Studying the ISM at ∼10 pc scale in NGC 7793 with MUSE

II. Constraints on the oxygen abundance and ionising radiation escape (Corrigendum)

¹ Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, 106 91 Stockholm, Sweden
e-mail: lorenza.dellabruna@astro.su.se
² Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA, USA
³ European Space Agency (ESA), ESA Office, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
⁴ Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2612, Australia
⁵ Observatoire de Genève, Université de Genève, Chemin Pegasi 51, 1290 Versoix, Switzerland
⁶ Dipartimento di Fisica G. Occhialini, Università degli Studi di Milano Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
⁷ Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, UK
⁸ Centre for Extragalactic Astronomy, Durham University, South Road, Durham DH1 3LE, UK
⁹ Department of Astronomy, New Mexico State University, Las Cruces, NM 88001, USA
¹⁰ Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800 BC, México

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