O. Marggraf

3.3k total citations
8 papers, 82 citations indexed

About

O. Marggraf is a scholar working on Astronomy and Astrophysics, Aerospace Engineering and Electrical and Electronic Engineering. According to data from OpenAlex, O. Marggraf has authored 8 papers receiving a total of 82 indexed citations (citations by other indexed papers that have themselves been cited), including 4 papers in Astronomy and Astrophysics, 2 papers in Aerospace Engineering and 2 papers in Electrical and Electronic Engineering. Recurrent topics in O. Marggraf's work include Stellar, planetary, and galactic studies (3 papers), CCD and CMOS Imaging Sensors (2 papers) and Galaxies: Formation, Evolution, Phenomena (2 papers). O. Marggraf is often cited by papers focused on Stellar, planetary, and galactic studies (3 papers), CCD and CMOS Imaging Sensors (2 papers) and Galaxies: Formation, Evolution, Phenomena (2 papers). O. Marggraf collaborates with scholars based in Germany, United States and Netherlands. O. Marggraf's co-authors include R. Massey, T. Schrabback, H. Israel, M. Cropper, Thibaut Prod’homme, O. Cordes, S.-M Niemi, David Hall, L. Miller and Harald Bluhm and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Digital Access to Libraries (Université catholique de Louvain (UCL), l'Université de Namur (UNamur) and the Université Saint-Louis (USL-B)).

In The Last Decade

O. Marggraf

7 papers receiving 81 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
O. Marggraf Germany 6 54 34 23 20 19 8 82
S.-M Niemi United Kingdom 3 46 0.9× 29 0.9× 23 1.0× 22 1.1× 20 1.1× 8 71
Roger Smith United States 5 46 0.9× 23 0.7× 32 1.4× 15 0.8× 23 1.2× 7 78
Daigo Tomono Japan 6 84 1.6× 20 0.6× 34 1.5× 6 0.3× 31 1.6× 17 115
M. C. Runyan United States 5 53 1.0× 28 0.8× 18 0.8× 10 0.5× 16 0.8× 10 86
S. Deiries Germany 5 31 0.6× 39 1.1× 18 0.8× 27 1.4× 14 0.7× 12 75
Ralf Kohley Spain 5 28 0.5× 27 0.8× 14 0.6× 20 1.0× 17 0.9× 15 64
Jason Ray United States 6 45 0.8× 18 0.5× 12 0.5× 24 1.2× 9 0.5× 12 74
C. Crowley Spain 4 45 0.8× 39 1.1× 10 0.4× 18 0.9× 26 1.4× 11 78
U. Grözinger Germany 5 21 0.4× 24 0.7× 26 1.1× 10 0.5× 13 0.7× 18 48
V. Cessa Switzerland 5 58 1.1× 27 0.8× 17 0.7× 18 0.9× 20 1.1× 8 87

Countries citing papers authored by O. Marggraf

Since Specialization
Citations

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

Fields of papers citing papers by O. Marggraf

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of O. Marggraf

This figure shows the co-authorship network connecting the top 25 collaborators of O. Marggraf. A scholar is included among the top collaborators of O. Marggraf 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 O. Marggraf. O. Marggraf is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

8 of 8 papers shown
1.
Scognamiglio, Diana, T. Schrabback, M. Tewes, et al.. (2025). Euclid preparation. LX. The use of HST images as input for weak-lensing image simulations. Astronomy and Astrophysics.
2.
Schrabback, T., S. Bocquet, Martin Sommer, et al.. (2022). Extending empirical constraints on the SZ–mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at z ≳ 1. Astronomy and Astrophysics. 668. A18–A18. 5 indexed citations
3.
Gillis, B., T. Schrabback, O. Marggraf, et al.. (2020). Validation of PSF models for HST and other space-based observations. Monthly Notices of the Royal Astronomical Society. 496(4). 5017–5038. 6 indexed citations
4.
Israel, H., R. Massey, Thibaut Prod’homme, et al.. (2015). How well can charge transfer inefficiency be corrected? A parameter sensitivity study for iterative correction. Monthly Notices of the Royal Astronomical Society. 453(1). 561–580. 11 indexed citations
5.
Moser, Albert, et al.. (2015). Ergebnisse der FNN-Studie zu neuen Verfahren der statischen Spannungshaltung. RWTH Publications (RWTH Aachen). 5 indexed citations
6.
Kundt, Wolfgang & O. Marggraf. (2014). Physikalische Mythen auf dem Prüfstand. Digital Access to Libraries (Université catholique de Louvain (UCL), l'Université de Namur (UNamur) and the Université Saint-Louis (USL-B)). 2 indexed citations
7.
Massey, R., T. Schrabback, O. Cordes, et al.. (2014). An improved model of charge transfer inefficiency and correction algorithm for the Hubble Space Telescope. Monthly Notices of the Royal Astronomical Society. 439(1). 887–907. 44 indexed citations
8.
Bluhm, Harald, K. S. de Boer, O. Marggraf, & P. Richter. (2001). ORFEUS echelle spectra: Molecular hydrogen in disk, IVC, and HVC gas in front of the LMC. Astronomy and Astrophysics. 367(1). 299–310. 9 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026