L. Casamiquela
- Instrumentation top 1%
- Astronomy and Astrophysical Research 28
- Astronomy and Astrophysics top 2%
- Stellar, planetary, and galactic studies 37
- Astrophysics and Star Formation Studies 25
- Astro and Planetary Science 9
- Gamma-ray bursts and supernovae 4
- Computational Mechanics top 10%
- Astronomical Observations and Instrumentation 3
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- Chalcogenide Semiconductor Thin Films 1
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- Geomagnetism and Paleomagnetism Studies 1
L. Casamiquela
35 papers receiving 1.3k citations
Hit Papers
Peers
Comparison fields: 5 of 45
- Instrumentation 839
- Astronomy and Astrophysics 1.4k
- Computational Mechanics 70
- Nuclear and High Energy Physics 43
- Spectroscopy 24
Countries citing papers authored by L. Casamiquela
This map shows the geographic impact of L. Casamiquela'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 L. Casamiquela with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. Casamiquela more than expected).
Fields of papers citing papers by L. Casamiquela
This network shows the impact of papers produced by L. Casamiquela. 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 L. Casamiquela. The network helps show where L. Casamiquela may publish in the future.
Co-authorship network
The 25 scholars most cited alongside L. Casamiquela, 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 | 4 | |
| 2 | 2024 | 10 | |
| 3 | 2024 | 6 | |
| 4 | 2023 | 23 | |
| 5 | 2023 | 12 | |
| 6 | 2022 | 6 | |
| 7 | 2022 | 86 | |
| 8 | 2021 | 91 | |
| 9 | 2021 | 11 | |
| 10 | 2021 | 1 | |
| 11 | 2020 | 30 | |
| 12 | Hunting for open clusters in Gaia DR2: 582 new OCs in the Galactic disc | 2020 | 145 |
| 13 | VizieR Online Data Catalog: Portrait Galactic disc (Cantat-Gaudin+, 2020) | 2020 | 1 |
| 14 | Painting a portrait of the Galactic disc with its stellar clustersbreakdown → | 2020 | 333 |
| 15 | 2019 | 57 | |
| 16 | 2019 | 172 | |
| 17 | 2018 | 16 | |
| 18 | 2018 | 125 | |
| 19 | 2016 | 30 | |
| 20 | 2016 | 40 |
About L. Casamiquela
L. Casamiquela is a scholar working on Instrumentation, Astronomy and Astrophysics and Computational Mechanics, having authored 37 papers that have together received 1.5k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (37 papers), Astronomy and Astrophysical Research (28 papers), Astrophysics and Star Formation Studies (25 papers), Astro and Planetary Science (9 papers), Gamma-ray bursts and supernovae (4 papers), Astronomical Observations and Instrumentation (3 papers), Chalcogenide Semiconductor Thin Films (1 paper) and Geomagnetism and Paleomagnetism Studies (1 paper). The work is most often cited by research in Instrumentation (839 citations), Astronomy and Astrophysics (1.4k citations) and Computational Mechanics (70 citations). L. Casamiquela has collaborated with scholars based in Spain, France and Italy. Frequent co-authors include C. Jordi, T. Cantat-Gaudin, C. Soubiran, A. Castro-Ginard, L. Balaguer-Núñez, F. Anders, A. Bragaglia, A. Vallenari, A. Moitinho and R. Carrera. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and The Astronomical 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.