Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
What Powers UltraluminousIRASGalaxies?
1998708 citationsR. Genzel, D. Lutz et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
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).
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.
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
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
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
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.