P. D. Barthel

4.8k total citations · 1 hit paper
101 papers, 2.1k citations indexed

About

P. D. Barthel is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, P. D. Barthel has authored 101 papers receiving a total of 2.1k indexed citations (citations by other indexed papers that have themselves been cited), including 94 papers in Astronomy and Astrophysics, 56 papers in Nuclear and High Energy Physics and 20 papers in Instrumentation. Recurrent topics in P. D. Barthel's work include Galaxies: Formation, Evolution, Phenomena (73 papers), Astrophysics and Cosmic Phenomena (56 papers) and Radio Astronomy Observations and Technology (47 papers). P. D. Barthel is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (73 papers), Astrophysics and Cosmic Phenomena (56 papers) and Radio Astronomy Observations and Technology (47 papers). P. D. Barthel collaborates with scholars based in Netherlands, United States and United Kingdom. P. D. Barthel's co-authors include C. L. Carilli, G. K. Miley, C. P. O’Dea, M. Filho, Stefi A. Baum, K. A. Arnaud, W. H. de Vries, C. P. O’Dea, Á. Labiano and C. J. Lonsdale and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

P. D. Barthel

98 papers receiving 2.0k citations

Hit Papers

Is every quasar beamed? 1989 2026 2001 2013 1989 100 200 300 400

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
P. D. Barthel Netherlands 26 2.0k 1.2k 245 44 36 101 2.1k
D. J. Saikia India 26 2.1k 1.0× 1.4k 1.1× 187 0.8× 44 1.0× 47 1.3× 167 2.2k
S. Giacintucci United States 29 2.5k 1.2× 1.4k 1.1× 366 1.5× 37 0.8× 67 1.9× 103 2.5k
J. J. Condon United States 20 1.6k 0.8× 855 0.7× 240 1.0× 29 0.7× 48 1.3× 71 1.7k
M. Villar-Martı́n Spain 26 1.9k 0.9× 586 0.5× 506 2.1× 21 0.5× 28 0.8× 99 2.0k
S. T. Myers United States 16 1.1k 0.6× 530 0.4× 155 0.6× 30 0.7× 70 1.9× 40 1.2k
Preeti Kharb India 23 1.5k 0.8× 894 0.7× 196 0.8× 25 0.6× 21 0.6× 100 1.6k
O. González-Martín Spain 24 1.8k 0.9× 524 0.4× 258 1.1× 13 0.3× 52 1.4× 94 1.8k
W. J. M. van Breugel United States 26 2.5k 1.2× 1.1k 0.8× 602 2.5× 23 0.5× 27 0.8× 45 2.6k
S. F. Hönig Germany 29 2.7k 1.3× 615 0.5× 354 1.4× 14 0.3× 76 2.1× 67 2.7k
T. J. Balonek United States 18 1.0k 0.5× 490 0.4× 155 0.6× 33 0.8× 32 0.9× 43 1.1k

Countries citing papers authored by P. D. Barthel

Since Specialization
Citations

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

Fields of papers citing papers by P. D. Barthel

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of P. D. Barthel

This figure shows the co-authorship network connecting the top 25 collaborators of P. D. Barthel. A scholar is included among the top collaborators of P. D. Barthel 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. D. Barthel. P. D. Barthel 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.
Andernach, H., et al.. (2024). Giant radio galaxies in the LOFAR deep fields. Astronomy and Astrophysics. 686. A21–A21. 5 indexed citations
2.
Chiaberge, M., Erini Lambrides, Eileen T. Meyer, et al.. (2024). Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages. The Astrophysical Journal. 963(2). 91–91. 9 indexed citations
3.
Azadi, Mojegan, B. J. Wilkes, Joanna Kuraszkiewicz, et al.. (2023). Disentangling the AGN and Star formation Contributions to the Radio–X-Ray Emission of Radio-loud Quasars at 1 < Z < 2. The Astrophysical Journal. 945(2). 145–145. 8 indexed citations
4.
Morganti, R., Frits Sweijen, L. K. Morabito, et al.. (2023). Nuclear regions as seen with LOFAR international baselines. Astronomy and Astrophysics. 682. A118–A118. 5 indexed citations
5.
Radcliffe, J. F., P. D. Barthel, A. P. Thomson, et al.. (2021). Nowhere to hide: Radio-faint AGN in the GOODS-N field. Astronomy and Astrophysics. 649. A27–A27. 12 indexed citations
6.
Kuraszkiewicz, Joanna, B. J. Wilkes, Johannes Büchner, et al.. (2021). Beyond Simple AGN Unification with Chandra-observed 3CRR Sources at 0.5 < z < 1. The Astrophysical Journal. 913(2). 134–134. 11 indexed citations
7.
Peletier, R. F., et al.. (2020). Infrared-detected AGNs in the local Universe. Astronomy and Astrophysics. 640. A68–A68. 3 indexed citations
8.
Shulevski, A., P. D. Barthel, R. Morganti, et al.. (2019). Open Research Online (The Open University). 9 indexed citations
9.
Drouart, G., C. De Breuck, J. Vernet, et al.. (2014). Rapidly growing black holes and host galaxies in the distant Universe from theHerschelRadio Galaxy Evolution Project. Astronomy and Astrophysics. 566. A53–A53. 66 indexed citations
10.
Hocuk, S. & P. D. Barthel. (2010). The asymmetric radio structure and record jet of giant quasar 4C 34.47. Springer Link (Chiba Institute of Technology). 16 indexed citations
11.
White, G. J., C. P. Pearson, Róbert Braun, et al.. (2010). A deep survey of the AKARI north ecliptic pole field. Astronomy and Astrophysics. 517. A54–A54. 12 indexed citations
12.
Barthel, P. D., et al.. (2009). Dust tori in radio galaxies. Astronomy and Astrophysics. 511. A64–A64. 28 indexed citations
13.
Papadopoulos, P. P., A. Kovács, A. Evans, & P. D. Barthel. (2008). High-excitation molecular gas in local luminous AGN hosts. Springer Link (Chiba Institute of Technology). 23 indexed citations
14.
Barthel, P. D.. (2006). Star-forming QSO host galaxies. Springer Link (Chiba Institute of Technology). 14 indexed citations
15.
Labiano, Á., R. C. Vermeulen, P. D. Barthel, et al.. (2006). H I absorption in 3C 49 and 3C 268.3. Astronomy and Astrophysics. 447(2). 481–487. 26 indexed citations
16.
Vermeulen, R. C., Y. M. Pihlström, W. H. de Vries, et al.. (2003). Observations of H I absorbing gas in compact radio sources at cosmological redshifts. Astronomy and Astrophysics. 404(3). 861–870. 97 indexed citations
17.
Barthel, P. D., David Tytler, & Blake Thomson. (1990). Optical spectra of distant radio loud quasars. I. Data: spectra of 67 quasars. Astronomy & Astrophysics Supplement Series. 82(2). 339–389. 1 indexed citations
18.
Barthel, P. D.. (1989). Is every quasar beamed?. The Astrophysical Journal. 336. 606–606. 402 indexed citations breakdown →
19.
Barthel, P. D., G. K. Miley, R. T. Schilizzi, & C. J. Lonsdale. (1988). Observations of the large scale radio structure in high redshift quasars. Leiden Repository (Leiden University). 73(3). 515–547. 4 indexed citations
20.
Lonsdale, C. J. & P. D. Barthel. (1987). Radio sources with strong jets and weak cores. The Astronomical Journal. 94. 1487–1487. 2 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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