S. Moehler

3.8k total citations
68 papers, 1.6k citations indexed

About

S. Moehler is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, S. Moehler has authored 68 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 53 papers in Astronomy and Astrophysics, 46 papers in Instrumentation and 8 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in S. Moehler's work include Stellar, planetary, and galactic studies (47 papers), Astronomy and Astrophysical Research (46 papers) and Astrophysics and Star Formation Studies (26 papers). S. Moehler is often cited by papers focused on Stellar, planetary, and galactic studies (47 papers), Astronomy and Astrophysical Research (46 papers) and Astrophysics and Star Formation Studies (26 papers). S. Moehler collaborates with scholars based in Germany, United States and Italy. S. Moehler's co-authors include U. Heber, D. Koester, R. Napiwotzki, A. V. Sweigart, P. Ballester, W. Freudling, D. M. Bramich, Mark Neeser, M. Romaniello and V. La Parola and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Atmospheric chemistry and physics.

In The Last Decade

S. Moehler

63 papers receiving 1.6k 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. Moehler Germany 24 1.6k 754 84 69 68 68 1.6k
Mark E. Everett United States 24 2.1k 1.3× 935 1.2× 72 0.9× 138 2.0× 68 1.0× 78 2.2k
А. В. Моисеев Russia 20 1.6k 1.0× 456 0.6× 202 2.4× 52 0.8× 35 0.5× 162 1.7k
A. Santerne France 20 1.3k 0.8× 526 0.7× 47 0.6× 62 0.9× 39 0.6× 69 1.3k
Alfred Rosenberg Spain 17 2.0k 1.3× 1.1k 1.5× 102 1.2× 80 1.2× 47 0.7× 31 2.1k
R. L. M. Corradi Spain 32 2.9k 1.9× 979 1.3× 158 1.9× 67 1.0× 54 0.8× 147 3.0k
G. Jasniewicz France 8 1.5k 0.9× 573 0.8× 194 2.3× 63 0.9× 47 0.7× 30 1.6k
Jeffrey R. Pier United States 16 2.0k 1.2× 875 1.2× 55 0.7× 106 1.5× 39 0.6× 29 2.0k
Elena Sabbi United States 25 2.3k 1.5× 1.1k 1.5× 132 1.6× 58 0.8× 26 0.4× 94 2.4k
Constance M. Rockosi United States 25 2.7k 1.7× 1.5k 1.9× 82 1.0× 80 1.2× 43 0.6× 49 2.7k
S. Borde France 2 1.2k 0.8× 471 0.6× 173 2.1× 53 0.8× 41 0.6× 5 1.3k

Countries citing papers authored by S. Moehler

Since Specialization
Citations

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

Fields of papers citing papers by S. Moehler

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of S. Moehler. A scholar is included among the top collaborators of S. Moehler 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. Moehler. S. Moehler 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.
Moehler, S.. (2024). Pollution versus diffusion: Abundance patterns of blue horizontal branch stars in the globular clusters NGC6388, NGC6397, and NGC6752. Astronomy and Astrophysics. 693. A136–A136. 1 indexed citations
2.
Spiniello, Chiara, C. Tortora, G. D’Ago, et al.. (2020). INSPIRE: INvestigating Stellar Population In RElics. Astronomy and Astrophysics. 646. A28–A28. 30 indexed citations
3.
Moehler, S., V. La Parola, T. Lanz, & M. M. Miller Bertolami. (2019). Hot UV-bright stars of galactic globular clusters. Springer Link (Chiba Institute of Technology). 23 indexed citations
4.
Noll, Stefan, Wuhu Feng, J. M. C. Plane, et al.. (2017). Measuring FeO variation using astronomical spectroscopic observations. Atmospheric chemistry and physics. 17(6). 4177–4187. 16 indexed citations
5.
Martayan, C., A. Mehner, G. Beccari, et al.. (2014). The X-shooter Imaging Mode. Msngr. 156. 21–23. 1 indexed citations
6.
Freudling, W., M. Romaniello, D. M. Bramich, et al.. (2013). Automated data reduction workflows for astronomy. Springer Link (Chiba Institute of Technology). 211 indexed citations
7.
Boffin, H. M. J., David Jones, Y. Beletsky, et al.. (2012). POPIPlaN: A Deep Morphological Catalogue of Newly Discovered Southern Planetary Nebulae. Durham Research Online (Durham University). 148. 25–27. 3 indexed citations
8.
Patat, F., S. Moehler, K. O’Brien, et al.. (2011). . UvA-DARE (University of Amsterdam). 53 indexed citations
9.
Modigliani, A., P. Goldoni, F. Royer, et al.. (2010). The X-shooter pipeline. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 7737. 773728–773728. 94 indexed citations
10.
Bidin, C. Moni, M. Catelan, S. Villanova, et al.. (2008). Binaries among Extreme Horizontal Branch Stars in Globular Clusters. ASPC. 392. 27. 1 indexed citations
11.
Szeifert, T., Roland Reiss, S. Deiries, et al.. (2007). FORS1 is getting Blue: New Blue Optimised Detectors and High Throughput Filters. Open Repository and Bibliography (University of Liège). 128. 9. 2 indexed citations
12.
Bidin, C. Moni, S. Moehler, G. Piotto, Y. Momany, & A. Recio–Blanco. (2007). Spectroscopy of horizontal branch stars in NGC6752 - Anomalous results on atmospheric parameters and masses. ArXiv.org. 18 indexed citations
13.
Moehler, S. & A. V. Sweigart. (2006). Observations of the hot horizontal-branch stars in the metal-rich bulge globular cluster NGC 6388. Astronomy and Astrophysics. 455(3). 943–952. 3 indexed citations
14.
Moehler, S., D. Koester, M. Zoccali, et al.. (2004). Spectral types and masses of white dwarfs in globular clusters. Springer Link (Chiba Institute of Technology). 33 indexed citations
15.
Moehler, S., V. La Parola, A. V. Sweigart, & F. Grundahl. (2003). Hot HB stars in globular clusters – Physical parameters andconsequences for theory. Springer Link (Chiba Institute of Technology). 15 indexed citations
16.
Napiwotzki, R., N. Christlieb, H. Drechsel, et al.. (2003). SPY - the ESO Supernovae type Ia Progenitor survey. University of Hertfordshire Research Archive (University of Hertfordshire). 112. 25–30. 51 indexed citations
17.
Heber, U., et al.. (2001). Early type stars at high galactic latitudes. Astronomy and Astrophysics. 378(3). 907–917. 42 indexed citations
18.
Moehler, S., W. Seifert, I. Appenzeller, & B. Muschielok. (1995). The FORS instrument for the ESO VLT. 53. 149.
19.
Moehler, S., T. Richtler, K. S. de Boer, R.‐J. Dettmar, & U. Heber. (1990). Hot subluminous stars at high galactic latitudes. I, Spectra and Strömgren photometry. Astronomy & Astrophysics Supplement Series. 86(1). 53–74. 4 indexed citations
20.
Heber, U., S. Dreizler, K. S. de Boer, S. Moehler, & T. Richtler. (1988). Spectroscopy of helium-rich subluminous O and B stars.. 1. 16. 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.

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