T. O. B. Schmidt

2.4k total citations
39 papers, 503 citations indexed

About

T. O. B. Schmidt is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, T. O. B. Schmidt has authored 39 papers receiving a total of 503 indexed citations (citations by other indexed papers that have themselves been cited), including 38 papers in Astronomy and Astrophysics, 11 papers in Instrumentation and 3 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in T. O. B. Schmidt's work include Stellar, planetary, and galactic studies (38 papers), Astrophysics and Star Formation Studies (31 papers) and Astro and Planetary Science (23 papers). T. O. B. Schmidt is often cited by papers focused on Stellar, planetary, and galactic studies (38 papers), Astrophysics and Star Formation Studies (31 papers) and Astro and Planetary Science (23 papers). T. O. B. Schmidt collaborates with scholars based in Germany, Chile and United States. T. O. B. Schmidt's co-authors include R. Neuhäuser, M. Mugrauer, N. Vogt, Andreas Seifahrt, A. Bedalov, C. Ginski, Misato Fukagawa, Guillermo Torres, S. Müller and T. Löhne 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

T. O. B. Schmidt

37 papers receiving 474 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
T. O. B. Schmidt Germany 15 492 134 19 16 15 39 503
R. Petrucci Argentina 8 297 0.6× 132 1.0× 12 0.6× 10 0.6× 15 1.0× 9 304
Eric Stempels United States 8 349 0.7× 101 0.8× 14 0.7× 12 0.8× 7 0.5× 73 357
Mark J. Pecaut United States 7 438 0.9× 118 0.9× 20 1.1× 9 0.6× 13 0.9× 10 457
P. Székely Hungary 10 285 0.6× 118 0.9× 10 0.5× 26 1.6× 14 0.9× 24 299
Н. П. Иконникова Russia 11 333 0.7× 128 1.0× 11 0.6× 17 1.1× 10 0.7× 72 340
A. Milone Brazil 8 254 0.5× 118 0.9× 12 0.6× 25 1.6× 11 0.7× 17 268
C. Saffe Argentina 12 426 0.9× 127 0.9× 26 1.4× 31 1.9× 10 0.7× 37 449
J. F. Gameiro Portugal 13 629 1.3× 107 0.8× 49 2.6× 14 0.9× 18 1.2× 35 633
Mercedes López‐Morales United States 6 373 0.8× 196 1.5× 9 0.5× 7 0.4× 16 1.1× 8 377
María-Fernanda Nieva Germany 5 340 0.7× 126 0.9× 20 1.1× 12 0.8× 12 0.8× 8 346

Countries citing papers authored by T. O. B. Schmidt

Since Specialization
Citations

This map shows the geographic impact of T. O. B. Schmidt'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. O. B. Schmidt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. O. B. Schmidt more than expected).

Fields of papers citing papers by T. O. B. Schmidt

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by T. O. B. Schmidt. 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. O. B. Schmidt. The network helps show where T. O. B. Schmidt may publish in the future.

