tokens: ACKNOWLEDGEMENTS We thank the anonymous referee for her/his suggested improvements. IB is supported by an Alexander von Humboldt postdoctoral research fellowship. KG was supported by the German-Russian Interdisciplinary Science Center funded by the German Federal Foreign Office via the German Academic Exchange Service. We thank Graeme Candlish for sharing his data on the velocity field in MOND cosmology and Hosein Haghi for useful discussions about the properties of NGC 1052-DF2.
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