This map shows the geographic impact of A. Mazure'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 A. Mazure with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Mazure more than expected).
This network shows the impact of papers produced by A. Mazure. 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 A. Mazure. The network helps show where A. Mazure may publish in the future.
Co-authorship network of co-authors of A. Mazure
This figure shows the co-authorship network connecting the top 25 collaborators of A. Mazure.
A scholar is included among the top collaborators of A. Mazure 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 A. Mazure. A. Mazure is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Olsen, L. F., Christophe Benoıst, A. Cappi, et al.. (2007). Galaxy clusters in the CFHTLS. Astronomy and Astrophysics. 478(1). 93–94.
2.
Brun, V. Le, A. Mazure, S. Arnouts, & D. Burgarella. (2006). The fabulous destiny of galaxies : bridging past and present. Foundations of Digital Games.43 indexed citations
Mazure, A., J. Perea, & V. Le Brun. (2000). Clustering at High Redshift. ASPC. 200.42 indexed citations
6.
Katgert, P., A. Mazure, R. den Hartog, et al.. (1998). The ESO Nearby Abell Cluster Survey. Astronomy and Astrophysics Supplement Series. 129(2). 399–412.78 indexed citations
7.
Adami, C., et al.. (1998). The ESO nearby Abell cluster survey. IV. The fundamental plane of clusters of galaxies. Leiden Repository (Leiden University). 331(2). 493–505.3 indexed citations
Giuricin, G., A. Biviano, A. Mazure, et al.. (1997). The ESO nearby Abell cluster survey.. 36. 129–131.22 indexed citations
10.
Gurzadyan, V. G. & A. Mazure. (1996). Revealing the galaxy associations in Abell 119. Observatory. 116. 391.2 indexed citations
11.
Biviano, A., G. Giuricin, P. Katgert, et al.. (1996). The ESO Nearby Abell Clusters Survey (ENACS): Velocity Dispersion Distribution for a Complete Cluster Sample. 33. 157.1 indexed citations
Durret, F., et al.. (1994). Clusters of galaxies: Proceedings of the XXIXth Rencontre de Moriond, XIVth Moriond Astrophysics Meetings, Méribel, Savoie, France, March 12-19, 1994. Medical Entomology and Zoology.5 indexed citations
15.
Durret, F., A. Mazure, & J. Trân Thanh Vân. (1994). Clusters of galaxies. 14.4 indexed citations
16.
Lapparent, V. de, Cindy Bellanger, S. Arnouts, et al.. (1993). Mapping the large-scale structure with the ESO multi-slit spectrographs.. Msngr. 72. 34–38.
17.
Sodré, L., H. V. Capelato, J. E. Steiner, D. Proust, & A. Mazure. (1992). The cluster of galaxies SC2008 - 57 (A3667). Monthly Notices of the Royal Astronomical Society. 259(2). 233–246.21 indexed citations
18.
Slezak, E., et al.. (1992). New evidence for subclustering in the Coma cluster using the wavelet analysis.. 264(2). 379–384.11 indexed citations
19.
Mellier, Y., et al.. (1988). Subclustering and evolution of the Coma cluster. 199. 67–72.9 indexed citations
20.
Capelato, H. V., et al.. (1987). New measurements of radial velocities in clusters of galaxies. Astronomy & Astrophysics Supplement Series. 67(1). 355–364.1 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.