H. Brunner

10.4k total citations
87 papers, 2.3k citations indexed

About

H. Brunner is a scholar working on Astronomy and Astrophysics, Electronic, Optical and Magnetic Materials and Nuclear and High Energy Physics. According to data from OpenAlex, H. Brunner has authored 87 papers receiving a total of 2.3k indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 17 papers in Electronic, Optical and Magnetic Materials and 16 papers in Nuclear and High Energy Physics. Recurrent topics in H. Brunner's work include Astrophysical Phenomena and Observations (31 papers), Galaxies: Formation, Evolution, Phenomena (21 papers) and Magnetism in coordination complexes (16 papers). H. Brunner is often cited by papers focused on Astrophysical Phenomena and Observations (31 papers), Galaxies: Formation, Evolution, Phenomena (21 papers) and Magnetism in coordination complexes (16 papers). H. Brunner collaborates with scholars based in Germany, United States and Spain. H. Brunner's co-authors include Hanspaul Hagenmaier, Roland Haag, Michael Kraft, Karl H. Hausser, G. Hasinger, Petra Bele, D. Schweitzer, F. A. Neugebauer, A. C. Fabian and H. J. Keller and has published in prestigious journals such as Advanced Materials, The Journal of Chemical Physics and Physical review. B, Condensed matter.

In The Last Decade

H. Brunner

85 papers receiving 2.2k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
H. Brunner Germany 27 949 437 431 411 296 87 2.3k
Dongwon Kim United States 15 373 0.4× 52 0.1× 111 0.3× 47 0.1× 105 0.4× 31 1.4k
Svatopluk Civiš Czechia 28 878 0.9× 35 0.1× 90 0.2× 38 0.1× 421 1.4× 179 2.7k
Victor F. Plyusnin Russia 20 172 0.2× 489 1.1× 27 0.1× 104 0.3× 653 2.2× 111 1.5k
Rolf Mitzner Germany 26 41 0.0× 191 0.4× 59 0.1× 318 0.8× 496 1.7× 119 2.6k
A. Ichimura United States 26 230 0.2× 53 0.1× 24 0.1× 436 1.1× 806 2.7× 58 2.6k
Anmin Tian China 29 908 1.0× 40 0.1× 22 0.1× 137 0.3× 691 2.3× 198 2.9k
Thomas Pino France 30 946 1.0× 22 0.1× 20 0.0× 54 0.1× 786 2.7× 119 2.6k
John C. Fetzer United States 33 73 0.1× 39 0.1× 229 0.5× 93 0.2× 707 2.4× 166 3.1k
Svend J. Knak Jensen Denmark 20 89 0.1× 67 0.2× 43 0.1× 56 0.1× 222 0.8× 91 1.2k
Takashi Tsuji Japan 30 616 0.6× 12 0.0× 8 0.0× 147 0.4× 720 2.4× 179 2.9k

