Journal Article PUBDB-2025-01817

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Evidence for $γ$-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations (Corrigendum)

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2024
EDP Sciences Les Ulis

Astronomy and astrophysics 683, C1 () [10.1051/0004-6361/202348902e]
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Report No.: arXiv:2201.05839

Abstract: In the version of this article initially published, there was a typographical error in the second paragraph of Sect. 4. The normalization constant should be read N$_0$ = (9.5 ± 2.3$_{stat}$± 2.9$_{sys}$ × 10$^{−14}$ cm$^{−2}$ s$^{−1}$ TeV$^{−1}$. The normalization was correctly stated elsewhere.Also, the author’s name D. Malyshev (affiliated with Institute 23) was inadvertently missing from the author list of the published version. It is added here.

Classification:

Contributing Institute(s):
  1. High Energy Steroscopic System (Z_HESS)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
Experiment(s):
  1. High Energy Stereoscopic System

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Medline ; Clarivate Analytics Master Journal List ; Current Contents - Physical, Chemical and Earth Sciences ; Ebsco Academic Search ; Essential Science Indicators ; IF >= 5 ; JCR ; SCOPUS ; Science Citation Index Expanded ; Web of Science Core Collection
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http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Journal Article  ;  ;  ; et al
Evidence for $\gamma$-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations
Astronomy and astrophysics 662, A65 () [10.1051/0004-6361/202243096]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2025-06-05, last modified 2025-06-25


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