U. Hopp

7.3k total citations
138 papers, 2.1k citations indexed

About

U. Hopp is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, U. Hopp has authored 138 papers receiving a total of 2.1k indexed citations (citations by other indexed papers that have themselves been cited), including 110 papers in Astronomy and Astrophysics, 89 papers in Instrumentation and 28 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in U. Hopp's work include Astronomy and Astrophysical Research (87 papers), Galaxies: Formation, Evolution, Phenomena (76 papers) and Stellar, planetary, and galactic studies (75 papers). U. Hopp is often cited by papers focused on Astronomy and Astrophysical Research (87 papers), Galaxies: Formation, Evolution, Phenomena (76 papers) and Stellar, planetary, and galactic studies (75 papers). U. Hopp collaborates with scholars based in Germany, United States and Russia. U. Hopp's co-authors include R. Bender, Niv Drory, Georg Feulner, R. P. Saglia, J. Snigula, L. Greggio, S. Seitz, A. Gabasch, Claudia Maraston and R. E. Schulte‐Ladbeck and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

U. Hopp

127 papers receiving 2.1k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
U. Hopp Germany 26 2.0k 1.1k 252 144 73 138 2.1k
Peter M. Weilbacher Germany 28 2.7k 1.3× 1.2k 1.1× 320 1.3× 157 1.1× 39 0.5× 100 2.7k
Ray A. Lucas United States 20 2.0k 1.0× 1.0k 0.9× 258 1.0× 150 1.0× 113 1.5× 60 2.1k
Myungshin Im South Korea 20 1.6k 0.8× 841 0.8× 197 0.8× 124 0.9× 56 0.8× 132 1.7k
M. A. Pahre United States 27 2.6k 1.3× 1.1k 1.0× 449 1.8× 97 0.7× 56 0.8× 46 2.7k
C. Gronwall United States 27 2.5k 1.2× 1.3k 1.1× 410 1.6× 125 0.9× 120 1.6× 129 2.5k
K. J. Fricke Germany 32 2.5k 1.2× 1.1k 1.0× 241 1.0× 81 0.6× 66 0.9× 108 2.6k
B. Lanzoni Italy 31 2.9k 1.4× 1.6k 1.4× 219 0.9× 157 1.1× 41 0.6× 113 3.0k
R. W. O’Connell United States 33 3.4k 1.7× 1.4k 1.2× 352 1.4× 117 0.8× 60 0.8× 142 3.5k
N. Arimoto Japan 35 3.5k 1.7× 1.9k 1.7× 324 1.3× 149 1.0× 61 0.8× 119 3.6k
P. Amram France 32 3.0k 1.5× 1.4k 1.3× 322 1.3× 119 0.8× 63 0.9× 140 3.1k

Countries citing papers authored by U. Hopp

Since Specialization
Citations

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

Fields of papers citing papers by U. Hopp

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of U. Hopp

This figure shows the co-authorship network connecting the top 25 collaborators of U. Hopp. A scholar is included among the top collaborators of U. Hopp 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 U. Hopp. U. Hopp 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.
Seth, Anil C., Peter Erwin, Victor P. Debattista, et al.. (2023). Composite Bulges. III. A Study of Nuclear Star Clusters in Nearby Spiral Galaxies. The Astrophysical Journal. 958(1). 100–100. 5 indexed citations
2.
Gebhardt, Karl, Erin Mentuch Cooper, John Chisholm, et al.. (2021). Detection of Lyman Continuum from 3.0 < z < 3.5 Galaxies in the HETDEX Survey. The Astrophysical Journal. 920(2). 122–122. 6 indexed citations
3.
Boehnhardt, H., A. Riffeser, C. Ries, Michael Schmidt, & U. Hopp. (2020). Mt. Wendelstein imaging of comet 41P/Tuttle-Giacobini-Kresak during the 2017 perihelion arc. Springer Link (Chiba Institute of Technology). 4 indexed citations
4.
Obermeier, Christian, H. Kellermann, R. P. Saglia, et al.. (2020). Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2b. Springer Link (Chiba Institute of Technology). 4 indexed citations
5.
Brucalassi, Anna, F. Grupp, Florian Lang-Bardl, et al.. (2012). A testbed for simultaneous measurement of fiber near and far-field for the evaluation of fiber scrambling properties. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 8446. 844692–844692. 6 indexed citations
6.
Montalto, M., S. Seitz, A. Riffeser, et al.. (2009). Properties of M31. Astronomy and Astrophysics. 507(1). 283–300. 31 indexed citations
7.
Bomans, D. J., J. van Eymeren, R.‐J. Dettmar, K. Weis, & U. Hopp. (2007). Galactic winds in dwarf galaxies. New Astronomy Reviews. 51(1-2). 141–145. 10 indexed citations
8.
Gabasch, A., U. Hopp, Georg Feulner, et al.. (2006). The evolution of the luminosity functions in the FORS deep field from low to high redshift. Astronomy and Astrophysics. 448(1). 101–121. 44 indexed citations
9.
Appenzeller, I., R. Bender, A. Böhm, et al.. (2004). Exploring Cosmic Evolution with the FORS Deep Field. Max Planck Institute for Plasma Physics. 116. 18–24. 4 indexed citations
10.
Gabasch, A., R. Bender, S. Seitz, et al.. (2004). The evolution of the luminosity functions in the FORS Deep Field from low to high redshift. Astronomy and Astrophysics. 421(1). 41–58. 90 indexed citations
11.
Heidt, J., Klaus Jäger, K. Nilsson, et al.. (2003). PKS 0537-441: Extended [O II] emission and a binary QSO?. Springer Link (Chiba Institute of Technology). 4 indexed citations
12.
Saracco, P., M. Longhetti, P. Severgnini, et al.. (2003). Massive $z\sim1.3$ evolved galaxies revealed. Astronomy and Astrophysics. 398(1). 127–132. 20 indexed citations
13.
Kniazev, A. Y., D. Engels, S. A. Pustilnik, et al.. (2001). The Hamburg/SAO survey for emission-line galaxies. Astronomy and Astrophysics. 366(3). 771–787. 11 indexed citations
14.
Hopp, U.. (1999). Distance, structure and bright stellar content\n of the dwarf irregular galaxy UGC 685. Springer Link (Chiba Institute of Technology). 6 indexed citations
15.
Klein, U., E. Hummel, D. J. Bomans, & U. Hopp. (1996). The synchrotron halo and magnetic field of NGC 4449.. 313(2). 396–404. 2 indexed citations
16.
Wagner, S. J., et al.. (1995). Simultaneous optical and gamma-ray flaring in PKS 0420-014. Implications for emission processes and rotating jet models.. A&A. 298. 688. 1 indexed citations
17.
Hopp, U., et al.. (1995). A redshift survey for faint galaxies towards voids of galaxies.. Astronomy & Astrophysics Supplement Series. 109. 537–549. 3 indexed citations
18.
Hopp, U. & R. E. Schulte‐Ladbeck. (1995). CCD photometry of 11 resolved dwarf irregular galaxies.. Astronomy & Astrophysics Supplement Series. 111. 527. 1 indexed citations
19.
Hopp, U. & U. Graser. (1990). Optical quality of the Calar Alto 3.5 M telescope. 235(4). 543–548. 1 indexed citations
20.
Hopp, U., et al.. (1985). The Antlia cluster of galaxies and its environment: the Hydra I-Centaurus supercluster. Astronomy & Astrophysics Supplement Series. 61(1). 93–106. 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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