K. Kosack

18.8k total citations
21 papers, 146 citations indexed

About

K. Kosack is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Radiation. According to data from OpenAlex, K. Kosack has authored 21 papers receiving a total of 146 indexed citations (citations by other indexed papers that have themselves been cited), including 18 papers in Nuclear and High Energy Physics, 15 papers in Astronomy and Astrophysics and 2 papers in Radiation. Recurrent topics in K. Kosack's work include Astrophysics and Cosmic Phenomena (18 papers), Gamma-ray bursts and supernovae (12 papers) and Astrophysical Phenomena and Observations (8 papers). K. Kosack is often cited by papers focused on Astrophysics and Cosmic Phenomena (18 papers), Gamma-ray bursts and supernovae (12 papers) and Astrophysical Phenomena and Observations (8 papers). K. Kosack collaborates with scholars based in France, Germany and United Kingdom. K. Kosack's co-authors include Ryo Yamazaki, Aya Bamba, C. Deil, T. Hassan, Ellis R. Owen, N. Kelley-Hoskins, D. A. Sanchez⋆, Nu. Komin, R. Buehler and S. Ohm and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Astroparticle Physics.

In The Last Decade

K. Kosack

19 papers receiving 145 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
K. Kosack France 7 136 105 11 5 5 21 146
V. Marandon France 6 119 0.9× 104 1.0× 11 1.0× 3 0.6× 5 1.0× 25 136
C. Deil Germany 4 80 0.6× 53 0.5× 11 1.0× 3 0.6× 4 0.8× 5 92
S. Westerhoff United States 8 109 0.8× 53 0.5× 15 1.4× 6 1.2× 13 2.6× 21 133
O. Blanch Spain 7 129 0.9× 103 1.0× 4 0.4× 5 1.0× 4 0.8× 38 151
J. Holder United Kingdom 3 221 1.6× 191 1.8× 5 0.5× 7 1.4× 5 1.0× 5 227
D. Sobczyńska Poland 7 93 0.7× 37 0.4× 12 1.1× 6 1.2× 7 1.4× 24 102
D. R. Bergman United States 8 160 1.2× 61 0.6× 4 0.4× 3 0.6× 3 0.6× 39 170
C. B. Rulten United Kingdom 6 69 0.5× 49 0.5× 8 0.7× 9 1.8× 4 0.8× 15 79
D. Dominis Prester Croatia 5 56 0.4× 48 0.5× 11 1.0× 4 0.8× 4 0.8× 30 63
Jenni Adams United States 9 154 1.1× 127 1.2× 7 0.6× 2 0.4× 11 2.2× 22 178

Countries citing papers authored by K. Kosack

Since Specialization
Citations

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

Fields of papers citing papers by K. Kosack

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Kosack

This figure shows the co-authorship network connecting the top 25 collaborators of K. Kosack. A scholar is included among the top collaborators of K. Kosack 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 K. Kosack. K. Kosack 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.
Khélifi, B., et al.. (2023). The Very-high-energy Open Data Format: towards a shared, open data format in very-high-energy astronomy. arXiv (Cornell University). 1510–1510. 1 indexed citations
2.
Giunti, Luca, et al.. (2022). Constraining leptonic emission scenarios for the PeVatron candidate HESS J1702−420 with deep XMM-Newton observations. Astronomy and Astrophysics. 667. A130–A130. 2 indexed citations
3.
Kosack, K. & M. Peresano. (2019). ctapipe: A Low-level Data Processing Framework for CTA. ICRC. 36. 717. 1 indexed citations
4.
Peresano, M. & K. Kosack. (2019). ctapipe: A Low-level Data Processing Framework for the Cherenkov Telescope Array. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019). 717–717.
5.
Hassan, T., C. Boisson, & K. Kosack. (2017). Open high-level data formats and software for gamma-ray astronomy. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 5 indexed citations
6.
Parsons, R. D., J. King, F. Aharonian, et al.. (2017). The galactic centre viewed with H.E.S.S.. AIP conference proceedings. 1792. 40005–40005. 1 indexed citations
7.
Knödlseder, J., M. Mayer, C. Deil, et al.. (2016). GammaLib and ctools. Astronomy and Astrophysics. 593. A1–A1. 48 indexed citations
8.
Horns, D., et al.. (2014). A new method of reconstructing VHE γ-ray spectra: the Template Background Spectrum. 2 indexed citations
9.
Tibolla, O., S. Kaufmann, & K. Kosack. (2014). XMM-NewtonandChandraX-ray follow-up observations of the VHE gamma-ray source HESS J1507-622. Astronomy and Astrophysics. 567. A74–A74. 2 indexed citations
10.
Hahn, J., R. de los Reyes, K. Bernlöhr, et al.. (2013). Impact of aerosols and adverse atmospheric conditions on the data quality for spectral analysis of the H.E.S.S. telescopes. Astroparticle Physics. 54. 25–32. 21 indexed citations
11.
Viana, A., M. C. Medina, Jorge Peñarrubia, et al.. (2012). Prospects for a Dark Matter Annihilation Signal toward the Sagittarius Dwarf Galaxy with Ground-based Cherenkov telescopes. CONICET Digital (CONICET). 4 indexed citations
12.
Hahn, Joachim, R. de los Reyes, K. Bernlöhr, et al.. (2012). Ensuring long-term stability of data quality selection for H.E.S.S. under challenging atmospheric conditions. AIP conference proceedings. 721–724. 1 indexed citations
13.
Kosack, K., R. C. G. Chaves, & F. Acero. (2011). HESS J1852-000: A Very High Energy Gamma-ray source near Supernova Remnant Kes~78. International Cosmic Ray Conference. 7. 76–78.
14.
Tibolla, O., Nu. Komin, K. Kosack, et al.. (2009). HESS J1741-302: a new source discovered in the Galactic Center region. AIP conference proceedings. 233–237. 1 indexed citations
15.
Feinstein, F., A. Fiaßon, Y. A. Gallant, et al.. (2009). What do supernova remnants interacting with molecular clouds reveal?. AIP conference proceedings. 54–62. 7 indexed citations
16.
Bamba, Aya, Ryo Yamazaki, Kazunori Kohri, et al.. (2009). X-RAY OBSERVATION OF VERY HIGH ENERGY GAMMA-RAY SOURCE, HESS J1745–303, WITHSUZAKU. The Astrophysical Journal. 691(2). 1854–1861. 17 indexed citations
17.
Fiaßon, A., K. Kosack, J. L. Skilton, et al.. (2008). Probing cosmic ray acceleration through molecular clouds in the vicinity of supernova remnant with H.E.S.S.. AIP conference proceedings. 361–363. 2 indexed citations
18.
Tibolla, O., Nu. Komin, K. Kosack, et al.. (2008). A new source discovered close to the Galactic Center: HESS J1741-302. AIP conference proceedings. 249–252. 5 indexed citations
19.
Gallant, Y. A., S. Carrigan, A. Djannati-Ataï, et al.. (2008). VHE γ-ray emitting pulsar wind nebulae discovered by H.E.S.S.. AIP conference proceedings. 983. 195–199. 6 indexed citations
20.
Hinton, J. A., S. Funk, S. Carrigan, et al.. (2007). Discovery of an X-ray nebula around PSR J1718-3825 and implications for the nature of the γ-ray source HESS J1718–385. Astronomy and Astrophysics. 476(3). L25–L28. 6 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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