D. Kunze

1.9k total citations · 1 hit paper
18 papers, 891 citations indexed

About

D. Kunze is a scholar working on Astronomy and Astrophysics, Instrumentation and Spectroscopy. According to data from OpenAlex, D. Kunze has authored 18 papers receiving a total of 891 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 6 papers in Instrumentation and 5 papers in Spectroscopy. Recurrent topics in D. Kunze's work include Stellar, planetary, and galactic studies (11 papers), Astrophysics and Star Formation Studies (8 papers) and Astronomy and Astrophysical Research (5 papers). D. Kunze is often cited by papers focused on Stellar, planetary, and galactic studies (11 papers), Astrophysics and Star Formation Studies (8 papers) and Astronomy and Astrophysical Research (5 papers). D. Kunze collaborates with scholars based in Germany, Australia and Netherlands. D. Kunze's co-authors include D. Lutz, R. Genzel, A. F. M. Moorwood, D. Rigopoulou, E. Sturm, Eiichi Egami, A. Sternberg, H. W. W. Spoon, N. Thatte and L. J. Tacconi and has published in prestigious journals such as The Astrophysical Journal, Space Science Reviews and Journal of Quantitative Spectroscopy and Radiative Transfer.

In The Last Decade

D. Kunze

18 papers receiving 880 citations

Hit Papers

What Powers UltraluminousIRASGalaxies? 1998 2026 2007 2016 1998 200 400 600

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. Kunze Germany 8 869 234 96 51 46 18 891
S. Oliver United Kingdom 12 717 0.8× 238 1.0× 120 1.3× 47 0.9× 26 0.6× 14 738
S. Lord United States 10 796 0.9× 168 0.7× 81 0.8× 53 1.0× 31 0.7× 15 805
eljko Ivezi United States 6 858 1.0× 254 1.1× 85 0.9× 54 1.1× 20 0.4× 6 873
B. Buckalew United States 10 819 0.9× 171 0.7× 45 0.5× 69 1.4× 43 0.9× 27 836
G. S. Wright United Kingdom 13 572 0.7× 170 0.7× 44 0.5× 47 0.9× 43 0.9× 22 590
F. Selman Chile 14 702 0.8× 283 1.2× 47 0.5× 29 0.6× 48 1.0× 44 722
S. J. U. Higdon United States 18 1.5k 1.7× 443 1.9× 148 1.5× 72 1.4× 34 0.7× 31 1.5k
R. B. C. Henry United States 16 845 1.0× 227 1.0× 103 1.1× 22 0.4× 25 0.5× 31 876
Kazushi Sakamoto Taiwan 21 1.3k 1.4× 200 0.9× 171 1.8× 135 2.6× 55 1.2× 50 1.3k
Letizia Stanghellini United States 21 1.3k 1.5× 517 2.2× 64 0.7× 45 0.9× 48 1.0× 67 1.3k

Countries citing papers authored by D. Kunze

Since Specialization
Citations

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

Fields of papers citing papers by D. Kunze

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Kunze

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

All Works

18 of 18 papers shown
1.
Rigopoulou, D., D. Kunze, D. Lutz, R. Genzel, & A. F. M. Moorwood. (2002). An ISO–SWS survey of molecular hydrogen in starburst and Seyfertgalaxies. Springer Link (Chiba Institute of Technology). 66 indexed citations
2.
Rodríguez-Fernández, Nemesio, J. Martín‐Pintado, P. de Vicente, et al.. (2000). Non-equilibrium H 2 ortho-to-para ratio in two molecular clouds of the Galactic Center. SPIRE - Sciences Po Institutional REpository. 356. 127–704. 1 indexed citations
3.
Sturm, E., D. Lutz, Dan N. Tran, et al.. (2000). ISO-SWS spectra of galaxies: Continuum and features ?. CERN Bulletin. 358. 481–493. 5 indexed citations
4.
Lutz, D., R. Genzel, D. Kunze, et al.. (1999). ISO Spectroscopy of Ultraluminous Infrared Galaxies. Astrophysics and Space Science. 266(1-2). 85–90. 8 indexed citations
5.
Fuente, A., J. Martín‐Pintado, Nemesio Rodríguez-Fernández, et al.. (1999). [ITAL]Infrared Space Observatory[/ITAL] Observations toward the Reflection Nebula NGC 7023: A Nonequilibrium Ortho–to–Para-H[TINF]2[/TINF] Ratio. The Astrophysical Journal. 518(1). L45–L48. 33 indexed citations
6.
Thornley, M. D., N. M. Förster Schreiber, H. W. W. Spoon, et al.. (1999). 30 Doradus as a Nearby Infrared Guide to Starbursts. Symposium - International Astronomical Union. 190. 247–248. 1 indexed citations
7.
Lundqvist, Peter, J. Sollerman, Cecilia Kozma, et al.. (1999). ISO SWS/LWS observations of SN 1987A. CERN Bulletin. 347(2). 500–507. 2 indexed citations
8.
Genzel, R., D. Lutz, E. Sturm, et al.. (1998). What Powers UltraluminousIRASGalaxies?. The Astrophysical Journal. 498(2). 579–605. 708 indexed citations breakdown →
9.
Sturm, E., D. Lutz, R. Genzel, et al.. (1996). ISO-SWS spectroscopy of Arp 220: A highly obscured starburst galaxy. University of Groningen research database (University of Groningen / Centre for Information Technology). 315(2). 2 indexed citations
10.
Kunze, D., D. Rigopoulou, D. Lutz, et al.. (1996). SWS spectroscopy of the colliding galaxies NGC 4038/39. University of Groningen research database (University of Groningen / Centre for Information Technology). 315(2). 3 indexed citations
11.
Lutz, D., H. Feuchtgruber, R. Genzel, et al.. (1996). SWS observations of the galactic center. Oxford University Research Archive (ORA) (University of Oxford). 315(2). 7 indexed citations
12.
Lutz, D., R. Genzel, A. Sternberg, et al.. (1996). What powers luminous infrared galaxies. University of Groningen research database (University of Groningen / Centre for Information Technology). 315(2). 3 indexed citations
13.
Lutz, D., R. Genzel, E. Egami, et al.. (1996). SWS SPECTROSCOPY OF THE STARBURST GALAXY NGC 3256. Oxford University Research Archive (ORA) (University of Oxford). 315(2). 1 indexed citations
14.
Thejll, Peter, et al.. (1994). Analysis of helium-rich subdwarf O stars. 1: NLTE models, methods, and FITS for 21 Palomar Green survey sdOs. The Astrophysical Journal. 433. 819–819. 21 indexed citations
15.
Vanbeveren, D., A. Herrero, D. Kunze, & M. H. van Kerkwijk. (1993). The mass and helium discrepancy in massive stars: The case Vela X-1. Space Science Reviews. 66(1-4). 395–400. 2 indexed citations
16.
Alonso‐Herrero, A., et al.. (1992). Intrinsic parameters of galactic luminous OB stars.. 261(1). 209–234. 17 indexed citations
17.
Lennon, D. J., et al.. (1991). Quantitative spectroscopy of B supergiants in the Galaxy, the LMC and theSMC. I. The B0.5 IA supergiants kappa Orionis, SK -68 41 and SK 159.. 252(2). 498–507. 1 indexed citations
18.
Kutepov, A. A., D. Kunze, D. G. Hummer, & G. B. Rybicki. (1991). The solution of radiative transfer problems in molecular bands without the LTE assumption by accelerated lambda iteration methods. Journal of Quantitative Spectroscopy and Radiative Transfer. 46(5). 347–365. 10 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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