E. Slezak

14.3k total citations
67 papers, 1.2k citations indexed

About

E. Slezak is a scholar working on Astronomy and Astrophysics, Instrumentation and Computer Vision and Pattern Recognition. According to data from OpenAlex, E. Slezak has authored 67 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 43 papers in Astronomy and Astrophysics, 30 papers in Instrumentation and 18 papers in Computer Vision and Pattern Recognition. Recurrent topics in E. Slezak's work include Galaxies: Formation, Evolution, Phenomena (31 papers), Astronomy and Astrophysical Research (30 papers) and Stellar, planetary, and galactic studies (16 papers). E. Slezak is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (31 papers), Astronomy and Astrophysical Research (30 papers) and Stellar, planetary, and galactic studies (16 papers). E. Slezak collaborates with scholars based in France, Italy and Germany. E. Slezak's co-authors include A. Bijaoui, H. Quintana, C. Ferrari, F. Durret, D. Gerbal, Q. A. Parker, M. J. Drinkwater, Sébastien Bourguignon, O. Smirnov and Jonathan S. Kenyon and has published in prestigious journals such as Science, The Astrophysical Journal and Proceedings of the IEEE.

In The Last Decade

E. Slezak

62 papers receiving 1.1k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
E. Slezak France 21 945 403 154 144 68 67 1.2k
Tsutomu T. Takeuchi Japan 26 1.5k 1.6× 530 1.3× 42 0.3× 178 1.2× 25 0.4× 154 2.1k
O. Ivy Wong Australia 21 1.5k 1.6× 630 1.6× 108 0.7× 309 2.1× 59 0.9× 76 1.6k
François Lanusse France 18 550 0.6× 188 0.5× 129 0.8× 80 0.6× 51 0.8× 38 769
B. Hoyle Germany 18 965 1.0× 479 1.2× 89 0.6× 98 0.7× 38 0.6× 35 1.2k
V. de Lapparent France 17 885 0.9× 355 0.9× 79 0.5× 210 1.5× 19 0.3× 34 1.0k
Barnaby Rowe United Kingdom 17 1.1k 1.2× 491 1.2× 174 1.1× 151 1.0× 36 0.5× 24 1.3k
W. Wamsteker Spain 21 1.3k 1.4× 152 0.4× 68 0.4× 302 2.1× 102 1.5× 118 1.5k
C. Tortora Italy 25 1.6k 1.7× 879 2.2× 105 0.7× 248 1.7× 80 1.2× 98 1.7k
M. Barbieri Italy 22 1.8k 1.9× 758 1.9× 192 1.2× 73 0.5× 60 0.9× 78 2.1k
E. A. Valentijn Australia 24 1.7k 1.8× 796 2.0× 66 0.4× 207 1.4× 85 1.3× 105 1.9k

Countries citing papers authored by E. Slezak

Since Specialization
Citations

This map shows the geographic impact of E. Slezak'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 E. Slezak with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. Slezak more than expected).

Fields of papers citing papers by E. Slezak

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by E. Slezak. 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 E. Slezak. The network helps show where E. Slezak may publish in the future.

