This map shows the geographic impact of É. Maurice'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 É. Maurice with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites É. Maurice more than expected).
This network shows the impact of papers produced by É. Maurice. 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 É. Maurice. The network helps show where É. Maurice may publish in the future.
Co-authorship network of co-authors of É. Maurice
This figure shows the co-authorship network connecting the top 25 collaborators of É. Maurice.
A scholar is included among the top collaborators of É. Maurice 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 É. Maurice. É. Maurice is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Udry, S., M. Mayor, J. Andersen, et al.. (1997). CORAVEL Radial Velocity Surveys of Late-Type Stars of the HIPPARCOS Mission. Research at the University of Copenhagen (University of Copenhagen). 402. 693–698.1 indexed citations
Gerbaldi, M., A. Gómez, S. Grenier, et al.. (1989). Complementary astrophysical data for Hipparcos stars. (1) Astrophysical fundamental parameters of early-type Hipparcos stars. (2) Radial velocities of southern late-type Hipparcos stars. Profile of two key programmes.. The Messenger. 56. 12–15.3 indexed citations
9.
Maurice, É., P. Bouchet, & N. Martin. (1989). BVR photoelectric photometry of late-type stars and a compilation of other data in the Small Magellanic Cloud.. Astronomy & Astrophysics Supplement Series. 78(3). 445–467.
10.
Imbert, M., J. Andersen, A. Ardeberg, et al.. (1989). Radial velocities of southern stars obtained with the photoelectric scanner Coravel. VII: Radial velocity variations of eleven Cepheids in the Large and Small Magellanic Clouds. Astronomy & Astrophysics Supplement Series. 81(3). 339–351.1 indexed citations
11.
Maurice, É., J. Andersen, A. Ardeberg, et al.. (1987). Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. VI: 233 F to M type stars in and near the Small Magellanic Cloud. Comparison with 80 spectrographic radial velocities of O to K type stars in this galaxy. Astronomy & Astrophysics Supplement Series. 67(3). 423–445.3 indexed citations
12.
Prévôt, L., J. Andersen, A. Ardeberg, et al.. (1985). Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. V: 404 F to M supergiant stars in the Large Magellanic Cloud. Astronomy & Astrophysics Supplement Series. 62(1). 23–37.1 indexed citations
13.
Bouchet, P., et al.. (1985). The visible and infrared extinction law and the gas-to-dust ratio in the Small Magellanic Cloud.. 149(2). 330–336.6 indexed citations
Prévôt, L., et al.. (1983). A catalogue of late-type supergiant stars in the Small Magellanic Cloud.. 53. 255–269.1 indexed citations
18.
Gillet, Denis, et al.. (1983). Pulsating stars, spectroscopy and shock waves.. Msngr. 34. 38–41.
19.
Gillet, Denis, É. Maurice, & D. Baade. (1983). The shock-induced variability of the H-alpha emission profile in Mira. II.. 128(2). 384–390.3 indexed citations
20.
Ardeberg, A., et al.. (1972). Spectrographic and photometric observations of supergiants and foreground stars, in the direction of the Large Magellanic Cloud.. Astronomy & Astrophysics Supplement Series. 6. 249–309.1 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.