Y. M. Pihlström
- Astronomy and Astrophysics top 2%
- Astrophysics and Star Formation Studies 38
- Stellar, planetary, and galactic studies 26
- Galaxies: Formation, Evolution, Phenomena 21
- Astrophysical Phenomena and Observations 12
- Radio Astronomy Observations and Technology 9
- Gamma-ray bursts and supernovae 6
-
- Astrophysics and Cosmic Phenomena 17
- Instrumentation top 10%
- Astronomy and Astrophysical Research 11
- Spectroscopy top 10%
- Co-authors
- Loránt O. SjouwermanG. B. TaylorJ. E. ConwayS. J. CurranJohn K. WebbVincent L. FishR. C. VermeulenM. T. Murphy
- Partner nations
- United StatesNetherlandsSweden
In The Last Decade
Y. M. Pihlström
51 papers receiving 1.0k citations
Peers
Comparison fields: 5 of 33
- Astronomy and Astrophysics 1.0k
- Nuclear and High Energy Physics 426
- Instrumentation 66
- Spectroscopy 123
- Aerospace Engineering 72
Countries citing papers authored by Y. M. Pihlström
This map shows the geographic impact of Y. M. Pihlström'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 Y. M. Pihlström with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Y. M. Pihlström more than expected).
Fields of papers citing papers by Y. M. Pihlström
This network shows the impact of papers produced by Y. M. Pihlström. 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 Y. M. Pihlström. The network helps show where Y. M. Pihlström may publish in the future.
Co-authorship network
The 25 scholars most cited alongside Y. M. Pihlström, 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 | 2024 | 2 | |
| 2 | 2024 | 1 | |
| 3 | 2024 | 2 | |
| 4 | 2023 | 2 | |
| 5 | 2022 | 0 | |
| 6 | 2022 | 0 | |
| 7 | 2020 | 3 | |
| 8 | 2017 | 0 | |
| 9 | 2017 | 1 | |
| 10 | 2011 | 18 | |
| 11 | 2010 | 11 | |
| 12 | 2009 | 81 | |
| 13 | 2009 | 44 | |
| 14 | 2007 | 39 | |
| 15 | Exploring the Last Electromagnetic Frontier with the Long Wavelength Array (LWA) | 2006 | 1 |
| 16 | 2004 | 34 | |
| 17 | 2003 | 64 | |
| 18 | 2003 | 97 | |
| 19 | Radio Studies of Circumnuclear Gas in Active Galaxies | 2001 | 1 |
| 20 | 2001 | 43 |
About Y. M. Pihlström
Y. M. Pihlström is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 59 papers that have together received 1.1k indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (38 papers), Stellar, planetary, and galactic studies (26 papers), Galaxies: Formation, Evolution, Phenomena (21 papers), Astrophysics and Cosmic Phenomena (17 papers), Astrophysical Phenomena and Observations (12 papers), Astronomy and Astrophysical Research (11 papers), Radio Astronomy Observations and Technology (9 papers) and Gamma-ray bursts and supernovae (6 papers). The work is most often cited by research in Astronomy and Astrophysics (1.0k citations), Nuclear and High Energy Physics (426 citations) and Instrumentation (66 citations). Y. M. Pihlström has collaborated with scholars based in United States, Netherlands and Sweden. Frequent co-authors include Loránt O. Sjouwerman, G. B. Taylor, J. E. Conway, S. J. Curran, John K. Webb, Vincent L. Fish, R. C. Vermeulen, M. T. Murphy, M. J. Claussen and Steven W. Ellingson.
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.