D. Eckert

9.5k total citations
123 papers, 3.0k citations indexed

About

D. Eckert is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, D. Eckert has authored 123 papers receiving a total of 3.0k indexed citations (citations by other indexed papers that have themselves been cited), including 115 papers in Astronomy and Astrophysics, 39 papers in Nuclear and High Energy Physics and 34 papers in Instrumentation. Recurrent topics in D. Eckert's work include Galaxies: Formation, Evolution, Phenomena (89 papers), Astrophysical Phenomena and Observations (50 papers) and Astronomy and Astrophysical Research (34 papers). D. Eckert is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (89 papers), Astrophysical Phenomena and Observations (50 papers) and Astronomy and Astrophysical Research (34 papers). D. Eckert collaborates with scholars based in Switzerland, Italy and United States. D. Eckert's co-authors include S. Ettori, S. Molendi, F. Vazza, S. Paltani, M. Rossetti, F. Gastaldello, É. Pointecouteau, D. Malyshev, A. Neronov and M. Brüggen and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and Journal of the American Statistical Association.

In The Last Decade

D. Eckert

113 papers receiving 2.8k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. Eckert Switzerland 35 2.8k 1.2k 807 154 74 123 3.0k
F. Gastaldello Italy 31 2.9k 1.0× 1.2k 1.0× 641 0.8× 94 0.6× 93 1.3× 121 3.0k
Sebastiano Cantalupo Switzerland 34 3.1k 1.1× 968 0.8× 1000 1.2× 108 0.7× 49 0.7× 103 3.2k
I. Hook United Kingdom 27 3.0k 1.1× 755 0.7× 975 1.2× 120 0.8× 38 0.5× 88 3.1k
R. Srianand India 38 4.4k 1.5× 997 0.9× 667 0.8× 268 1.7× 155 2.1× 192 4.6k
M. Sereno Italy 32 2.6k 0.9× 900 0.8× 636 0.8× 185 1.2× 130 1.8× 114 2.7k
Patrick L. Kelly United States 29 3.0k 1.1× 1.0k 0.9× 680 0.8× 117 0.8× 52 0.7× 69 3.1k
A. Evans United States 29 3.1k 1.1× 910 0.8× 528 0.7× 128 0.8× 60 0.8× 131 3.1k
É. Pointecouteau France 25 2.8k 1.0× 962 0.8× 783 1.0× 63 0.4× 105 1.4× 79 2.9k
Jayaram N. Chengalur India 31 3.0k 1.1× 807 0.7× 763 0.9× 135 0.9× 77 1.0× 126 3.1k
E. M. Sadler Australia 35 4.3k 1.5× 2.0k 1.7× 889 1.1× 98 0.6× 43 0.6× 151 4.4k

Countries citing papers authored by D. Eckert

Since Specialization
Citations

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

Fields of papers citing papers by D. Eckert

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Eckert

This figure shows the co-authorship network connecting the top 25 collaborators of D. Eckert. A scholar is included among the top collaborators of D. Eckert 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 D. Eckert. D. Eckert 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.
Seppi, R., D. Eckert, A. Finoguenov, et al.. (2025). Modelling the selection of galaxy groups with end-to-end simulations. Astronomy and Astrophysics. 699. A206–A206.
2.
Rasia, Elena, S. Borgani, Veronica Biffi, et al.. (2025). The Three Hundred Project: Modeling baryon and hot-gas fraction evolution in simulated clusters. Astronomy and Astrophysics. 702. A182–A182.
3.
Clerc, N., É. Pointecouteau, D. Eckert, et al.. (2024). CHEX-MATE: Turbulence in the intra-cluster medium from X-ray surface brightness fluctuations. Astronomy and Astrophysics. 687. A58–A58. 9 indexed citations
4.
Molendi, S., S. Ghizzardi, S. De Grandi, et al.. (2024). Metal enrichment: The apex accretor perspective. Astronomy and Astrophysics. 685. A88–A88. 1 indexed citations
5.
Clerc, N., et al.. (2023). Investigating the turbulent hot gas in X-COP galaxy clusters. Astronomy and Astrophysics. 673. A91–A91. 12 indexed citations
6.
Bourdin, H., Federico De Luca, P. Mazzotta, et al.. (2023). CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters. Astronomy and Astrophysics. 678. A181–A181. 1 indexed citations
7.
Ettori, S., L. Lovisari, I. Bartalucci, et al.. (2022). . IRIS UNIMORE (University of Modena and Reggio Emilia). 27 indexed citations
8.
Ghizzardi, S., S. Molendi, R. F. J. van der Burg, et al.. (2021). Iron in X-COP: Tracing enrichment in cluster outskirts with high accuracy abundance profiles (. Springer Link (Chiba Institute of Technology). 24 indexed citations
9.
Ge, Chong, Ruo-Yu Liu, Ming Sun, et al.. (2020). Chandra and XMM–Newton observations of A2256: cold fronts, merger shocks, and constraint on the IC emission. Monthly Notices of the Royal Astronomical Society. 497(4). 4704–4717. 9 indexed citations
10.
Jauzac, Mathilde, R. Massey, David Harvey, et al.. (2020). The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451−03. Monthly Notices of the Royal Astronomical Society. 496(3). 4032–4050. 16 indexed citations
11.
Grandi, S. De, S. Ghizzardi, M. Rossetti, et al.. (2019). Growth and disruption in the Lyra complex. Springer Link (Chiba Institute of Technology). 3 indexed citations
12.
Ghirardini, V., S. Ettori, D. Eckert, & S. Molendi. (2019). Polytropic state of the intracluster medium in the X-COP cluster sample. Springer Link (Chiba Institute of Technology). 11 indexed citations
13.
Green, Sheridan B, Michelle Ntampaka, Daisuke Nagai, et al.. (2019). Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning. The Astrophysical Journal. 884(1). 33–33. 22 indexed citations
14.
Gaspari, M., D. Eckert, S. Ettori, et al.. (2019). The X-Ray Halo Scaling Relations of Supermassive Black Holes. The Astrophysical Journal. 884(2). 169–169. 60 indexed citations
15.
Venturi, T., M. Rossetti, G. Brunetti, et al.. (2017). The two-component giant radio halo in the galaxy cluster Abell 2142. Astronomy and Astrophysics. 603. A125–A125. 44 indexed citations
16.
Pavan, L., G. Pühlhofer, P. Bordas, et al.. (2016). Closer view of the IGR J11014-6103 outflows. Springer Link (Chiba Institute of Technology). 29 indexed citations
17.
Tchernin, C., et al.. (2015). Reconstructing the projected gravitational potential of Abell 1689 from X-ray measurements. Springer Link (Chiba Institute of Technology). 5 indexed citations
18.
Rossetti, M., D. Eckert, S. De Grandi, et al.. (2013). Abell 2142 at large scales: An extreme case for sloshing?. Springer Link (Chiba Institute of Technology). 44 indexed citations
19.
Eckert, D., A. Neronov, T. J.-L. Courvoisier, & N. Produit. (2007). South-West extension of the hard X-ray emission from the Coma cluster. Springer Link (Chiba Institute of Technology). 12 indexed citations
20.
Eckert, D., et al.. (2005). IGR J01583+6713, a new hard X-ray transient discovered by INTEGRAL. The astronomer's telegram. 672. 1. 1 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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