Fabian Walter
About
In The Last Decade
Fabian Walter
354 papers receiving 16.6k citations
Hit Papers
Peers
Comparison fields: 5 of 110
- Astronomy and Astrophysics 16.9k
- Instrumentation 4.4k
- Nuclear and High Energy Physics 2.5k
- Spectroscopy 650
- Atomic and Molecular Physics, and Optics 411
Countries citing papers authored by Fabian Walter
This map shows the geographic impact of Fabian Walter'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 Fabian Walter with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Fabian Walter more than expected).
Fields of papers citing papers by Fabian Walter
This network shows the impact of papers produced by Fabian Walter. 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 Fabian Walter. The network helps show where Fabian Walter may publish in the future.
Co-authorship network of co-authors of Fabian Walter
This figure shows the co-authorship network connecting the top 25 collaborators of Fabian Walter. A scholar is included among the top collaborators of Fabian Walter based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Fabian Walter. Fabian Walter is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 1 | |
| 3 | 3 | |
| 4 | 8 | |
| 5 | 4 | |
| 6 | 11 | |
| 7 | 13 | |
| 8 | Detecting and Characterizing Young Quasars. I. Systemic Redshifts and Proximity Zone Measurements | 12 |
| 9 | 5 | |
| 10 | 28 | |
| 11 | 25 | |
| 12 | Cold Gas Outflows, Feedback, and the Shaping of Galaxies | 1 |
| 13 | COLDz: shape of the CO luminosity function at high redshift sand the cold gas history of the universe | 32 |
| 14 | Predicting Quasar Continua near Lyα with Principal Component Analysis | 45 |
| 15 | Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z 2.5 Submillimeter Galaxies | 71 |
| 16 | ALMA spectroscopic survey in the Hubble ultra deep field: survey description | 58 |
| 17 | 13 | |
| 18 | 92 | |
| 19 | 42 | |
| 20 | 1 |
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.