Erratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data

Author(s): Aartsen, MG; Ackermann, M; Adams, J; Aguilar, JA; Ahlers, M; Ahrens, M; Altmann, D; Andeen, K; Anderson, T; Ansseau, I; Anton, G; Archinger, M; Arguelles, C; Auffenberg, J; Axani, S; Bai, X; Barwick, SW; Baum, V; Bay, R; Beatty, JJ; Becker Tjus, J; Becker, KH; BenZvi, S; Berley, D; Bernardini, E; Bernhard, A; Besson, DZ; Binder, G; Bindig, D; Bissok, M; Blaufuss, E; Blot, S; Bohm, C; Borner, M; Bos, F; Bose, D; Boser, S; Botner, O; Braun, J; Brayeur, L; Bretz, HP; Bron, S; Burgman, A; Carver, T; Casier, M; Cheung, E; Chirkin, D; Christov, A; Clark, K; Classen, L; Coenders, S; Collin, GH; Conrad, JM; Cowen, DF; Cross, R; Day, M; de Andre, JPAM; De Clercq, C; del Pino Rosendo, E; Dembinski, H; De Ridder, S; Desiati, P; de Vries, KD; de Wasseige, G; de With, M; DeYoung, T; Diaz-Velez, JC; di Lorenzo, V; Dujmovic, H; Dumm, JP; Dunkman, M; Eberhardt, B; Ehrhardt, T; Eichmann, B; Eller, P; Euler, S; Evenson, PA; Fahey, S; Fazely, AR; Feintzeig, J; Felde, J; Filimonov, K; Finley, C; Flis, S; Fosig, CC | Abstract: © 2019, The Author(s). In the analysis published in 1, constraints on the number of signal events can be interpreted as constraints on the volumetric neutrino to muon conversion rate.