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1 Erratum to: Eur. Phys. J. C (2017) 77:146 https://doi.org/10.1140/epjc/s10052-017-4689-9
In the analysis published in Ref. [1], constraints on the number of signal events \(n_{\mathrm {s}}\) can be interpreted as constraints on the volumetric neutrino to muon conversion rate \(\varLambda _{\nu \bar{\nu } \rightarrow \mu ^+ \mu ^-}\),
where \(T_{\mathrm {live}}\) and \(V_{\mathrm {eff}}\) are the livetime and effective volume of the data sample of index j. These can then be interpreted as constraints on the muon flux \(\varPhi _{\mu ^+ + \mu ^-}\), dark matter (DM) annihilation rate in the Sun \(\varGamma _{\chi \chi \rightarrow \mathrm {SM}}\), as well as the spin-dependent (SD) and spin-independent (SI) scattering cross sections \(\sigma _{\mathrm {SD}}\) and \(\sigma _{\mathrm {SI}}\) using WimpSim [2].
In Table 4 of Ref. [1], the labels and units of columns 7 and 8 suggest that the muon flux \(\varPhi _{\mu ^+ + \mu ^-}\) (in units km\(^{-2}\) year\(^{-1}\)) is being presented. However for the first 12 rows, corresponding to points in which the DeepCore (DC) dataset was included, the volumetric neutrino to muon conversion rate \(\varLambda _{\nu \bar{\nu } \rightarrow \mu ^+ \mu ^-}\) (in units km\(^{-3}\) year\(^{-1}\)) were erroneously reported instead. The corrected table (Table 1) is presented hereby. All other columns remain unchanged. All quantities that go into the right hand side of Eq. 1 are presented in the table, as well as median sensitivities and 90% C.L. upper limits on the muon flux \(\varPhi _{\mu ^+ + \mu ^-}\) derived using WimpSim [2].
The final results and conclusions presented in Ref. [1] in terms of constraints on the SD and SI scattering cross sections \(\sigma _{\mathrm {SD}}\) and \(\sigma _{\mathrm {SI}}\) as well as the DM annihilation rate in the Sun \(\varGamma _{\chi \chi \rightarrow \mathrm {SM}}\), remain unchanged.
In Section 4.2 of Ref. [1], the maximum zenith angle of the Sun is erroneously mentioned as 104\(^{\circ }\). The correct maximum zenith angle of the Sun is 114\(^{\circ }\)at the South Pole.
References
M.G. Aartsen et al. (IceCube Collaboration), Eur. Phys. J. C 77, 146 (2017)
M. Blennow, J. Edsjö, T. Ohlsson, JCAP 01, 021 (2008)
Acknowledgements
We thank Joakim Edsjö and Tom Gaisser for the careful scrutiny through which these errors were brought to light.
The authors gratefully acknowledge support from the following agencies and institutions: USA – U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium – Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany – Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing cluster of the RWTH Aachen; Sweden – Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia – Australian Research Council; Canada – Natural Sciences and Engineering Research Council of Canada, Calcul Québec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark – Villum Fonden, Danish National Research Foundation (DNRF), Carlsberg Foundation; New Zealand – Marsden Fund; Japan – Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea – National Research Foundation of Korea (NRF); Switzerland – Swiss National Science Foundation (SNSF).
Author information
M. Rameez
Present address: Niels Bohr Institute, University of Copenhagen, 2100, Copenhagen, Denmark
Authors and Affiliations
III. Physikalisches Institut, RWTH Aachen University, 52056, Aachen, Germany
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Aartsen, M.G., Ackermann, M., Adams, J. et al. Erratum to: Search for annihilating dark matter in the Sun with 3 years of IceCube data. Eur. Phys. J. C 79, 214 (2019). https://doi.org/10.1140/epjc/s10052-019-6702-y
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DOI: https://doi.org/10.1140/epjc/s10052-019-6702-y
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