Erratum to "Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope" [Phys. Lett. B 769 (2017) 249-254]

doi:10.1016/j.physletb.2019.05.022

Erratum to "Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope" [Phys. Lett. B 769 (2017) 249-254]

Albert, A.
André, M.
Anghinolfi, M.
Anton, G.
Ardid, M.
Aubert, J. -J.
Avgitas, T.
Baret, B.
Barrios-Martí, J.
Basa, S.
Bertin, V.
Biagi, S.
Bormuth, R.
Bourret, S.
Bouwhuis, M. C.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Celli, S.
Chiarusi, T.
Circella, M.
Coelho, J. A. B.
Coleiro, A.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Deschamps, A.
De Bonis, G.
Distefano, C.
Di Palma, I.
Donzaud, C.
Dornic, D.
Drouhin, D.
Eberl, T.
El Bojaddaini, I.
Elsässer, D.
Enzenhöfer, A.
Felis, I.
Fusco, L. A.
Galatà, S.
Gay, P.
Geißelsöder, S.
Geyer, K.
Giordano, V.
Gleixner, A.
Glotin, H.
and 79 more

Limits on the neutrino flux for a given mass M_WIMP and annihilation channel are calculated as in Eq. (7) (page 252), with the integrated acceptances defined in Eq. (8) (page 252) as the effective area averaged over the neutrino energy. A numerical approximation of WIMP annihilation spectra, adapted from [1] with a too coarse binning, led to an overestimation of the integrated acceptances for dark-matter induced neutrino events. The spectra were replaced with a fine-binned version both in the likelihood and in the acceptances. The main change is a weaker limit for WIMP masses larger than 1 TeV/c². Updated versions of Figs. 3-6 are provided.

Publication:: Physics Letters B
Pub Date:: September 2019
DOI:: 10.1016/j.physletb.2019.05.022
Bibcode:: 2019PhLB..796..253A

ADS

Erratum to "Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope" [Phys. Lett. B 769 (2017) 249-254]

Abstract