Marco Selig

499 total citations
20 papers, 343 citations indexed

About

Marco Selig is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Statistical and Nonlinear Physics. According to data from OpenAlex, Marco Selig has authored 20 papers receiving a total of 343 indexed citations (citations by other indexed papers that have themselves been cited), including 7 papers in Astronomy and Astrophysics, 5 papers in Nuclear and High Energy Physics and 4 papers in Statistical and Nonlinear Physics. Recurrent topics in Marco Selig's work include Astrophysics and Cosmic Phenomena (4 papers), Dark Matter and Cosmic Phenomena (4 papers) and Radio Astronomy Observations and Technology (3 papers). Marco Selig is often cited by papers focused on Astrophysics and Cosmic Phenomena (4 papers), Dark Matter and Cosmic Phenomena (4 papers) and Radio Astronomy Observations and Technology (3 papers). Marco Selig collaborates with scholars based in Germany, Canada and United Kingdom. Marco Selig's co-authors include T. A. Enßlin, Niels Oppermann, M. R. Bell, H. Junklewitz, V. Vacca, Xiaoyuan Huang, M. Reinecke, Martin Greiner, Ulrich Gerland and Tiago Ramalho and has published in prestigious journals such as Scientific Reports, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

Marco Selig

17 papers receiving 331 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Marco Selig Germany 9 212 139 31 23 22 20 343
Niels Oppermann Germany 14 591 2.8× 274 2.0× 25 0.8× 35 1.5× 34 1.5× 26 730
M. Galassi United States 10 158 0.7× 75 0.5× 63 2.0× 25 1.1× 14 0.6× 57 349
Sihao Cheng United States 8 297 1.4× 47 0.3× 26 0.8× 21 0.9× 8 0.4× 16 357
E. Sánchez Spain 12 306 1.4× 120 0.9× 14 0.5× 24 1.0× 7 0.3× 43 413
Yichao Li China 14 524 2.5× 199 1.4× 76 2.5× 19 0.8× 45 2.0× 52 776
Miles Cranmer United States 12 209 1.0× 55 0.4× 111 3.6× 32 1.4× 14 0.6× 23 363
Devansh Agarwal United States 11 264 1.2× 44 0.3× 51 1.6× 65 2.8× 31 1.4× 18 485
V. B. Ryabov Japan 12 367 1.7× 67 0.5× 24 0.8× 69 3.0× 21 1.0× 55 525
Youling Yue China 13 603 2.8× 197 1.4× 19 0.6× 13 0.6× 93 4.2× 41 690
Itamar Reis Israel 8 219 1.0× 122 0.9× 35 1.1× 13 0.6× 49 2.2× 16 399

Countries citing papers authored by Marco Selig

Since Specialization
Citations

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

Fields of papers citing papers by Marco Selig

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Marco Selig

This figure shows the co-authorship network connecting the top 25 collaborators of Marco Selig. A scholar is included among the top collaborators of Marco Selig 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 Marco Selig. Marco Selig 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.
2.
Elsasser, Peter, Jakob Hildebrandt, Kathleen Meisel, et al.. (2024). Dynamics of bio-based carbon dioxide removal in Germany. Scientific Reports. 14(1). 20395–20395. 3 indexed citations
3.
Bestenlehner, J. M., T. A. Enßlin, M. Bergemann, et al.. (2024). Spectroscopic analysis of hot, massive stars in large spectroscopic surveys with de-idealized models. Monthly Notices of the Royal Astronomical Society. 528(4). 6735–6750. 4 indexed citations
4.
Junklewitz, H., M. R. Bell, Marco Selig, & T. A. Enßlin. (2016). RESOLVE: A new algorithm for aperture synthesis imaging of extended emission in radio astronomy. Springer Link (Chiba Institute of Technology). 42 indexed citations
5.
Vacca, V., Niels Oppermann, T. A. Enßlin, et al.. (2016). Using rotation measure grids to detect cosmological magnetic fields: A Bayesian approach. Astronomy and Astrophysics. 591. A13–A13. 21 indexed citations
6.
Selig, Marco, V. Vacca, Niels Oppermann, & T. A. Enßlin. (2016). The Denoised, Deconvolved, and Decomposed Fermi gamma-ray sky. Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015). 768–768. 1 indexed citations
7.
Huang, Xiaoyuan, T. A. Enßlin, & Marco Selig. (2016). Galactic dark matter search via phenomenological astrophysics modeling. Journal of Cosmology and Astroparticle Physics. 2016(4). 30–30. 26 indexed citations
8.
Selig, Marco & T. A. Enßlin. (2015). Denoising, deconvolving, and decomposing photon observations. Springer Link (Chiba Institute of Technology). 14 indexed citations
9.
Vacca, V., T. A. Enßlin, Marco Selig, et al.. (2015). Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era. 114–114. 4 indexed citations
10.
Dörn, Sebastian, et al.. (2015). Signal inference with unknown response: Calibration-uncertainty renormalized estimator. Physical Review E. 91(1). 13311–13311. 4 indexed citations
11.
Selig, Marco, V. Vacca, Niels Oppermann, & T. A. Enßlin. (2015). The denoised, deconvolved, and decomposedFermiγ-ray sky. Astronomy and Astrophysics. 581. A126–A126. 41 indexed citations
12.
Enßlin, T. A., et al.. (2014). Improving self-calibration. Physical Review E. 90(4). 43301–43301. 5 indexed citations
13.
Selig, Marco, V. Vacca, Niels Oppermann, & T. A. Enßlin. (2014). The Denoised, Deconvolved, and Decomposed Fermi $γ$-ray sky - An application of the D$^3$PO algorithm. MPG.PuRe (Max Planck Society). 581. 1–16. 27 indexed citations
14.
Selig, Marco, M. R. Bell, H. Junklewitz, et al.. (2013). NIFTY: A versatile Python library for signal inference. Astrophysics Source Code Library.
15.
Ramalho, Tiago, Marco Selig, Ulrich Gerland, & T. A. Enßlin. (2013). Simulation of stochastic network dynamics via entropic matching. Physical Review E. 87(2). 22719–22719. 6 indexed citations
16.
Selig, Marco, M. R. Bell, H. Junklewitz, et al.. (2013). NIFTY – Numerical Information Field Theory. Astronomy and Astrophysics. 554. A26–A26. 52 indexed citations
17.
Selig, Marco & T. A. Enßlin. (2013). D$^3$PO - Denoising, Deconvolving, and Decomposing Photon Observations. arXiv (Cornell University). 2 indexed citations
18.
Dörn, Sebastian, Niels Oppermann, Rishi Khatri, Marco Selig, & T. A. Enßlin. (2013). Fast and precise way to calculate the posterior for the local non-Gaussianity parameterfnlfrom cosmic microwave background observations. Physical review. D. Particles, fields, gravitation, and cosmology. 88(10). 3 indexed citations
19.
Oppermann, Niels, Marco Selig, M. R. Bell, & T. A. Enßlin. (2013). Reconstruction of Gaussian and log-normal fields with spectral smoothness. Physical Review E. 87(3). 79 indexed citations
20.
Selig, Marco, Niels Oppermann, & T. A. Enßlin. (2012). Improving stochastic estimates with inference methods: Calculating matrix diagonals. Physical Review E. 85(2). 21134–21134. 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.

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