This map shows the geographic impact of T. Müller'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 T. Müller with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Müller more than expected).
This network shows the impact of papers produced by T. Müller. 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 T. Müller. The network helps show where T. Müller may publish in the future.
Co-authorship network of co-authors of T. Müller
This figure shows the co-authorship network connecting the top 25 collaborators of T. Müller.
A scholar is included among the top collaborators of T. Müller 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 T. Müller. T. Müller is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
19 of 19 papers shown
1.
Szakáts, Róbert, Csaba Kiss, G. Marton, et al.. (2017). Serendipitous observations of asteroids in Herschel PACS and SPIRE maps. EPSC.1 indexed citations
Barucci, Maria Antonella, F. Merlin, D. Perna, et al.. (2012). The extra red plutino (55638) 2002 VE95. Astronomy and Astrophysics. 539. A152–A152.7 indexed citations
8.
Lellouch, E., P. Santos-Sanz, M. Mommert, et al.. (2012). Thermal Properties Of Trans-neptunian Objects And Centaurs From Combined Herschel And Spitzer Observations. elib (German Aerospace Center).1 indexed citations
Érard, S., O. Forni, Matthieu Ollivier, et al.. (2005). The 2004 opposition of ceres observed with adaptive optics on the VLT. Max Planck Institute for Plasma Physics. 1388.2 indexed citations
12.
Burgdorf, M., et al.. (2003). Matching the Spectrometers on board ISO. Max Planck Institute for Plasma Physics. 481. 175–178.1 indexed citations
Müller, T., J. S. V. Lagerros, M. Burgdorf, et al.. (1999). Fundamental thermal emission parameters of main-belt asteroids derived from ISO. 427. 141.11 indexed citations
16.
Müller, T. & J. S. V. Lagerros. (1999). Fundamental Properties and Thermophysical Modelling of Asteroids after ISO. DPS. 31(4). 1075.2 indexed citations
17.
Dotto, E., T. Müller, J. Crovisier, et al.. (1999). ISO observations of main belt asteroids.. UvA-DARE (University of Amsterdam). 31(4). 1075.4 indexed citations
18.
Müller, T. & J. S. V. Lagerros. (1998). Asteroids as far-infrared photometric standards for ISOPHOT. 338(1). 340–352.44 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.