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.
A super-Earth transiting a nearby low-mass star
2009389 citationsDavid Charbonneau, C. Lovis et al.profile →
The HARPS search for southern extra-solar planets
2007269 citationsS. Udry, X. Bonfıls et al.Astronomy and Astrophysicsprofile →
The HARPS search for southern extra-solar planets
2009206 citationsX. Bonfıls, T. Forveille et al.Astronomy and Astrophysicsprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
hero ref
This map shows the geographic impact of X. Bonfıls'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 X. Bonfıls with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites X. Bonfıls more than expected).
This network shows the impact of papers produced by X. Bonfıls. 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 X. Bonfıls. The network helps show where X. Bonfıls may publish in the future.
Co-authorship network of co-authors of X. Bonfıls
This figure shows the co-authorship network connecting the top 25 collaborators of X. Bonfıls.
A scholar is included among the top collaborators of X. Bonfıls 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 X. Bonfıls. X. Bonfıls is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Danchi, W. C., Richard Barry, B. López, et al.. (2010). Infrared Detection and Characterization of Debris Disks, Exozodiacal Dust, and Exoplanets: The FKSI Mission Concept. Open Repository and Bibliography (University of Liège).2 indexed citations
16.
Barry, Richard, W. C. Danchi, B. López, et al.. (2010). The Fourier-Kelvin Stellar Interferometer: Exploring Exoplanetary Systems with an Infrared Probe-class Mission. Open Repository and Bibliography (University of Liège). 430. 317.
17.
Udry, S., X. Bonfıls, X. Delfosse, et al.. (2008). The HARPS search for southern extra-solar planets ? XI. Super-Earths (5&8M ) in a 3-planet system. arXiv (Cornell University).1 indexed citations
18.
Delfosse, X., Jean-Luc Beuzit, Laura Marchal–Crespo, et al.. (2004). M dwarfs binaries: Results from accurate radial velocities and high angular resolution observations. ASPC. 318. 166–174.3 indexed citations
19.
Ségransan, D., J. L. Beuzit, X. Bonfıls, et al.. (2003). Mass-luminosity relations of very low-mass stars. 613.1 indexed citations
20.
Boehnhardt, H., X. Bonfıls, O. Hainaut, et al.. (2002). Post-perihelion coma monitoring of comet Hale-Bopp at ESO. Open Repository and Bibliography (University of Liège). 500. 613–616.1 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.