P. Schilke

19.1k total citations · 1 hit paper
214 papers, 8.2k citations indexed

About

P. Schilke is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, P. Schilke has authored 214 papers receiving a total of 8.2k indexed citations (citations by other indexed papers that have themselves been cited), including 193 papers in Astronomy and Astrophysics, 118 papers in Spectroscopy and 56 papers in Atmospheric Science. Recurrent topics in P. Schilke's work include Astrophysics and Star Formation Studies (183 papers), Molecular Spectroscopy and Structure (106 papers) and Stellar, planetary, and galactic studies (84 papers). P. Schilke is often cited by papers focused on Astrophysics and Star Formation Studies (183 papers), Molecular Spectroscopy and Structure (106 papers) and Stellar, planetary, and galactic studies (84 papers). P. Schilke collaborates with scholars based in Germany, United States and France. P. Schilke's co-authors include K. M. Menten, F. Wyrowski, H. Beuther, H. S. P. Müller, C. Comito, D. C. Lis, T. K. Sridharan, C. M. Walmsley, А. Беллоче and T. G. Phillips and has published in prestigious journals such as Nature, Science and The Astrophysical Journal.

In The Last Decade

P. Schilke

206 papers receiving 7.8k citations

Hit Papers

The Cologne Database for ... 2016 2026 2019 2022 2016 100 200 300 400 500

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author Last Decade Papers Cites
P. Schilke 7.0k 4.9k 2.5k 2.0k 249 214 8.2k
Edwin A. Bergin 8.9k 1.3× 4.7k 1.0× 2.5k 1.0× 1.3k 0.7× 196 0.8× 245 9.5k
C. Ceccarelli 7.0k 1.0× 5.7k 1.2× 3.3k 1.3× 3.1k 1.6× 210 0.8× 259 8.4k
D. C. B. Whittet 6.6k 0.9× 2.7k 0.5× 2.0k 0.8× 1.7k 0.9× 146 0.6× 191 7.2k
D. C. Lis 5.5k 0.8× 2.7k 0.6× 1.8k 0.7× 1.3k 0.6× 311 1.2× 194 6.3k
S. Viti 4.3k 0.6× 2.6k 0.5× 1.7k 0.7× 1.5k 0.7× 181 0.7× 229 5.2k
A. C. A. Boogert 5.9k 0.8× 3.4k 0.7× 2.0k 0.8× 1.8k 0.9× 65 0.3× 114 6.4k
E. Roueff 4.1k 0.6× 3.2k 0.7× 2.3k 0.9× 2.8k 1.4× 204 0.8× 238 6.1k
Maryvonne Gérin 3.3k 0.5× 2.2k 0.4× 1.5k 0.6× 1.3k 0.7× 144 0.6× 180 4.1k
J. Stützki 4.4k 0.6× 2.6k 0.5× 1.6k 0.6× 1.1k 0.6× 169 0.7× 187 5.4k
J. K. Jørgensen 7.8k 1.1× 5.3k 1.1× 2.5k 1.0× 1.3k 0.6× 68 0.3× 200 8.2k

Countries citing papers authored by P. Schilke

Since Specialization
Citations

This map shows the geographic impact of P. Schilke'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 P. Schilke with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Schilke more than expected).

Fields of papers citing papers by P. Schilke

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by P. Schilke. 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 P. Schilke. The network helps show where P. Schilke may publish in the future.