Co-authorship network of co-authors of E. Slezak

This figure shows the co-authorship network connecting the top 25 collaborators of E. Slezak. A scholar is included among the top collaborators of E. Slezak 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 E. Slezak. E. Slezak 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.
Ducourant, C., et al.. (2022). Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation. arXiv (Cornell University). 5 indexed citations
2.
Wertz, O., Daniel Stern, A. Krone-Martins, et al.. (2019). Gaia GraL: Gaia DR2 gravitational lens systems. Astronomy and Astrophysics. 628. A17–A17. 3 indexed citations
3.
Krone-Martins, A., L. Delchambre, O. Wertz, et al.. (2018). Gaia GraL: Gaia DR2 gravitational lens systems. I. New quadruply imaged quasar candidates around known quasars. CaltechAUTHORS (California Institute of Technology). 7 indexed citations
4.
Ducourant, C., O. Wertz, A. Krone-Martins, et al.. (2018). Gaia GraL: Gaia DR2 gravitational lens systems. II. The known multiply imaged quasars. SPIRE - Sciences Po Institutional REpository. 5 indexed citations
5.
Ducourant, C., O. Wertz, A. Krone-Martins, et al.. (2018). GaiaGraL:GaiaDR2 gravitational lens systems. Astronomy and Astrophysics. 618. A56–A56. 16 indexed citations
6.
Perret, Benjamin, Sébastien Lefèvre, C. Collet, & E. Slezak. (2011). Hyperconnections and Hierarchical Representations for Grayscale and Multiband Image Processing. IEEE Transactions on Image Processing. 21(1). 14–27. 22 indexed citations
7.
Chilingarian, Igor, V. Cayatte, L. Chemin, et al.. (2007). Discovery of a new M 32-like “Compact Elliptical” galaxy in thehalo of the Abell 496 cD galaxy. Astronomy and Astrophysics. 466(2). L21–L24. 29 indexed citations
8.
Proust, Dominique, H. Quintana, E. R. Carrasco, et al.. (2006). Structure and dynamics of the Shapley Supercluster - Velocity catalogue, general morphology and mass. SPIRE - Sciences Po Institutional REpository. 48 indexed citations
9.
Proust, Dominique, H. Quintana, E. R. Carrasco, et al.. (2006). The Shapley supercluster : the largest matter concentration in the local Universe. Msngr. 124. 30. 2 indexed citations
10.
Olsen, L. F., Christophe Benoıst, A. Cappi, et al.. (2006). Galaxy clusters in the CFHTLS. Astronomy and Astrophysics. 461(1). 81–93. 17 indexed citations
11.
Ferrari, C., Christophe Benoıst, S. Maurogordato, A. Cappi, & E. Slezak. (2005). Dynamical state and star formation properties of the merging galaxy cluster Abell 3921. Springer Link (Chiba Institute of Technology). 39 indexed citations
12.
Adami, C., E. Slezak, F. Durret, et al.. (2004). Large scale diffuse light in the Coma cluster: A multi-scale approach. Springer Link (Chiba Institute of Technology). 26 indexed citations
13.
Bourdin, H., et al.. (2004). Temperature map computation for X-ray clusters of galaxies. Astronomy and Astrophysics. 414(2). 429–443. 19 indexed citations
14.
Reisenegger, Andreas, H. Quintana, D. Proust, & E. Slezak. (2002). Dynamics and mass of the Shapley Supercluster, the largest bound structure in the local Universe. Msngr. 107. 18–23.
15.
Durret, F., E. Slezak, Richard Lieu, S. Dos Santos, & Massimiliano Bonamente. (2002). The extreme ultraviolet excess emission in five clusters of galaxiesrevisited. Astronomy and Astrophysics. 390(2). 397–406. 13 indexed citations
16.
Durret, F., et al.. (1999). A catalogue of velocities in the direction of the cluster ofgalaxies Abell 496. Springer Link (Chiba Institute of Technology). 3 indexed citations
17.
Durret, F., et al.. (1998). A catalogue of velocities in the cluster of galaxies Abell 85. Springer Link (Chiba Institute of Technology). 17 indexed citations
18.
Biviano, A., F. Durret, D. Gerbal, et al.. (1997). A photometric catalogue of the Coma cluster core. Springer Link (Chiba Institute of Technology). 8 indexed citations
19.
Bouchet, P., et al.. (1989). Infrared photometry and spectrophotometry of SN 1987A. I - March to October 1987 observations. Open Repository and Bibliography (University of Liège).
20.
Slezak, E., et al.. (1988). Study of a field in the Coma Supercluster. I: Automated galaxies count. Astronomy & Astrophysics Supplement Series. 74(1). 83–106. 6 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.

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