This map shows the geographic impact of M. Feissel'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 M. Feissel with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Feissel more than expected).
This network shows the impact of papers produced by M. Feissel. 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 M. Feissel. The network helps show where M. Feissel may publish in the future.
Co-authorship network of co-authors of M. Feissel
This figure shows the co-authorship network connecting the top 25 collaborators of M. Feissel.
A scholar is included among the top collaborators of M. Feissel 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 M. Feissel. M. Feissel 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.
Biancale, R., Jean‐Michel Lemoine, Sylvain Loyer, et al.. (2005). Geocenter : notion, definition and realization. AGUFM. 2005.1 indexed citations
Gontier, A. M., M. Feissel, & Chao Ma. (1997). The contribution of VLBI to the realization of a celestial reference system.. 23.2 indexed citations
4.
Arias, E. F., P. Charlot, M. Feissel, & J.-F. Lestrade. (1995). The extragalactic reference system of the International Earth Rotation Service, ICRS. 23. 604–608.24 indexed citations
5.
Boucher, C., Z. Altamimi, & M. Feissel. (1994). Results and analysis of the ITRF93.. 18. 1–166.71 indexed citations
6.
Feissel, M., et al.. (1994). Results from the SEARCH'92 campaign.. 16.2 indexed citations
7.
Vondrák, J., et al.. (1992). Expected accuracy of the 1900-1990 Earth orientation parameters in the Hipparcos reference frame. 262(1). 329–340.7 indexed citations
8.
Nastula, Jolanta, D. Gambis, & M. Feissel. (1990). Correlated high frequency variations in polar motion and length of the day in early 1988.. 8. 565–570.11 indexed citations
9.
Arias, E. F., M. Feissel, & J.-F. Lestrade. (1988). Comparison of VLBI celestial reference frames.. 199. 357–363.6 indexed citations
10.
Feissel, M. & B. Guinot. (1988). A homogeneous series of the Earth rotation parameters based on all observing techniques, 1962 - 1987.. 79.2 indexed citations
Feissel, M. & Christian Nıtschelm. (1985). Time-dependent aspects of the atmospheric driven fluctuations in the duration of the day.. Annales Geophysicae. 3(2). 181–185.6 indexed citations
Yokoyama, K., et al.. (1982). Project MERIT. Report on the Short Campaign and Grasse workshop with observations and results on earth-rotation during 1980 August_-October..1 indexed citations
16.
Chollet, F., et al.. (1976). Observations of Saturn with the astrolabe of the Paris Observatory during the winter 1974 - 1975.. 25. 365–367.
17.
Feissel, M., et al.. (1973). Observations of Saturn with the Astrolabe of the Paris Observatory during the Winter 1971-72. 26. 141.1 indexed citations
Feissel, M., et al.. (1969). Une valeur de la constante de l'aberration deduite de mesures optiques de vitesses radiales. 10. 1594–1596.1 indexed citations
20.
Feissel, M., et al.. (1968). Mesure spectrographique de mouvements dans l'atmosphere de Venus. 9(36). 13–20.8 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.