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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

Author
Acharyya, A.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Ascasibar Sequeiros, Yagountranslated; Gaggero, D.; Gammaldi, V.; Pérez-Romero, J.; Sánchez-Conde, MA; CTA Consortium
Entity
UAM.Departamento de Física Teórica; Instituto de Física Teórica (IFT)
Publisher
IOP
Date
2021-01-27
Citation
Journal of Cosmology and Astroparticle Physics 2021.1 (2021): 51
ISSN
1475-7516
DOI
10.1088/1475-7516/2021/01/057
Editor's Version
http://doi.org/10.1088/1475-7516/2021/01/057
Subjects
Dark Matter Experiments; Dark Matter Theory; Galaxy Morphology; Gamma Ray Experiments; Gamma-Ray Signals; Radiative Processes; Candidates; Annihilation; Contraction; Simulations; Mass; Particle; Clumpy; Physics; Astronomía; Física
URI
http://hdl.handle.net/10486/701034
Rights
© 2021, The Author(s)

Licencia Creative Commons
Esta obra está bajo una Licencia Creative Commons Atribución 4.0 Internacional.
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Google™ Scholar:Acharyya, A. - Aguirre-Santaella, A. - Alfaro, R. - Alfaro, J. - Ascasibar Sequeiros, Yago - Gaggero, D. - Gammaldi, V. - Pérez-Romero, J. - Sánchez-Conde, MA - CTA Consortium

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