This map shows the geographic impact of M. Bester'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. Bester with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Bester more than expected).
This network shows the impact of papers produced by M. Bester. 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. Bester. The network helps show where M. Bester may publish in the future.
Co-authorship network of co-authors of M. Bester
This figure shows the co-authorship network connecting the top 25 collaborators of M. Bester.
A scholar is included among the top collaborators of M. Bester 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. Bester. M. Bester 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.
Lillis, R. J., Aroh Barjatya, D. W. Curtis, et al.. (2018). The ESCAPADE mission to Mars: Escape and Plasma Acceleration and Dynamics Explorers. SPIRE - Sciences Po Institutional REpository. 2018.
2.
Garrick‐Bethell, I., Robert P. Lin, Hugo Santiago Sánchez, et al.. (2013). Lunar magnetic field measurements with a cubesat. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 8739. 873903–873903.18 indexed citations
Bester, M., et al.. (2007). TELEMETRY AND COMMAND FRAME ROUTING IN A MULTI-MISSION ENVIRONMENT. UA Campus Repository (The University of Arizona).7 indexed citations
7.
Cruzalèbes, P., B. López, M. Bester, É. Gendron, & B. Sams. (1998). Near-infrared adaptive optics imaging of dust shells around five late-type stars with COME-ON+. 338(1). 132–138.
8.
Townes, C. H., M. Bester, W. C. Danchi, et al.. (1998). Infrared Spatial Interferometer. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3350. 908–908.5 indexed citations
Danchi, W. C., M. Bester, L. J. Greenhill, C. G. Degiacomi, & C. H. Townes. (1994). Analysis of Visibility Data from the U.C. Berkeley Infrared Spatial Interferometer-Radiative Transfer Modeling and Results on Fifteen Stars.. Proc SPIE. 2200. 286–303.3 indexed citations
12.
Danchi, W. C., L. J. Greenhill, M. Bester, C. G. Degiacomi, & C. H. Townes. (1992). Long Baseline Interferometric Observations of the Spatial Distribution of Dust Surrounding Late-Type Stars at 11 microns. AAS. 181.
13.
Bester, M., C. G. Degiacomi, W. C. Danchi, L. J. Greenhill, & C. H. Townes. (1992). Automation of Interferometric Observations. ASPC. 34. 213.1 indexed citations
Danchi, W. C., M. Bester, & C. H. Townes. (1988). The U.C. Berkeley infrared heterodyne interferometer.. European Southern Observatory Conference and Workshop Proceedings. 29. 867–877.1 indexed citations
Olberg, M., M. Bester, Gioia Rau, et al.. (1985). A new search for and discovery of deuterated ammonia in three molecular clouds. 142(1).3 indexed citations
19.
Bester, M., Kazunari Yamada, G. Winnewisser, & Š. Urban. (1983). The nuclear hyperfine structure of deuterated ammonia. A&A. 121(1).1 indexed citations
20.
Winnewisser, G., et al.. (1982). The Cologne 3-m millimetre and submillimetre radio telescope. ESASP. 189. 53–57.1 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.