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.
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
20141.6k citationsMark Vogelsberger, Shy Genel et al.Monthly Notices of the Royal Astronomical Societyprofile →
Properties of galaxies reproduced by a hydrodynamic simulation
2014917 citationsMark Vogelsberger, Shy Genel et al.profile →
The illustris simulation: Public data release
2015372 citationsDylan Nelson, Annalisa Pillepich et al.profile →
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. Xu'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. Xu with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Xu more than expected).
This network shows the impact of papers produced by D. Xu. 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. Xu. The network helps show where D. Xu may publish in the future.
Co-authorship network of co-authors of D. Xu
This figure shows the co-authorship network connecting the top 25 collaborators of D. Xu.
A scholar is included among the top collaborators of D. Xu 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. Xu. D. Xu is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Xu, D., et al.. (2020). GRB 200219C: Nanshan/NEXT optical upper limit and possible host galaxy from PanSTARRS. GRB Coordinates Network. 27161. 1.1 indexed citations
9.
Izzo, L., et al.. (2020). GRB 201015A: redshift confirmation. GRB Coordinates Network. 28661. 1.2 indexed citations
Канн, Д. А., C. C. Thoene, J. Selsing, et al.. (2019). GRB 190114C: X-shooter observations of a highly extinguished afterglow.. GRB Coordinates Network. 23710. 1.
Izzo, L., J. Selsing, J. Japelj, et al.. (2017). GRB 171205A: VLT/X-shooter optical counterpart and spectroscopic observations.. GCN. 22180. 1.2 indexed citations
16.
Flores, H., S. Covino, D. Xu, et al.. (2013). GRB 130427A: VLT/X-shooter redshift confirmation. UvA-DARE (University of Amsterdam). 14491(1). 1.2 indexed citations
17.
Xu, D., et al.. (2013). GRB 131004A: optical afterglow from the NOT.. GCN. 15304. 1.1 indexed citations
18.
Fynbo, J. P. U., et al.. (2012). GRB 120811C: NOT redshift.. GRB Coordinates Network. 13632. 1.1 indexed citations
19.
Xu, D., Xiaohong Zhao, J. R. Mao, & J. M. Bai. (2011). GRB 111215A: GMG optical upper limit.. GRB Coordinates Network. 12683. 1.1 indexed citations
20.
Thoene, C. C., J. Gorosabel, S. Guziy, et al.. (2010). GRB 101225: optical follow-up of the christmas burst.. GRB Coordinates Network. 11503. 1.1 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.