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.
This map shows the geographic impact of M. Cassé'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. Cassé with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Cassé more than expected).
This network shows the impact of papers produced by M. Cassé. 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. Cassé. The network helps show where M. Cassé may publish in the future.
Co-authorship network of co-authors of M. Cassé
This figure shows the co-authorship network connecting the top 25 collaborators of M. Cassé.
A scholar is included among the top collaborators of M. Cassé 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. Cassé. M. Cassé is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Cassé, M., Laurent Brunet, P. Batude, et al.. (2017). Thermal effects in 3D sequential technology. HAL (Le Centre pour la Communication Scientifique Directe).6 indexed citations
Cordier, B., D. Attié, M. Cassé, et al.. (2004). Search for a Light Dark Matter Annihilation Signal in the Sagittarius Dwarf Galaxy. CERN Bulletin. 552. 581.1 indexed citations
Lebrun, F., A. Bazzano, V. Borrel, et al.. (2003). The Compton Cube. Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment. 504(1-3). 38–43.1 indexed citations
Vangioni–Flam, E., A. Coc, & M. Cassé. (2000). Big bang nucleosynthesis updated with the NACRE compilation. HAL (Le Centre pour la Communication Scientifique Directe). 360. 15–23.6 indexed citations
10.
Vangioni–Flam, E., M. Cassé, & R. Ramaty. (1997). Light element production by low energy nuclei from massive stars. ESASP. 382. 123.1 indexed citations
Vangioni–Flam, E., M. Cassé, J. Audouze, & J. Trân Thanh Vân. (1990). Astrophysical ages and dating methods. 5.34 indexed citations
15.
Prantzos, Nikos, M. Arnould, J. P. Arcoragi, & M. Cassé. (1985). Neutron-rich nuclei in cosmic rays and Wolf-Rayet stars. NASA Technical Reports Server (NASA). 3. 167.3 indexed citations
16.
Cassé, M.. (1981). Cosmic ray sources. I - Clues to the origin of galactic cosmic rays. ICRC. 13. 111–130.1 indexed citations
17.
Césarsky, C. J., R. Rothenflug, & M. Cassé. (1981). Mass Per Charge Ratio in Hot Plasmas and Cosmic-Ray Source Composition. International Cosmic Ray Conference. 2. 269.2 indexed citations
18.
Meyer, J. P. & M. Cassé. (1979). Origin of the Solar Cosmic Ray Composition. International Cosmic Ray Conference. 5. 76.1 indexed citations
19.
Cassé, M., J. P. Meyer, & H. Reeves. (1979). The Cosmic-Ray Source Composition as a Probe of the Acceleration Mechanisms. ICRC. 2. 114.1 indexed citations
20.
Cassé, M., P. Goret, & C. J. Césarsky. (1975). Atomic Properties of the Elements and Cosmic Ray Composition at the Source. International Cosmic Ray Conference. 2. 646.1 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.