Klaus Bernhard

1.3k total citations
53 papers, 874 citations indexed

About

Klaus Bernhard is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, Klaus Bernhard has authored 53 papers receiving a total of 874 indexed citations (citations by other indexed papers that have themselves been cited), including 39 papers in Astronomy and Astrophysics, 19 papers in Instrumentation and 6 papers in Computational Mechanics. Recurrent topics in Klaus Bernhard's work include Stellar, planetary, and galactic studies (38 papers), Astrophysics and Star Formation Studies (29 papers) and Astronomy and Astrophysical Research (19 papers). Klaus Bernhard is often cited by papers focused on Stellar, planetary, and galactic studies (38 papers), Astrophysics and Star Formation Studies (29 papers) and Astronomy and Astrophysical Research (19 papers). Klaus Bernhard collaborates with scholars based in United States, Czechia and Slovakia. Klaus Bernhard's co-authors include Stefan Hümmerich, E. Paunzen, Steen Steenken, Massimo Bietti, Slobodan V. Jovanović, Liang Tong, Jeffrey B. Madwed, Pier F. Cirillo, Alan Swinamer and John R. Regan and has published in prestigious journals such as Journal of the American Chemical Society, Monthly Notices of the Royal Astronomical Society and Journal of Medicinal Chemistry.

In The Last Decade

Klaus Bernhard

50 papers receiving 823 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Klaus Bernhard United States 12 373 297 240 134 86 53 874
Thomas L. Jacobs United States 20 91 0.2× 446 1.5× 419 1.7× 133 1.0× 14 0.2× 78 1.0k
Richard M. West United Kingdom 11 135 0.4× 63 0.2× 87 0.4× 15 0.1× 31 0.4× 29 488
Ricardo Gobato United States 26 247 0.7× 14 0.0× 123 0.5× 6 0.0× 518 6.0× 82 1.6k
John Harrison United States 19 538 1.4× 266 0.9× 29 0.1× 49 0.4× 41 0.5× 50 1.1k
Ágnes Gömöry Hungary 17 261 0.7× 16 0.1× 493 2.1× 2 0.0× 67 0.8× 97 995
Jinru Wang China 20 748 2.0× 56 0.2× 465 1.9× 170 2.0× 54 1.5k
Duxi Zhang United States 14 287 0.8× 46 0.2× 79 0.3× 39 0.5× 20 1.0k
Saidul Islam United Kingdom 15 557 1.5× 428 1.4× 364 1.5× 44 0.5× 24 1.0k
Ning Su United States 15 295 0.8× 37 0.1× 117 0.5× 75 0.9× 34 968
Shengwei Wei Germany 16 487 1.3× 299 1.0× 689 2.9× 30 0.3× 22 1.3k

Countries citing papers authored by Klaus Bernhard

Since Specialization
Citations

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

Fields of papers citing papers by Klaus Bernhard

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Klaus Bernhard

This figure shows the co-authorship network connecting the top 25 collaborators of Klaus Bernhard. A scholar is included among the top collaborators of Klaus Bernhard 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 Klaus Bernhard. Klaus Bernhard 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.
Hümmerich, Stefan, Klaus Bernhard, & E. Paunzen. (2024). A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey. Astronomy and Astrophysics. 692. A231–A231. 1 indexed citations
2.
Uttenthaler, S., S. Shetye, A. Nanni, et al.. (2024). The impact of third dredge-up on the mass loss of Mira variables. Astronomy and Astrophysics. 690. A393–A393. 3 indexed citations
3.
Paunzen, E., et al.. (2024). Chemically peculiar stars on the pre-main sequence. Astronomy and Astrophysics. 687. A176–A176. 1 indexed citations
4.
Bernhard, Klaus, et al.. (2024). New ACV variables discovered in the Zwicky Transient Facility survey. Astronomy and Astrophysics. 687. A211–A211. 2 indexed citations
5.
Bernhard, Klaus, et al.. (2023). High-velocity CP2 stars in the Galactic halo. Astronomy and Astrophysics. 674. A215–A215. 2 indexed citations
6.
Labadie-Bartz, Jonathan, Stefan Hümmerich, Klaus Bernhard, E. Paunzen, & M. E. Shultz. (2023). Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS. Astronomy and Astrophysics. 676. A55–A55. 8 indexed citations
7.
Mikulášek, Zdeněk, Е. А. Семенко, E. Paunzen, et al.. (2022). HD 60431, the CP2 star with the shortest rotational period. Astronomy and Astrophysics. 668. A159–A159. 6 indexed citations
8.
Xia, Changlei, et al.. (2021). A case study of ACV variables discovered in the Zwicky Transient Facility survey. arXiv (Cornell University). 9 indexed citations
9.
Paunzen, E., et al.. (2020). Pulsational properties of ten new slowly pulsating B stars. Springer Link (Chiba Institute of Technology). 8 indexed citations
10.
Hümmerich, Stefan, E. Paunzen, & Klaus Bernhard. (2020). A plethora of new, magnetic chemically peculiar stars from LAMOST DR4. Springer Link (Chiba Institute of Technology). 26 indexed citations
11.
Uttenthaler, S., Iain McDonald, Klaus Bernhard, S. Cristallo, & D. Gobrecht. (2019). Interplay between pulsation, mass loss, and third dredge-up: More about Miras with and without technetium. Springer Link (Chiba Institute of Technology). 11 indexed citations
12.
Paunzen, E., Klaus Bernhard, Stefan Hümmerich, et al.. (2019). Search for stellar spots in field blue horizontal-branch stars. Springer Link (Chiba Institute of Technology). 6 indexed citations
13.
Mikulášek, Zdeněk, Jiřı́ Krtička, E. Paunzen, et al.. (2018). Differential rotation in magnetic chemically peculiar stars. Contributions of the Astronomical Observatory Skalnaté Pleso. 48(1). 203–207. 1 indexed citations
14.
Hümmerich, Stefan, Franz-Josef Hambsch, Franky Dubois, et al.. (2016). NSV 1907 - A new eclipsing, nova-like cataclysmic variable. New Astronomy. 50. 30–36. 4 indexed citations
15.
Bernhard, Klaus, Stefan Hümmerich, S. Otero, & E. Paunzen. (2015). A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data. Springer Link (Chiba Institute of Technology). 12 indexed citations
16.
Frank, Peter, et al.. (2015). Lichtkurve und Periode von 2 neuen Bedeckungsveraenderlichen. 64. 80–82. 1 indexed citations
17.
Lloyd, C., et al.. (2007). GSC 3377-0296 is a New Short-Period Eclipsing RS CVn Variable. Information Bulletin on Variable Stars. 5772. 1–2. 1 indexed citations
18.
Lloyd, C., et al.. (2002). Two New Eclipsing Binaries: V1626 Ori (Brh V38) and GSC 0486-4828 (Brh V64). IBVS. 5339. 1. 1 indexed citations
19.
Bernhard, Klaus, et al.. (2001). Photo- and Radiation-Chemical Formation and Electrophilic and Electron Transfer Reactivities of Enolether Radical Cations in Aqueous Solution. Chemistry - A European Journal. 7(21). 4640–4650. 16 indexed citations
20.
Bernhard, Klaus. (1968). Seelsorgerliche Begegnung mit dem modernen Menschen im Blick auf die »Neue Moral«. Praktische Theologie. 3(3). 242–261. 1 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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