M. Schöller
- Instrumentation top 2%
- Astronomy and Astrophysical Research 38
- Astronomy and Astrophysics top 1%
- Stellar, planetary, and galactic studies 106
- Astrophysics and Star Formation Studies 95
- Astro and Planetary Science 51
- Astrophysical Phenomena and Observations 13
- Solar and Space Plasma Dynamics 9
- Computational Mechanics top 10%
- Astronomical Observations and Instrumentation 8
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- Adaptive optics and wavefront sensing 7
M. Schöller
124 papers receiving 2.1k citations
Peers
Comparison fields: 5 of 74
- Instrumentation 481
- Astronomy and Astrophysics 2.0k
- Computational Mechanics 128
- Nuclear and High Energy Physics 68
- Spectroscopy 53
Countries citing papers authored by M. Schöller
This map shows the geographic impact of M. Schöller'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. Schöller with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Schöller more than expected).
Fields of papers citing papers by M. Schöller
This network shows the impact of papers produced by M. Schöller. 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. Schöller. The network helps show where M. Schöller may publish in the future.
Co-authorship network
The 25 scholars most cited alongside M. Schöller, 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 | 2025 | 0 | |
| 3 | 2024 | 0 | |
| 4 | 2024 | 0 | |
| 5 | 2022 | 1 | |
| 6 | 2020 | 2 | |
| 7 | 2020 | 0 | |
| 8 | 2019 | 15 | |
| 9 | 2019 | 12 | |
| 10 | 2018 | 5 | |
| 11 | 2018 | 7 | |
| 12 | 2016 | 12 | |
| 13 | 2014 | 22 | |
| 14 | The strong magnetic field of the large-amplitude β-Cephei pulsator V1449 Aql | 2011 | 15 |
| 15 | 2011 | 47 | |
| 16 | 2009 | 63 | |
| 17 | 2008 | 17 | |
| 18 | MIDI combines light from the VLTI: the start of 10 μm interferometry at ESO | 2003 | 5 |
| 19 | The VLTI Data Flow System: from observation preparation to data processing | 2001 | 0 |
| 20 | 1994 | 2 |
About M. Schöller
M. Schöller is a scholar working on Instrumentation, Astronomy and Astrophysics, Periodontics, Computational Mechanics and Atomic and Molecular Physics, and Optics, having authored 131 papers that have together received 2.2k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (106 papers), Astrophysics and Star Formation Studies (95 papers), Astro and Planetary Science (51 papers), Astronomy and Astrophysical Research (38 papers), Astrophysical Phenomena and Observations (13 papers), Solar and Space Plasma Dynamics (9 papers), Astronomical Observations and Instrumentation (8 papers) and Adaptive optics and wavefront sensing (7 papers). The work is most often cited by research in Instrumentation (481 citations), Astronomy and Astrophysics (2.0k citations), Computational Mechanics (128 citations), Nuclear and High Energy Physics (68 citations) and Spectroscopy (53 citations). M. Schöller has collaborated with scholars based in Germany, Chile and Russia. Frequent co-authors include S. Hubrig, I. Ilyin, M. Briquet, G. Mathys, R. V. Yudin, J. F. González, M. A. Pogodin, S. P. Järvinen, P. De Cat and N. Langer. Their work appears in journals such as Astronomy and Astrophysics, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society Letters, Microbiology 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.