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.
New catalogue of optically visible open clusters and candidates
2002595 citationsW. S. Dias, B. S. Alessi et al.Astronomy and Astrophysicsprofile →
Updated parameters of 1743 open clusters based on Gaia DR2
2021183 citationsW. S. Dias, A. Moitinho 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
Countries citing papers authored by J. R. D. Lépine
Since
Specialization
Citations
This map shows the geographic impact of J. R. D. Lépine'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 J. R. D. Lépine with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. R. D. Lépine more than expected).
This network shows the impact of papers produced by J. R. D. Lépine. 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 J. R. D. Lépine. The network helps show where J. R. D. Lépine may publish in the future.
Co-authorship network of co-authors of J. R. D. Lépine
This figure shows the co-authorship network connecting the top 25 collaborators of J. R. D. Lépine.
A scholar is included among the top collaborators of J. R. D. Lépine 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 J. R. D. Lépine. J. R. D. Lépine is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lépine, J. R. D., et al.. (2014). A Minimum of Stellar Density at the Corotation Radius of the Milky Way Spiral Pattern. ASPC. 480. 23.
12.
Lépine, J. R. D., et al.. (2012). Galactic corotation as a principal ``driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. 27(2). 359–364.1 indexed citations
Dias, W. S., B. S. Alessi, A. Moitinho, & J. R. D. Lépine. (2002). VizieR Online Data Catalog: Optically visible open clusters and Candidates (Dias+ 2002-2005).3 indexed citations
16.
Epchtein, N., T. Le Bertre, P. Fouqué, et al.. (1993). Identification of 106 new infrared carbon stars in the IRAS Point Source Catalog: near-infrared photometry and their space distribution in the Galaxy. Astronomy & Astrophysics Supplement Series. 99(1). 31–69.3 indexed citations
17.
Lépine, J. R. D., et al.. (1988). Star counts and IRAS sources in southern dark clouds. Astronomy & Astrophysics Supplement Series. 76(3). 347–363.
18.
Epchtein, N., et al.. (1987). Valinhos 2.2 micron survey of the southern galactic plane.II. Near-IR photometry, IRAS identifications and nature of the sources.. Astronomy & Astrophysics Supplement Series. 71. 39–55.2 indexed citations
19.
Epchtein, N., et al.. (1985). Valinhos 2.2 micron survey of the southern galactic plane. Positions and infrared photometry of 338 sources. Astronomy & Astrophysics Supplement Series. 61(2). 203–210.2 indexed citations
20.
Lépine, J. R. D., et al.. (1974). OH emission associated with early-type stars.. A&A. 36. 469–472.1 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.