3 | 2024 | 0 | |
| 4 | 2023 | 8 | |
| 5 | 2023 | 1 | |
| 6 | 2023 | 2 | |
| 7 | 2022 | 5 | |
| 8 | 2021 | 3 | |
| 9 | 2021 | 11 | |
| 10 | 2021 | 11 | |
| 11 | A Census of Galaxy Constituents in a Coma Progenitor Observed at z > 3 | 2019 | 13 |
| 12 | 2019 | 10 | |
| 13 | 2019 | 9 | |
| 14 | 2018 | 17 | |
| 15 | 2018 | 17 | |
| 16 | 2017 | 99 | |
| 17 | 2016 | 25 | |
| 18 | 2016 | 81 | |
| 19 | 2015 | 90 | |
| 20 | <i>S</i>pitzer IRAC Infrared Colours of Submillimetre-Bright Galaxies | 2008 | 22 |
About M. L. N. Ashby
M. L. N. Ashby is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 136 papers that have together received 4.3k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (106 papers), Astronomy and Astrophysical Research (60 papers), Astrophysics and Star Formation Studies (48 papers), Stellar, planetary, and galactic studies (48 papers), Gamma-ray bursts and supernovae (35 papers), Astrophysical Phenomena and Observations (23 papers), Astrophysics and Cosmic Phenomena (15 papers) and Radio Astronomy Observations and Technology (13 papers). The work is most often cited by research in Instrumentation (1.6k citations), Astronomy and Astrophysics (4.1k citations) and Nuclear and High Energy Physics (632 citations). M. L. N. Ashby has collaborated with scholars based in United States, United Kingdom and France. Frequent co-authors include S. P. Willner, G. G. Fazio, M. A. Pahre, P. Barmby, Jiasheng Huang, M. Brodwin, Peter Eisenhardt, Daniel Stern, Anton M. Koekemoer and A. Zezas. Their work appears in journals such as Nature, Nature Communications and The Astrophysical Journal.
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.