Co-authorship network of co-authors of P. Schilke

This figure shows the co-authorship network connecting the top 25 collaborators of P. Schilke. A scholar is included among the top collaborators of P. Schilke 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 P. Schilke. P. Schilke is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Xu, Fengwei, Xing Lu, Hauyu Baobab Liu, et al.. (2025). Dual-band Unified Exploration of three CMZ Clouds (DUET). Astronomy and Astrophysics. 697. A164–A164.
2.
Ginsburg, Adam, Á. Sánchez-Monge, M. Bonfand, et al.. (2024). Thermal Properties of the Hot Core Population in Sagittarius B2 Deep South. The Astrophysical Journal. 962(1). 48–48. 2 indexed citations
3.
Kim, W.-J., J. S. Urquhart, V. S. Veena, et al.. (2023). A survey of SiO J = 1−0 emission toward massive star-forming regions. Astronomy and Astrophysics. 679. A123–A123. 3 indexed citations
4.
Avison, A., G. A. Fuller, S. Etoka, et al.. (2023). Tracing Evolution in Massive Protostellar Objects – I. Fragmentation and emission properties of massive star-forming clumps in a luminosity-limited ALMA sample. Monthly Notices of the Royal Astronomical Society. 526(2). 2278–2300. 4 indexed citations
5.
Kim, W.-J., P. Schilke, David A. Neufeld, et al.. (2022). HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. Astronomy and Astrophysics. 670. A111–A111. 4 indexed citations
6.
Sewiło, M., A. Karska, L. E. Kristensen, et al.. (2022). The Detection of Deuterated Water in the Large Magellanic Cloud with ALMA. The Astrophysical Journal. 933(1). 64–64. 6 indexed citations
7.
Roth, Lorenz, J. Boissier, Arielle Moullet, et al.. (2020). An attempt to detect transient changes in Io’s SO2 and NaCl atmosphere. Icarus. 350. 113925–113925. 17 indexed citations
8.
Louvet, F., F. Motte, P. Hennebelle, et al.. (2014). The W43-MM1 mini-starburst ridge, a test for star formation efficiency models. Springer Link (Chiba Institute of Technology). 36 indexed citations
9.
Rodón, J. A., H. Beuther, & P. Schilke. (2012). Fragmentation in the massive star-forming region IRAS 19410+2336. Springer Link (Chiba Institute of Technology). 4 indexed citations
10.
Rolffs, R., P. Schilke, F. Wyrowski, et al.. (2011). Hot HCN around young massive stars at 0.1′′ resolution. Springer Link (Chiba Institute of Technology). 15 indexed citations
11.
Zapata, Luis A., J. Schmid‐Burgk, D. Muders, et al.. (2010). A rotating molecular jet in Orion. Springer Link (Chiba Institute of Technology). 16 indexed citations
12.
Leurini, S., F. Wyrowski, P. Schilke, et al.. (2010). A study of three southern high-mass star-forming regions. Springer Link (Chiba Institute of Technology). 3 indexed citations
13.
Leurini, S., C. Codella, Luis A. Zapata, et al.. (2009). Extremely high velocity gas from the massive young stellar objects in IRAS 17233-3606. Springer Link (Chiba Institute of Technology). 15 indexed citations
14.
Beuther, H., S. Leurini, P. Schilke, et al.. (2007). Interferometric multi-wavelength (sub)millimeter continuum study of the young high-mass protocluster IRAS 05358+3543. Springer Link (Chiba Institute of Technology). 48 indexed citations
15.
Zapata, Luis A., et al.. (2007). Circumbinary molecular rings around young stars in Orion. Astronomy and Astrophysics. 471(3). L59–L62. 11 indexed citations
16.
Comito, C., P. Schilke, Maryvonne Gérin, et al.. (2003). The line-of-sight distribution of water in the SgrB2 complex. Springer Link (Chiba Institute of Technology). 28 indexed citations
17.
Beuther, H., J. Kerp, T. Preibisch, Thomas Stanke, & P. Schilke. (2002). Hard X-ray emission from a young massive star-forming cluster. Springer Link (Chiba Institute of Technology). 10 indexed citations
18.
Beuther, H., P. Schilke, T. K. Sridharan, et al.. (2002). Massive molecular outflows. Springer Link (Chiba Institute of Technology). 320 indexed citations
19.
Schilke, P., C. M. Walmsley, & R. Mauersberger. (1991). Peculiar 15NH3 toward NGC 7538-IRS1.. A&A. 247. 516. 1 indexed citations
20.
Schilke, P., C. M. Walmsley, T. J. Millar, & C. Henkel. (1991). PROTONATED HCN IN MOLECULAR CLOUDS. Research Portal (Queen's University Belfast). 247(17). 487–496. 13 indexed citations

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.

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