E. M. Carlson

1.4k total citations
8 papers, 275 citations indexed

About

E. M. Carlson is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, E. M. Carlson has authored 8 papers receiving a total of 275 indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Nuclear and High Energy Physics, 5 papers in Astronomy and Astrophysics and 1 paper in Atomic and Molecular Physics, and Optics. Recurrent topics in E. M. Carlson's work include Dark Matter and Cosmic Phenomena (8 papers), Astrophysics and Cosmic Phenomena (7 papers) and Galaxies: Formation, Evolution, Phenomena (4 papers). E. M. Carlson is often cited by papers focused on Dark Matter and Cosmic Phenomena (8 papers), Astrophysics and Cosmic Phenomena (7 papers) and Galaxies: Formation, Evolution, Phenomena (4 papers). E. M. Carlson collaborates with scholars based in United States, Netherlands and Germany. E. M. Carlson's co-authors include Stefano Profumo, Tim Linden, T. Jeltema, Alejandro Ibarra, Adam Coogan, Sebastian Wild, Dan Hooper and Christoph Weniger and has published in prestigious journals such as Physical Review Letters, Physical review. D and Journal of Cosmology and Astroparticle Physics.

In The Last Decade

E. M. Carlson

8 papers receiving 268 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
E. M. Carlson United States 7 258 186 12 7 6 8 275
E. Moulin France 10 338 1.3× 210 1.1× 22 1.8× 7 1.0× 9 1.5× 41 350
Sarah Recchia Italy 11 294 1.1× 229 1.2× 11 0.9× 3 0.4× 4 0.7× 19 329
Louis Yang Japan 8 169 0.7× 151 0.8× 15 1.3× 4 0.6× 8 1.3× 11 186
Heling Deng United States 7 198 0.8× 246 1.3× 20 1.7× 12 1.7× 3 0.5× 12 265
D. Albornoz Vásquez France 9 246 1.0× 185 1.0× 10 0.8× 3 0.4× 3 0.5× 10 279
Wanlei Guo China 11 465 1.8× 188 1.0× 21 1.8× 7 1.0× 4 0.7× 29 472
F. Krennrich United States 6 230 0.9× 194 1.0× 7 0.6× 9 1.3× 4 0.7× 23 256
S. V. Demidov Russia 9 198 0.8× 114 0.6× 20 1.7× 11 1.6× 2 0.3× 25 214
Tonia M. Venters United States 10 276 1.1× 171 0.9× 4 0.3× 7 1.0× 3 0.5× 30 291
Jennifer M. Siegal‐Gaskins United States 10 402 1.6× 271 1.5× 8 0.7× 14 2.0× 4 0.7× 17 410

Countries citing papers authored by E. M. Carlson

Since Specialization
Citations

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

Fields of papers citing papers by E. M. Carlson

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by E. M. Carlson. 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 E. M. Carlson. The network helps show where E. M. Carlson may publish in the future.

Co-authorship network of co-authors of E. M. Carlson

This figure shows the co-authorship network connecting the top 25 collaborators of E. M. Carlson. A scholar is included among the top collaborators of E. M. Carlson 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 E. M. Carlson. E. M. Carlson 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.
Carlson, E. M., Stefano Profumo, & Tim Linden. (2016). Cosmic-Ray Injection from Star-Forming Regions. Physical Review Letters. 117(11). 111101–111101. 23 indexed citations
2.
Carlson, E. M., Tim Linden, & Stefano Profumo. (2016). Improved cosmic-ray injection models and the Galactic Center gamma-ray excess. Physical review. D. 94(6). 35 indexed citations
3.
Carlson, E. M., Dan Hooper, & Tim Linden. (2015). Improving the sensitivity of gamma-ray telescopes to dark matter annihilation in dwarf spheroidal galaxies. Physical review. D. Particles, fields, gravitation, and cosmology. 91(6). 11 indexed citations
4.
Carlson, E. M., T. Jeltema, & Stefano Profumo. (2015). Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus. Journal of Cosmology and Astroparticle Physics. 2015(2). 9–9. 47 indexed citations
5.
Carlson, E. M. & Stefano Profumo. (2015). When dark matter interacts with cosmic rays or interstellar matter: A morphological study. Physical review. D. Particles, fields, gravitation, and cosmology. 92(6). 5 indexed citations
6.
Carlson, E. M., Adam Coogan, Tim Linden, et al.. (2014). Antihelium from dark matter. Physical review. D. Particles, fields, gravitation, and cosmology. 89(7). 32 indexed citations
7.
Carlson, E. M. & Stefano Profumo. (2014). Cosmic ray protons in the inner Galaxy and the Galactic Center gamma-ray excess. Physical review. D. Particles, fields, gravitation, and cosmology. 90(2). 114 indexed citations
8.
Carlson, E. M., Tim Linden, Stefano Profumo, & Christoph Weniger. (2013). Clustering analysis of the morphology of the 130 GeV gamma-ray feature. Physical review. D. Particles, fields, gravitation, and cosmology. 88(4). 8 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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