S. Müller

1.1k total citations
21 papers, 692 citations indexed

About

S. Müller is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, S. Müller has authored 21 papers receiving a total of 692 indexed citations (citations by other indexed papers that have themselves been cited), including 21 papers in Astronomy and Astrophysics, 4 papers in Instrumentation and 4 papers in Nuclear and High Energy Physics. Recurrent topics in S. Müller's work include Galaxies: Formation, Evolution, Phenomena (13 papers), Astrophysics and Star Formation Studies (10 papers) and Stellar, planetary, and galactic studies (8 papers). S. Müller is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (13 papers), Astrophysics and Star Formation Studies (10 papers) and Stellar, planetary, and galactic studies (8 papers). S. Müller collaborates with scholars based in Germany, Chile and Sweden. S. Müller's co-authors include R. Chini, U. Klaas, Martin Haas, D. Lemke, F. Combes, K. Meisenheimer, M. Guélin, J. H. Black, S. J. Curran and A. Beelen and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

S. Müller

21 papers receiving 677 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
S. Müller Germany 14 650 163 122 100 88 21 692
M. P. Redman United Kingdom 18 802 1.2× 123 0.8× 137 1.1× 70 0.7× 48 0.5× 68 816
R. J. Cohen United Kingdom 22 1.1k 1.7× 162 1.0× 235 1.9× 115 1.1× 50 0.6× 63 1.1k
Z. Wang United States 13 619 1.0× 55 0.3× 208 1.7× 100 1.0× 104 1.2× 14 665
D M-A Meyer Germany 19 817 1.3× 207 1.3× 101 0.8× 54 0.5× 22 0.3× 42 833
Tracy L. Beck United States 20 1.3k 2.0× 80 0.5× 235 1.9× 147 1.5× 46 0.5× 63 1.3k
Francis P. Wilkin United States 7 1.2k 1.8× 153 0.9× 143 1.2× 38 0.4× 35 0.4× 13 1.2k
T. Wiklind Sweden 11 490 0.8× 176 1.1× 46 0.4× 42 0.4× 69 0.8× 29 546
N. L. J. Cox Netherlands 13 498 0.8× 44 0.3× 61 0.5× 95 0.9× 62 0.7× 23 529
Kenji Hamaguchi United States 22 1.3k 2.0× 156 1.0× 99 0.8× 57 0.6× 28 0.3× 85 1.3k
V. Migenes Mexico 13 668 1.0× 260 1.6× 133 1.1× 20 0.2× 43 0.5× 49 698

Countries citing papers authored by S. Müller

Since Specialization
Citations

This map shows the geographic impact of S. 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 S. Müller with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Müller more than expected).

Fields of papers citing papers by S. Müller

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. 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 S. Müller. The network helps show where S. Müller may publish in the future.

Co-authorship network of co-authors of S. Müller

This figure shows the co-authorship network connecting the top 25 collaborators of S. Müller. A scholar is included among the top collaborators of S. 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 S. Müller. S. Müller 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.
Mangum, J. G., Cosima Eibensteiner, V. M. Rivilla, et al.. (2025). Complex organic molecules towards the central molecular zone of NGC 253. Astronomy and Astrophysics. 698. A261–A261. 2 indexed citations
2.
Justtanont, K., S. Müller, M. J. Barlow, et al.. (2017). Mass loss from an extreme OH/IR star: OH 26.5+0.6. UCL Discovery (University College London). 88. 342. 1 indexed citations
3.
Henkel, C., S. A. Levshakov, S. Müller, et al.. (2017). Testing the variability of the proton-to-electron mass ratio from observations of methanol in the dark cloud core L1498. Monthly Notices of the Royal Astronomical Society. 472(4). 4434–4443. 14 indexed citations
4.
Kanekar, Nissim, W. Ubachs, K. M. Menten, et al.. (2015). Constraints on changes in the proton–electron mass ratio using methanol lines. Monthly Notices of the Royal Astronomical Society Letters. 448(1). L104–L108. 38 indexed citations
5.
Müller, S., A. Beelen, J. H. Black, et al.. (2013). A precise and accurate determination of the cosmic microwave background temperature atz= 0.89. Astronomy and Astrophysics. 551. A109–A109. 67 indexed citations
6.
Müller, S., A. Beelen, M. Guélin, et al.. (2011). Molecules atz= 0.89. Astronomy and Astrophysics. 535. A103–A103. 108 indexed citations
7.
Müller, S., et al.. (2006). Probing isotopic ratios at z = 0.89: molecular line absorption in front of the quasar PKS 1830-211. 34 indexed citations
8.
Haas, Martin, R. Chini, S. Müller, F. Bertoldi, & M. Albrecht. (2005). MAMBO 1.25 mm observations of 3CR quasars at z ~ 1.5: on the debate of the unified schemes. Astronomy and Astrophysics. 445(1). 115–122. 4 indexed citations
9.
Müller, S., Mary E. Haas, R. Siebenmorgen, et al.. (2004). Dust in 3CR radio galaxies: On the FR 1 – FR 2 difference. Springer Link (Chiba Institute of Technology). 18 indexed citations
10.
Haas, Martin, R. Siebenmorgen, C. Leipski, et al.. (2004). Mid-infrared selection of AGN. Springer Link (Chiba Institute of Technology). 15 indexed citations
11.
Albrecht, M., R. Chini, E. Krügel, S. Müller, & R. Lemke. (2004). Cold dust and molecular gas towards the centers of Magellanic type galaxies and irregulars. Astronomy and Astrophysics. 414(1). 141–153. 21 indexed citations
12.
Haas, Martin, S. Müller, F. Bertoldi, et al.. (2004). The ISOPHOT - MAMBO survey of 3CR radio sources: Further evidence for the unified schemes. Astronomy and Astrophysics. 424(2). 531–543. 40 indexed citations
13.
Haas, Martin, U. Klaas, S. Müller, et al.. (2003). The ISO view of Palomar-Green quasars. Astronomy and Astrophysics. 402(1). 87–111. 96 indexed citations
14.
Nielbock, M., R. Chini, & S. Müller. (2003). The stellar content of OMC 2/3. Astronomy and Astrophysics. 408(1). 245–256. 29 indexed citations
15.
Haas, Martin, U. Klaas, S. Müller, R. Chini, & I. M. Coulson. (2001). The PAH 7.7 μm/850 μm ratio as new diagnostics for high extinction in ULIRGs -increasing evidence for a hidden quasar in Arp 220. Astronomy and Astrophysics. 367(3). L9–L13. 22 indexed citations
16.
Klaas, U., Martin Haas, S. Müller, et al.. (2001). Infrared to millimetre photometry of ultra-luminous IR galaxies : New evidence favouring a 3-stage dust model. Astronomy and Astrophysics. 379(3). 823–844. 112 indexed citations
17.
Meisenheimer, K., Martin Haas, S. Müller, et al.. (2001). Dust emission from 3C radio galaxies and quasars: New ISO observations favour the unified scheme. Astronomy and Astrophysics. 372(3). 719–729. 43 indexed citations
18.
Haas, M., S. Müller, R. Chini, et al.. (2000). Dust in PG quasars as seen by ISO. A&A. 354. 453–466. 1 indexed citations
19.
Guélin, M., S. Müller, J. Cernicharo, et al.. (2000). Astronomical detection of the free radical SiCN. 363. 12 indexed citations
20.
Peng, Bo, Adam L. Kraus, T. P. Krichbaum, et al.. (2000). Infrared, radio and optical variability of the BL Lacertae object 2007+777. 353(3). 937–943. 4 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.

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