Co-authorship network of co-authors of T. O. B. Schmidt

This figure shows the co-authorship network connecting the top 25 collaborators of T. O. B. Schmidt. A scholar is included among the top collaborators of T. O. B. Schmidt 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. O. B. Schmidt. T. O. B. Schmidt 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.
Obrzud, Ewelina, T. O. B. Schmidt, F. Bouchy, et al.. (2024). Astrocomb for the Near Infra-Red Planet Searcher (NIRPS). 10–10. 1 indexed citations
2.
Marleau, Gabriel-Dominique, Yuhiko Aoyama, R. Kuiper, et al.. (2021). Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at Hα. Astronomy and Astrophysics. 657. A38–A38. 31 indexed citations
3.
Czesla, S., et al.. (2019). X-ray emission in the enigmatic CVSO 30 system. Springer Link (Chiba Institute of Technology). 2 indexed citations
4.
Eiff, M. Ammler‐von, A. Bedalov, M. Mugrauer, et al.. (2016). Coronagraphic search for wide substellar companions among members of the Ursa Major moving group. Astronomy and Astrophysics. 591. A84–A84. 3 indexed citations
5.
Schmidt, T. O. B., R. Neuhäuser, César Briceño, et al.. (2016). Direct Imaging discovery of a second planet candidate around the possibly transiting planet host CVSO 30. Springer Link (Chiba Institute of Technology). 6 indexed citations
6.
Khalafinejad, S., C. von Essen, H. J. Hoeijmakers, et al.. (2016). Exoplanetary atmospheric sodium revealed by orbital motion. Astronomy and Astrophysics. 598. A131–A131. 31 indexed citations
7.
Schmidt, T. O. B., M. Mugrauer, R. Neuhäuser, et al.. (2014). First spectroscopic observations of the substellar companion of the young debris disk star PZ Telescopii. Springer Link (Chiba Institute of Technology). 9 indexed citations
8.
Eiff, M. Ammler‐von, M. Mugrauer, Christian Adam, et al.. (2013). The Hercules-Lyra association revisited. Astronomy and Astrophysics. 556. A53–A53. 23 indexed citations
9.
Schmidt, T. O. B., et al.. (2013). New companions in the stellar systems of DI Cha, Sz 22, CHXR 32, and Cha Hα5 in the Chamaeleon I star-forming region. Astronomy and Astrophysics. 557. A80–A80. 11 indexed citations
10.
Vogt, N., T. O. B. Schmidt, R. Neuhäuser, et al.. (2012). Astrometric confirmation of young low-mass binaries and multiple systems in the Chamaeleon star-forming regions. Springer Link (Chiba Institute of Technology). 17 indexed citations
11.
Maciejewski, G., R. Neuhäuser, St. Raetz, et al.. (2011). A search for transit timing variation. Springer Link (Chiba Institute of Technology).
12.
Neuhäuser, R., C. Ginski, T. O. B. Schmidt, & M. Mugrauer. (2011). Further deep imaging of HR 7329 A (η Tel A) and its brown dwarf companion B★. Monthly Notices of the Royal Astronomical Society. 416(2). 1430–1435. 20 indexed citations
13.
Mugrauer, M., N. Vogt, R. Neuhäuser, & T. O. B. Schmidt. (2010). Direct detection of a substellar companion to the young nearby star PZ Telescopii. Springer Link (Chiba Institute of Technology). 18 indexed citations
14.
Neuhäuser, R., T. O. B. Schmidt, V. Hambaryan, & N. Vogt. (2009). Orbital motion of the young brown dwarf companion TWA 5 B?. Springer Link (Chiba Institute of Technology). 9 indexed citations
15.
Krivov, A. V., et al.. (2009). A possible architecture of the planetary system HR 8799. Springer Link (Chiba Institute of Technology). 46 indexed citations
16.
Schmidt, T. O. B., R. Neuhäuser, Andreas Seifahrt, et al.. (2008). Direct evidence of a sub-stellar companion around CT Chamaeleontis. Springer Link (Chiba Institute of Technology). 36 indexed citations
17.
Neuhäuser, R., M. Mugrauer, Andreas Seifahrt, T. O. B. Schmidt, & N. Vogt. (2008). Astrometric and photometric monitoring of GQ Lupi and its sub-stellar companion. Astronomy and Astrophysics. 484(1). 281–291. 41 indexed citations
18.
Broeg, C., T. O. B. Schmidt, E. W. Guenther, et al.. (2007). Rotational period of GQ Lupi. Astronomy and Astrophysics. 468(3). 1039–1044. 17 indexed citations
19.
Schmidt, T. O. B., E. W. Guenther, A. P. Hatzes, et al.. (2005). A new Doppler image of the weak-line T Tauri star V410 Tauri.. Astronomische Nachrichten. 326. 667–667. 3 indexed citations
20.
Schulz, A., et al.. (1981). Polarization of starlight in M 17.. A&A. 95. 94–99. 2 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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