T. Lanz

6.1k total citations · 2 hit papers
103 papers, 4.0k citations indexed

About

T. Lanz is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, T. Lanz has authored 103 papers receiving a total of 4.0k indexed citations (citations by other indexed papers that have themselves been cited), including 93 papers in Astronomy and Astrophysics, 44 papers in Instrumentation and 13 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in T. Lanz's work include Stellar, planetary, and galactic studies (81 papers), Astrophysics and Star Formation Studies (53 papers) and Astronomy and Astrophysical Research (44 papers). T. Lanz is often cited by papers focused on Stellar, planetary, and galactic studies (81 papers), Astrophysics and Star Formation Studies (53 papers) and Astronomy and Astrophysical Research (44 papers). T. Lanz collaborates with scholars based in United States, France and United Kingdom. T. Lanz's co-authors include I. Hubený, I. Hubený, J.‐C. Bouret, D. J. Hillier, Sara R. Heap, D. J. Lennon, C. J. Evans, F. Martins, A. V. Sweigart and A. W. Fullerton and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

T. Lanz

102 papers receiving 3.9k citations

Hit Papers

Non-LTE line-blanketed model atmospheres of hot stars. 1:... 1995 2026 2005 2015 1995 2003 200 400 600

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
T. Lanz United States 30 3.8k 1.4k 208 191 148 103 4.0k
F. Wesemaël Canada 32 2.9k 0.8× 1.2k 0.9× 187 0.9× 170 0.9× 98 0.7× 123 3.1k
O. Kochukhov Sweden 39 4.4k 1.1× 1.1k 0.8× 177 0.9× 238 1.2× 71 0.5× 213 4.5k
Kátia Cunha United States 37 3.8k 1.0× 1.6k 1.1× 142 0.7× 96 0.5× 351 2.4× 151 4.0k
N. Przybilla Germany 33 3.1k 0.8× 1.2k 0.8× 174 0.8× 112 0.6× 104 0.7× 106 3.2k
I. Hubený United States 34 4.1k 1.1× 1.2k 0.8× 159 0.8× 142 0.7× 273 1.8× 114 4.3k
Douglas R. Gies United States 36 4.6k 1.2× 1.7k 1.2× 222 1.1× 341 1.8× 332 2.2× 185 4.8k
Hugh C. Harris United States 32 3.9k 1.0× 1.8k 1.3× 190 0.9× 286 1.5× 212 1.4× 118 4.0k
D. E. Winget United States 31 2.7k 0.7× 1.1k 0.8× 243 1.2× 185 1.0× 236 1.6× 123 3.0k
G. Fontaine Canada 40 4.9k 1.3× 2.3k 1.6× 277 1.3× 333 1.7× 136 0.9× 192 5.1k
P. E. Nissen Denmark 38 3.7k 1.0× 1.5k 1.1× 116 0.6× 116 0.6× 481 3.3× 106 3.9k

Countries citing papers authored by T. Lanz

Since Specialization
Citations

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

Fields of papers citing papers by T. Lanz

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of T. Lanz

This figure shows the co-authorship network connecting the top 25 collaborators of T. Lanz. A scholar is included among the top collaborators of T. Lanz 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. Lanz. T. Lanz 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.
Artaud, Géraldine, et al.. (2025). Final architecture of FrOGS, validation, and first results of GEO optical links with TELEO. 260–260. 1 indexed citations
2.
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
3.
Chièze, J.-P., et al.. (2019). New insight on accretion shocks onto young stellar objects. Astronomy and Astrophysics. 630. A84–A84. 6 indexed citations
4.
Vakili, F., T. Lanz, M. Langlois, et al.. (2017). Uncrowding R 136 from VLT/SPHERE extreme adaptive optics. Springer Link (Chiba Institute of Technology). 12 indexed citations
5.
Dessart, Luc, C. P. Gutiérrez, M. Hamuy, et al.. (2014). Type II Plateau supernovae as metallicity probes of the Universe. Monthly Notices of the Royal Astronomical Society. 440(2). 1856–1864. 22 indexed citations
6.
Ibgui, L., I. Hubený, T. Lanz, & C. Stehlé. (2013). IRIS: a generic three-dimensional radiative transfer code. Springer Link (Chiba Institute of Technology). 27 indexed citations
7.
Bouret, J.‐C., T. Lanz, F. Martins, et al.. (2013). Massive stars at low metallicity. Astronomy and Astrophysics. 555. A1–A1. 61 indexed citations
8.
Cunha, Kátia, I. Hubený, & T. Lanz. (2012). Chemical homogeneity in the Orion Association: Oxygen abundances of B stars. Springer Link (Chiba Institute of Technology). 1 indexed citations
9.
Hubený, I. & T. Lanz. (2011). TLUSTY: Stellar Atmospheres, Accretion Disks, and Spectroscopic Diagnostics. Astrophysics Source Code Library. 1 indexed citations
10.
Hubený, I. & T. Lanz. (2011). Synspec: General Spectrum Synthesis Program. Astrophysics Source Code Library. 21 indexed citations
11.
Marcolino, W. L. F., et al.. (2009). Analysis of Galactic late-type O dwarfs: more constraints on the weak wind problem. Springer Link (Chiba Institute of Technology). 94 indexed citations
12.
Manousakis, A., R. Walter, M. Audard, & T. Lanz. (2009). Pulsed thermal emission from the accreting pulsar XMMU J054134.7-682550. Astronomy and Astrophysics. 498(1). 217–222. 9 indexed citations
13.
Bouret, J.‐C., J.‐F. Donati, F. Martins, et al.. (2008). The weak magnetic field of the O9.7 supergiant ζ Orionis. 49 indexed citations
14.
Hunter, I., P. L. Dufton, S. J. Smartt, et al.. (2007). The VLT-FLAMES survey of massive stars: surface chemical compositions of B-type stars in the Magellanic Clouds. Springer Link (Chiba Institute of Technology). 102 indexed citations
15.
Moehler, S., S. Dreizler, T. Lanz, et al.. (2007). The hottest horizontal-branch stars in $\mathsf{\omega}$ Centauri. Late hot flasher vs. helium enrichment. Astronomy and Astrophysics. 475(2). L5–L8. 29 indexed citations
16.
Marco, Orsola De, et al.. (2004). First Evidence of Circumstellar Disks around Blue Straggler Stars. The Astrophysical Journal. 606(2). L151–L154. 17 indexed citations
17.
Lanz, T. & I. Hubený. (2003). Atomic Data in Non-LTE Model Stellar Atmospheres. 288. 117. 1 indexed citations
18.
Ryans, R. S. I., P. L. Dufton, W. R. J. Rolleston, et al.. (2003). An analysis of the optical spectra of the post-asymptotic giant branch stars LSIV -12 111 and HD 341617. Astronomy and Astrophysics. 401(3). 1119–1129. 47 indexed citations
19.
North, P., et al.. (1994). The nature of the F STR λ4077 stars. V. Spectroscopic data. Astronomy & Astrophysics Supplement Series. 103(2). 321–347. 1 indexed citations
20.
Lanz, T., et al.. (1990). Compilation of atomic oscillator strengths for carbon, nitrogen and oxygen ions - The beryllium isoelectronic sequence (C III, N IV, and O V). Astronomy & Astrophysics Supplement Series. 84(3). 563–600. 10 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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