S. Casanova

14.2k total citations
46 papers, 597 citations indexed

About

S. Casanova is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atmospheric Science. According to data from OpenAlex, S. Casanova has authored 46 papers receiving a total of 597 indexed citations (citations by other indexed papers that have themselves been cited), including 38 papers in Astronomy and Astrophysics, 36 papers in Nuclear and High Energy Physics and 2 papers in Atmospheric Science. Recurrent topics in S. Casanova's work include Astrophysics and Cosmic Phenomena (36 papers), Gamma-ray bursts and supernovae (23 papers) and Dark Matter and Cosmic Phenomena (22 papers). S. Casanova is often cited by papers focused on Astrophysics and Cosmic Phenomena (36 papers), Gamma-ray bursts and supernovae (23 papers) and Dark Matter and Cosmic Phenomena (22 papers). S. Casanova collaborates with scholars based in Germany, Poland and Ireland. S. Casanova's co-authors include S. Gabici, Felix A. Aharonian, T. Montmerle, J. Gregorio‐Hetem, F. Aharonian, Giada Peron, Elena Amato, Ruizhi Yang, E. L. Martín and B. L. Dingus and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

S. Casanova

41 papers receiving 579 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. Casanova Germany 14 508 420 29 15 11 46 597
E. Semkov Bulgaria 11 305 0.6× 181 0.4× 19 0.7× 11 0.7× 15 1.4× 42 334
A. Tappe United States 7 431 0.8× 181 0.4× 74 2.6× 39 2.6× 32 2.9× 12 452
K. L. Emig United States 10 270 0.5× 119 0.3× 25 0.9× 13 0.9× 15 1.4× 25 290
M. T. Rushton United Kingdom 11 346 0.7× 102 0.2× 16 0.6× 5 0.3× 19 1.7× 29 371
Hidetoshi Sano Japan 15 558 1.1× 310 0.7× 52 1.8× 40 2.7× 11 1.0× 82 598
A. G. Polatidis Sweden 8 353 0.7× 198 0.5× 19 0.7× 12 0.8× 9 0.8× 14 359
D. W. Kavars United States 7 366 0.7× 116 0.3× 35 1.2× 26 1.7× 10 0.9× 7 375
Marco Fatuzzo United States 11 435 0.9× 180 0.4× 31 1.1× 13 0.9× 36 3.3× 38 476
A. Tarchi Italy 16 627 1.2× 253 0.6× 88 3.0× 15 1.0× 11 1.0× 44 636
Y. Takahashi United States 8 243 0.5× 157 0.4× 51 1.8× 9 0.6× 8 0.7× 14 267

Countries citing papers authored by S. Casanova

Since Specialization
Citations

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

Fields of papers citing papers by S. Casanova

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of S. Casanova. A scholar is included among the top collaborators of S. Casanova 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. Casanova. S. Casanova 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.
Peron, Giada, S. Casanova, S. Gabici, Vardan Baghmanyan, & F. Aharonian. (2024). The contribution of winds from star clusters to the Galactic cosmic-ray population. Nature Astronomy. 8(4). 530–537. 10 indexed citations
2.
Angüner, E. O., G. Spengler, Elena Amato, & S. Casanova. (2023). Search for the Galactic accelerators of cosmic rays up to the knee with the Pevatron test statistic. Monthly Notices of the Royal Astronomical Society. 523(3). 4097–4112.
3.
Guevel, David Joseph, A. P. Beardmore, K. L. Page, et al.. (2023). Limits on Leptonic TeV Emission from the Cygnus Cocoon with Swift-XRT. The Astrophysical Journal. 950(2). 116–116. 3 indexed citations
4.
Baghmanyan, Vardan, D. Zargaryan, F. Aharonian, et al.. (2022). Detailed study of extended γ-ray morphology in the vicinity of the Coma cluster with Fermi Large Area Telescope. Monthly Notices of the Royal Astronomical Society. 516(1). 562–571. 15 indexed citations
5.
Amato, Elena & S. Casanova. (2021). On particle acceleration and transport in plasmas in the Galaxy: theory and observations. Journal of Plasma Physics. 87(1). 23 indexed citations
6.
Aharonian, F., et al.. (2020). Probing the sea of galactic cosmic rays with Fermi-LAT. Physical review. D. 101(8). 32 indexed citations
7.
Greus, F. Salesa & S. Casanova. (2019). Spectral and Morphological Studies of the Very High Energy Gamma-Ray Source 2HWC J1825-134. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019). 781–781. 1 indexed citations
8.
Casanova, S., et al.. (2019). Spectral and morphological study of the gamma radiation of the middle-aged supernova remnant HB 21. Astronomy and Astrophysics. 623. A86–A86. 11 indexed citations
9.
Nayerhoda, A., et al.. (2019). Gamma Ray Diffuse Emission from the GalacticPlane with HAWC Data. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019). 750–750. 2 indexed citations
10.
Klepser, S., F. Aharonian, E. O. Angüner, et al.. (2017). New insights into pulsar wind nebula evolution with H.E.S.S. I and II. AIP conference proceedings. 1792. 40012–40012.
11.
López-Coto, R., et al.. (2017). Constraining the Origin of Local Positrons with HAWC TeV Gamma-Ray Observations of Two Nearby Pulsar Wind Nebulae. OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information). 11–11. 1 indexed citations
12.
Aharonian, F., P. Bordas, S. Casanova, et al.. (2017). HESS J1826−130: A very hard γ-ray spectrum source in the galactic plane. AIP conference proceedings. 1792. 40024–40024. 2 indexed citations
13.
Casanova, S., et al.. (2017). Very high energy emission from the hard spectrum sources HESS J1641-463, HESS J1741-302 and HESS J1826-130. Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017). 686–686. 1 indexed citations
14.
Casanova, S.. (2017). First year results from the HAWC observatory. SHILAP Revista de lepidopterología. 136. 3005–3005. 1 indexed citations
15.
Greus, F. Salesa, S. Casanova, B. L. Dingus, R. López-Coto, & H. Zhou. (2017). Constraining the Origin of Local Positrons with HAWC TeV Gamma-Ray Observations of Two Nearby Pulsar Wind Nebulae. Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017). 722–722. 1 indexed citations
16.
Becker, J. K., et al.. (2012). Cosmic-ray-induced ionization in molecular clouds adjacent to supernova remnants. Astronomy and Astrophysics. 541. A126–A126. 24 indexed citations
17.
Casanova, S., Felix A. Aharonian, Y. Fukui, et al.. (2010). Molecular Clouds as Cosmic-Ray Barometers. Publications of the Astronomical Society of Japan. 62(3). 769–777. 28 indexed citations
18.
Casanova, S., Peter L. Biermann, Ralph Engel, A. Meli, & R. Ulrich. (2004). Sources of cosmic rays and galactic diffuse gamma radiation. 552. 521–524. 1 indexed citations
19.
Feigelson, Eric D., S. Casanova, & T. Montmerle. (1992). ROSAT Observations of the Chamaeleon Star Forming Cloud. AAS. 180.
20.
Casanova, S., et al.. (1970). Dislocation Dynamics and the Formulation of Constitutive Equations for Rate-Dependent Plastic Flow in Metals. Defense Technical Information Center (DTIC). 2 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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