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.
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
2010339 citationsP. A. Crowther, O. Schnurr et al.Monthly Notices of the Royal Astronomical Societyprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of O. Schnurr'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 O. Schnurr with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites O. Schnurr more than expected).
This network shows the impact of papers produced by O. Schnurr. 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 O. Schnurr. The network helps show where O. Schnurr may publish in the future.
Co-authorship network of co-authors of O. Schnurr
This figure shows the co-authorship network connecting the top 25 collaborators of O. Schnurr.
A scholar is included among the top collaborators of O. Schnurr 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 O. Schnurr. O. Schnurr is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Schnurr, O., C. J. Walcher, C. Chiappini, et al.. (2014). From space to specs: requirements for 4MOST. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 9150. 91501C–91501C.2 indexed citations
Scholz, R.‐D., et al.. (2012). WISE J181834.00-284919.6: a bright infrared Nova in the Galactic bulge?. The astronomer's telegram. 4268. 1.1 indexed citations
11.
Scholz, R.‐D., G. Bihain, O. Schnurr, & J. Storm. (2012). UKIDSS detections of cool brown dwarfs. Astronomy and Astrophysics. 541. A163–A163.8 indexed citations
Chené, André-Nicolas, O. Schnurr, P. A. Crowther, E. Fernández Lajús, & A. F. J. Moffat. (2010). Very massive binaries in R 136. Proceedings of the International Astronomical Union. 6(S272). 497–498.3 indexed citations
16.
Crowther, P. A., O. Schnurr, Raphaël Hirschi, et al.. (2010). The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit. Monthly Notices of the Royal Astronomical Society. 408(2). 731–751.339 indexed citations breakdown →
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.