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# Erratum: Dark matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions

R Jackson, S Kaviraj, G Martin, J Devriendt, A Slyz, J Silk, Y Dubois, S Yi, C Pichon, M Volonteri, et al.

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► To cite this version:

R Jackson, S Kaviraj, G Martin, J Devriendt, A Slyz, et al. Erratum: Dark matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions. Monthly Notices of the Royal Astronomical Society, 2021, 506 (3), pp.4499-4499. 10.1093/mnras/stab2002. hal-03433188

HAL Id: hal-03433188

https://hal.science/hal-03433188v1

Submitted on 22 Nov 2024

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# Erratum: Dark matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions

by R. A. Jackson<sup>1,★</sup>, S. Kaviraj<sup>1</sup>, G. Martin<sup>1,2,3</sup>, J. E. G. Devriendt,<sup>4</sup> A. Slyz,<sup>4</sup> J. Silk,<sup>4,5,6</sup> Y. Dubois,<sup>5</sup> S. K. Yi,<sup>7</sup> C. Pichon,<sup>5,8</sup> M. Volonteri,<sup>5</sup> H. Choi,<sup>3</sup> T. Kimm<sup>1,9</sup>,<sup>7</sup> K. Kraljic<sup>1,9</sup> and S. Peirani<sup>5,10</sup>

**Key words:** errata, addenda – methods: numerical – galaxies: dwarf – galaxies: evolution – galaxies: formation – galaxies: interactions.

This is an erratum to the paper 'Dark matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions', which was published in MNRAS, 502, 1785 (Jackson et al. 2021). In the original version of the paper S. K. Yi's affiliation was incorrectly listed as 'School of Physics, Korea Institute for Advanced Study (KIAS), 85 Hoegiro, Dongdaemun-gu, Seoul 02455, Republic of Korea', whereas the correct affiliation is 'Department of Astronomy and Yonsei University Observatory, Yonsei University, Seoul 03722, Republic of Korea'. In addition S. K. Yi would also like to add the following acknowledgement: SKY acknowledges support from the Korean National Research Foundation (NRF-2020R1A2C3003769). The supercomputing time for numerical simulation was kindly provided by KISTI (KSC-2017-G2-003), and large data transfer was supported by KREONET.

## REFERENCE

Jackson R. A. et al., 2021, MNRAS, 502, 1785

This paper has been typeset from a TeX/LATEX file prepared by the author.

<footnote n="1"><sup>1</sup>Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, AL10 9AB, UK</footnote>

<footnote n="2"><sup>2</sup>Steward Observatory, University of Arizona, 933 N. Cherry Ave, Tucson, AZ 85719, USA</footnote>

<footnote n="3"><sup>3</sup>Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Korea</footnote>

<footnote n="4"><sup>4</sup>Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH, UK</footnote>

<footnote n="5"><sup>5</sup>Institut d'Astrophysique de Paris, Sorbonne Universités, UMPC Univ Paris 06 et CNRS, UMP 7095, 98 bis bd Arago, F-75014 Paris, France</footnote>

<footnote n="6"><sup>6</sup>Department of Physics & Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA</footnote>

<footnote n="7"><sup>7</sup>Department of Astronomy and Yonsei University Observatory, Yonsei University, Seoul 03722, Republic of Korea</footnote>

<footnote n="8"><sup>8</sup>School of Physics, Korea Institute for Advanced Study (KIAS), 85 Hoegiro, Dongdaemun-gu, Seoul, 02455, Republic of Korea</footnote>

<footnote n="9"><sup>9</sup>Institute for Astronomy, Royal Observatory, Edinburgh EH9 3HJ, UK</footnote>

<footnote n="10"><sup>10</sup>Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, Université Côte d'Azur, CS 34229, F-06304 Nice Cedex 4, France</footnote>

<footnote>* E-mail: r.jackson9@herts.ac.uk</footnote>