H. M. Schmid

5.7k total citations
74 papers, 1.2k citations indexed

About

H. M. Schmid is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, H. M. Schmid has authored 74 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 68 papers in Astronomy and Astrophysics, 26 papers in Instrumentation and 10 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in H. M. Schmid's work include Stellar, planetary, and galactic studies (58 papers), Astrophysics and Star Formation Studies (35 papers) and Astronomy and Astrophysical Research (26 papers). H. M. Schmid is often cited by papers focused on Stellar, planetary, and galactic studies (58 papers), Astrophysics and Star Formation Studies (35 papers) and Astronomy and Astrophysical Research (26 papers). H. M. Schmid collaborates with scholars based in Switzerland, Germany and Netherlands. H. M. Schmid's co-authors include F. Joos, E. Buenzli, H. Avenhaus, Sascha P. Quanz, R. Aznar Cuadrado, S. K. Solanki, R. Napiwotzki, Hans H. Schild, S. Jordan and A. Garufi 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

H. M. Schmid

71 papers receiving 1.2k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
H. M. Schmid Switzerland 19 1.1k 203 119 119 103 74 1.2k
Don J. Lindler United States 18 1.1k 1.0× 229 1.1× 83 0.7× 85 0.7× 114 1.1× 75 1.2k
Peter M. Onaka United States 11 1.3k 1.2× 297 1.5× 126 1.1× 102 0.9× 105 1.0× 32 1.5k
M. Fridlund Netherlands 20 1.2k 1.1× 295 1.5× 105 0.9× 59 0.5× 85 0.8× 80 1.3k
H. U. Käufl Germany 16 668 0.6× 198 1.0× 75 0.6× 113 0.9× 139 1.3× 59 787
Aki Roberge United States 24 1.7k 1.5× 204 1.0× 179 1.5× 264 2.2× 168 1.6× 89 1.8k
John Canfield United States 8 711 0.6× 269 1.3× 105 0.9× 89 0.7× 68 0.7× 8 832
Andrew Skemer United States 17 873 0.8× 276 1.4× 204 1.7× 99 0.8× 108 1.0× 80 967
G. Duvert France 16 921 0.8× 211 1.0× 115 1.0× 144 1.2× 51 0.5× 70 987
Toshihiko Tanabé Japan 17 994 0.9× 305 1.5× 76 0.6× 97 0.8× 69 0.7× 64 1.1k
John H. Debes United States 19 1.3k 1.1× 245 1.2× 87 0.7× 79 0.7× 35 0.3× 89 1.3k

Countries citing papers authored by H. M. Schmid

Since Specialization
Citations

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

Fields of papers citing papers by H. M. Schmid

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H. M. Schmid. 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 H. M. Schmid. The network helps show where H. M. Schmid may publish in the future.

Co-authorship network of co-authors of H. M. Schmid

This figure shows the co-authorship network connecting the top 25 collaborators of H. M. Schmid. A scholar is included among the top collaborators of H. M. Schmid 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 H. M. Schmid. H. M. Schmid 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.
Kamath, D., et al.. (2024). Multiwavelength high-resolution polarimetric imaging of second-generation disc around post-AGB binary IRAS 08544–4431 with SPHERE. Monthly Notices of the Royal Astronomical Society. 535(2). 1763–1777. 4 indexed citations
2.
Guidi, Greta, Andrea Isella, L. Testi, et al.. (2022). Distribution of solids in the rings of the HD 163296 disk: a multiwavelength study. Astronomy and Astrophysics. 664. A137–A137. 45 indexed citations
3.
Huélamo, N., G. Chauvin, I. Mendigutía, et al.. (2022). Searching for Hα-emitting sources in the gaps of five transitional disks. Astronomy and Astrophysics. 668. A138–A138. 18 indexed citations
4.
Schmid, H. M., et al.. (2021). Quantitative polarimetry of the disk around HD 169142. Springer Link (Chiba Institute of Technology). 12 indexed citations
5.
Engler, N., A. Boccaletti, H. M. Schmid, et al.. (2019). Investigating the presence of two belts in the HD 15115 system. Springer Link (Chiba Institute of Technology). 13 indexed citations
6.
Engler, N., H. M. Schmid, Sascha P. Quanz, H. Avenhaus, & A. Bazzon. (2018). Detection of scattered light from the hot dust in HD 172555. Springer Link (Chiba Institute of Technology). 11 indexed citations
7.
Garufi, A., G. Meeus, M. Benisty, et al.. (2017). . Springer Link (Chiba Institute of Technology). 46 indexed citations
8.
Lovis, C., I. A. G. Snellen, D. Mouillet, et al.. (2017). Atmospheric characterization of Proxima b by coupling the SPHERE high-contrast imager to the ESPRESSO spectrograph. Astronomy and Astrophysics. 599. A16–A16. 70 indexed citations
9.
Khouri, T., M. Maercker, L. B. F. M. Waters, et al.. (2016). Study of the inner dust envelope and stellar photosphere of the AGB star R Doradus using SPHERE/ZIMPOL. Astronomy and Astrophysics. 591. A70–A70. 59 indexed citations
10.
Garufi, A., Sascha P. Quanz, H. M. Schmid, et al.. (2014). Shadows and cavities in protoplanetary disks: HD 163296, HD 141569A, and HD 150193A in polarized light. Springer Link (Chiba Institute of Technology). 30 indexed citations
11.
Garufi, A., Sascha P. Quanz, H. Avenhaus, et al.. (2013). Small vs. large dust grains in transitional disks: do different cavity sizes indicate a planet?. Springer Link (Chiba Institute of Technology). 109 indexed citations
12.
Quanz, Sascha P., H. M. Schmid, Stephan M. Birkmann, et al.. (2011). Resolving the Inner Regions of Circumstellar Discs with VLT/NACO Polarimetric Differential Imaging. Max Planck Institute for Plasma Physics. 146. 25–27. 1 indexed citations
13.
Schmid, H. M., et al.. (2007). Polarimetry of Solar System Gaseous Planets. Msngr. 130. 27–31. 2 indexed citations
14.
Joos, F. & H. M. Schmid. (2006). Limb polarization of Uranus and Neptune. Astronomy and Astrophysics. 463(3). 1201–1210. 14 indexed citations
15.
Klose, S., E. Palazzi, N. Masetti, et al.. (2004). Prospects for multiwavelength polarization observations of GRB afterglows and the case GRB 030329. Max Planck Institute for Plasma Physics.
16.
Gisler, D. & H. M. Schmid. (2003). Non-solar Applications with the ZIMPOL Polarimeter. ASPC. 307. 58. 1 indexed citations
17.
Kaufer, A., O. Stahl, B. Wolf, et al.. (2002). The eclipsing hypergiant R 81 (B2.5Ia-O) in the Large Magellanic Cloud. Astronomy and Astrophysics. 389(3). 931–944. 9 indexed citations
18.
Schmid, H. M.. (1998). Raman Scattering and the Geometric Structure of Symbiotic Stars. 11. 297. 1 indexed citations
19.
Nussbaumer, H., et al.. (1991). Temperature and luminosity of hot components in symbiotic stars.. 248(2). 458–474. 11 indexed citations
20.
Hansen, H.‐J. & H. M. Schmid. (1970). Aromatische sigmatropische H-Verschiebungen und Claisen-Umlagerungen. CHIMIA International Journal for Chemistry. 24(3). 89–89.

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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