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 vast, thin plane of corotating dwarf galaxies orbiting the Andromeda galaxy
2013320 citationsRodrigo Ibata, Geraint F. Lewis et al.Natureprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by D. Valls‐Gabaud
Since
Specialization
Citations
This map shows the geographic impact of D. Valls‐Gabaud'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. Valls‐Gabaud with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Valls‐Gabaud more than expected).
This network shows the impact of papers produced by D. Valls‐Gabaud. 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. Valls‐Gabaud. The network helps show where D. Valls‐Gabaud may publish in the future.
Co-authorship network of co-authors of D. Valls‐Gabaud
This figure shows the co-authorship network connecting the top 25 collaborators of D. Valls‐Gabaud.
A scholar is included among the top collaborators of D. Valls‐Gabaud 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. Valls‐Gabaud. D. Valls‐Gabaud is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Ibata, Rodrigo, Geraint F. Lewis, A. R. Conn, et al.. (2013). A vast, thin plane of corotating dwarf galaxies orbiting the Andromeda galaxy. Nature. 493(7430). 62–65.320 indexed citations breakdown →
11.
Valls‐Gabaud, D. & A. Boksenberg. (2011). The role of astronomy in society and culture : proceedings of the 260th symposium of the International Astronomical Union held at the UNESCO Headquarters, Paris, France January 19-23, 2009. Cambridge University Press eBooks.1 indexed citations
12.
Cabanac, R., D. Valls‐Gabaud, A. O. Jaunsen, C. Lidman, & Helmut Jerjen. (2005). Discovery of a high-redshift Einstein ring. Astronomy and Astrophysics. 436(2). L21–L25.25 indexed citations
Hernández, X., D. Valls‐Gabaud, & G. Gilmore. (2000). The recent star formation history of the Hipparcos solar neighbourhood.45 indexed citations
16.
Roukema, Boudewijn F., D. Valls‐Gabaud, Bahram Mobasher, & S. Bajtlik. (1999). Galaxy clustering at z 2 and halo radii. Monthly Notices of the Royal Astronomical Society. 305(1). 151–165.5 indexed citations
17.
Valls‐Gabaud, D., et al.. (1997). From quantum fluctuations to cosmological structures : proceedings of the First Moroccan School of Astrophysics, Casablanca, Morocco, 1-10 December 1996. Astronomical Society of the Pacific eBooks.1 indexed citations
18.
Lejeune, Thierry, et al.. (1996). Field and cluster binaries as tests of stellar evolution. ASPC. 90. 157.
19.
Guibert, J., et al.. (1995). The DUO programme: first results of a microlensing investigation of the Galactic disk and bulge conducted with the ESO Schmidt telescope.. Msngr. 80. 31–34.3 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.