S. Seitz

9.9k total citations
78 papers, 1.7k citations indexed

About

S. Seitz is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, S. Seitz has authored 78 papers receiving a total of 1.7k indexed citations (citations by other indexed papers that have themselves been cited), including 71 papers in Astronomy and Astrophysics, 33 papers in Instrumentation and 12 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in S. Seitz's work include Galaxies: Formation, Evolution, Phenomena (64 papers), Astronomy and Astrophysical Research (33 papers) and Stellar, planetary, and galactic studies (30 papers). S. Seitz is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (64 papers), Astronomy and Astrophysical Research (33 papers) and Stellar, planetary, and galactic studies (30 papers). S. Seitz collaborates with scholars based in Germany, United States and Italy. S. Seitz's co-authors include R. Bender, A. Riffeser, U. Hopp, D. Gruen, R. P. Saglia, Petra Schneider, Chien‐Hsiu Lee, B. Hoyle, Markus Michael Rau and D. Mehlert and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

S. Seitz

77 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. Seitz Germany 26 1.5k 660 200 162 77 78 1.7k
C. Tortora Italy 25 1.6k 1.0× 879 1.3× 248 1.2× 158 1.0× 106 1.4× 98 1.7k
E. Semboloni Netherlands 19 1.5k 1.0× 587 0.9× 372 1.9× 213 1.3× 66 0.9× 22 1.6k
J. P. Dietrich Germany 19 1.4k 0.9× 597 0.9× 332 1.7× 212 1.3× 53 0.7× 35 1.6k
Angus H. Wright Germany 22 1.3k 0.8× 564 0.9× 304 1.5× 108 0.7× 85 1.1× 70 1.4k
Huanyuan Shan China 21 1.2k 0.8× 489 0.7× 338 1.7× 109 0.7× 74 1.0× 83 1.3k
E. A. Valentijn Australia 24 1.7k 1.1× 796 1.2× 207 1.0× 99 0.6× 115 1.5× 105 1.9k
Hironao Miyatake Japan 23 1.7k 1.1× 719 1.1× 325 1.6× 218 1.3× 110 1.4× 61 1.8k
M. Kilbinger France 22 1.7k 1.1× 684 1.0× 370 1.9× 226 1.4× 101 1.3× 61 1.9k
J. Hartlap Germany 15 1.3k 0.9× 462 0.7× 261 1.3× 119 0.7× 61 0.8× 17 1.4k
Andrew P. Cooper United Kingdom 22 1.6k 1.1× 912 1.4× 188 0.9× 79 0.5× 51 0.7× 51 1.7k

Countries citing papers authored by S. Seitz

Since Specialization
Citations

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

Fields of papers citing papers by S. Seitz

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of S. Seitz. A scholar is included among the top collaborators of S. Seitz 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. Seitz. S. Seitz 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.
Barreira, Alexandre, et al.. (2023). Cosmology from the integrated shear 3-point correlation function: simulated likelihood analyses with machine-learning emulators. Journal of Cosmology and Astroparticle Physics. 2023(7). 40–40. 7 indexed citations
2.
Zitrin, Adi, S. Seitz, A. Monna, et al.. (2017). A Very Large (θE ≳ 40″) Strong Gravitational Lens Selected with the Sunyaev–Zel’dovich Effect: PLCK G287.0+32.9 (z = 0.38). The Astrophysical Journal Letters. 839(1). L11–L11. 7 indexed citations
3.
Gozaliasl, G., A. Finoguenov, Habib G. Khosroshahi, et al.. (2014). Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3-square-degree XMM coverage of CFHTLS. Springer Link (Chiba Institute of Technology). 17 indexed citations
4.
Gruen, D., S. Seitz, F. Brimioulle, et al.. (2014). Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys. Monthly Notices of the Royal Astronomical Society. 442(2). 1507–1544. 63 indexed citations
5.
Henze, M., W. Pietsch, F. Haberl, et al.. (2012). Supersoft X-rays reveal a classical nova in the M 31 globular cluster Bol 126. Astronomy and Astrophysics. 549. A120–A120. 10 indexed citations
6.
Lee, Chien‐Hsiu, A. Riffeser, S. Seitz, et al.. (2011). The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M 31 nova catalogue. Astronomy and Astrophysics. 537. A43–A43. 10 indexed citations
7.
Lee, Chien‐Hsiu, S. Seitz, A. Riffeser, & R. Bender. (2010). Finite-source and finite-lens effects in astrometric microlensing. Monthly Notices of the Royal Astronomical Society. 407(3). 1597–1608. 9 indexed citations
8.
Montalto, M., S. Seitz, A. Riffeser, et al.. (2009). Properties of M31. Astronomy and Astrophysics. 507(1). 283–300. 31 indexed citations
9.
Saglia, R. P., Maximilian Fabricius, R. Bender, et al.. (2009). The old and heavy bulge of M 31. Astronomy and Astrophysics. 509. A61–A61. 64 indexed citations
10.
Pietsch, W., F. Haberl, G. Sala, et al.. (2007). X-ray monitoring of optical novae in M 31 from July 2004 to February 2005. Astronomy and Astrophysics. 465(2). 375–392. 49 indexed citations
11.
Gabasch, A., U. Hopp, Georg Feulner, et al.. (2006). The evolution of the luminosity functions in the FORS deep field from low to high redshift. Astronomy and Astrophysics. 448(1). 101–121. 44 indexed citations
12.
Tapken, C., I. Appenzeller, A. Gabasch, et al.. (2006). Lyαemission galaxies at a redshift ofz ≈ 5.7 in the FORS deep field. Astronomy and Astrophysics. 455(1). 145–152. 19 indexed citations
13.
Fliri, J., A. Riffeser, S. Seitz, & R. Bender. (2005). The Wendelstein Calar Alto Pixellensing Project (WeCAPP): theM 31 variable star catalogue. Springer Link (Chiba Institute of Technology). 22 indexed citations
14.
Appenzeller, I., R. Bender, A. Böhm, et al.. (2004). Exploring Cosmic Evolution with the FORS Deep Field. Max Planck Institute for Plasma Physics. 116. 18–24. 4 indexed citations
15.
Gabasch, A., R. Bender, S. Seitz, et al.. (2004). The evolution of the luminosity functions in the FORS Deep Field from low to high redshift. Astronomy and Astrophysics. 421(1). 41–58. 90 indexed citations
16.
Böhm, A., B. Ziegler, R. P. Saglia, et al.. (2004). The Tully-Fisher relation at intermediate redshift. Astronomy and Astrophysics. 420(1). 97–114. 69 indexed citations
17.
Noll, Stefan, D. Mehlert, I. Appenzeller, et al.. (2004). The FORS Deep Field spectroscopic survey. Astronomy and Astrophysics. 418(3). 885–906. 46 indexed citations
18.
Barrena, R., A. Biviano, M. Ramella, E. Falco, & S. Seitz. (2002). The dynamical status of the cluster of galaxies 1E0657-56. Astronomy and Astrophysics. 386(3). 816–828. 61 indexed citations
19.
Mehlert, D., S. Seitz, R. P. Saglia, et al.. (2001). Gravitationally lensed high redshift galaxies in the field of 1E0657-56. Astronomy and Astrophysics. 379(1). 96–106. 14 indexed citations
20.
Seitz, S. & Petra Schneider. (2001). A new finite-field mass reconstruction algorithm. Astronomy and Astrophysics. 374(2). 740–745. 33 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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