Countries citing papers authored by H. Brunner

Since Specialization
Citations

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

Fields of papers citing papers by H. Brunner

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of H. Brunner

This figure shows the co-authorship network connecting the top 25 collaborators of H. Brunner. A scholar is included among the top collaborators of H. Brunner 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 H. Brunner. H. Brunner 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.
Tubín-Arenas, D., M. Krumpe, G. Lamer, et al.. (2024). The eROSITA upper limits. Astronomy and Astrophysics. 682. A35–A35. 14 indexed citations
2.
Hornschemeier, A. E., F. Haberl, Antara Basu‐Zych, et al.. (2021). The eROSITA Final Equatorial-Depth Survey (eFEDS). Astronomy and Astrophysics. 661. A16–A16. 9 indexed citations
3.
Predehl, P., Thomas Böller, Diogo Coutinho, et al.. (2018). eROSITA ground operations. 193–193. 4 indexed citations
4.
Miyaji, T., T. Ishigaki, M. Krumpe, et al.. (2017). High excitation emission line nebula associated with an ultra-luminous X-ray source atz= 0.027 in the AKARI North Ecliptic Pole Deep Field. Astronomy and Astrophysics. 604. A14–A14. 4 indexed citations
5.
Miyaji, T., G. Hasinger, M. Salvato, et al.. (2015). DETAILED SHAPE AND EVOLUTIONARY BEHAVIOR OF THE X-RAY LUMINOSITY FUNCTION OF ACTIVE GALACTIC NUCLEI. The Astrophysical Journal. 804(2). 104–104. 62 indexed citations
6.
Ranalli, P., A. Comastri, C. Vignali, et al.. (2013). The XMM deep survey in the CDF-S. Astronomy and Astrophysics. 555. A42–A42. 32 indexed citations
7.
Kreykenbohm, I., Christoph Schmid, J. Wilms, H. Brunner, & G. Lamer. (2009). The eROSITA Near Realtime Analysis. Interpretation A Journal of Bible and Theology. 411. 149–288. 1 indexed citations
8.
Mateos, S., R. S. Warwick, F. J. Carrera, et al.. (2008). High precision X-ray log N – log S distributions: implications for the obscured AGN population. Astronomy and Astrophysics. 492(1). 51–69. 50 indexed citations
9.
Carrera, F. J., J. Ebrero, S. Mateos, et al.. (2007). The XMM-Newton serendipitous survey - III. The AXIS X-ray source counts and angular clustering. Figshare. 35 indexed citations
10.
Carrera, F. J., J. Ebrero, S. Mateos, et al.. (2007). The XMM-Newton serendipitous survey. Astronomy and Astrophysics. 469(1). 27–46. 44 indexed citations
11.
Brunner, H., N. Cappelluti, G. Hasinger, et al.. (2007). XMM-Newtonobservations of the Lockman Hole: X-ray source catalogue and number counts. Astronomy and Astrophysics. 479(1). 283–300. 47 indexed citations
12.
Ceca, R. Della, T. Maccacaro, A. Caccianiga, et al.. (2004). Exploring the X-ray sky with the\nXMM-Newton bright serendipitous survey \n. Springer Link (Chiba Institute of Technology). 67 indexed citations
13.
Hashimoto, Yasuhiro, X. Barcons, H. Böhringer, et al.. (2004). Abundance constraints and direct redshift measurement of the diffuse X-ray emission from a distant cluster of galaxies. Astronomy and Astrophysics. 417(3). 819–825. 19 indexed citations
14.
Schwope, A., H. Brunner, V. Hambaryan, & Richard P. Schwarz. (2002). LARPs -- Low-accretion rate polars. ASPC. 261. 102. 2 indexed citations
15.
Schwope, A., H. Brunner, D. A. H. Buckley, et al.. (2002). The census of cataclysmic variables in the ROSAT Bright Survey. Astronomy and Astrophysics. 396(3). 895–910. 53 indexed citations
16.
Page, K. L., K. O. Mason, F. J. Carrera, et al.. (2001). The variable XMM-Newton spectrum of Markarian 766. Springer Link (Chiba Institute of Technology). 24 indexed citations
17.
Abraham, Klaus, et al.. (1989). Elimination of various polychlorinated dibenzo-p-dioxins and dibenzofurans (PCDDs and PCDFs) in rat faeces. Archives of Toxicology. 63(1). 75–78. 15 indexed citations
18.
Abraham, Klaus, et al.. (1989). Absorption and tissue distribution of various polychlorinated dibenzo-p-dioxins and dibenzofurans (PCDDs and PCDFs) in the rat. Archives of Toxicology. 63(3). 193–202. 30 indexed citations
19.
Brunner, H., R. Fritsch, & Karl H. Hausser. (1987). Notizen: Cross Polarization in Electron Nuclear Double Resonance by Satisfying the Hartmann-Hahn Condition. Zeitschrift für Naturforschung A. 42(12). 1456–1457. 41 indexed citations
20.
Brunner, H., et al.. (1966). ESR-spectra of radical anions of macrocyclic aromatic compounds II: Tribenzo-cyclododecahexaene and tribenzocyclododecatrienetriine. Tetrahedron Letters. 7(24). 2775–2779. 6 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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