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tokens: A.M.B. thanks Christian Ginsky for the help in reducing the SPHERE/IRDIS data and the useful discussion afterwards, and Wolfgang Brandner for the help in reducing the GPI data. A.M.B. would also like to thank the anonymous referee for the useful and constructive comments. G.M.K. is supported by the Royal Society as a Royal Society University Research Fellow. G.C. and S.P.Q. thank the Swiss National Science Foundation for the financial support under the grant number 200021_169131. J.O. and N.G. acknowledge financial support from the ICM (Iniciativa Científica Milenio) via the Núcleo Milenio de Formación Planetaria grant. J.O. acknowledges financial support from the Universidad de Valparaíso, and from Fondecyt (grant 1180395). N.G. acknowledges support from project CONICYT-PFCHA/Doctorado Nacional/2017 folio 21170650. A.M. and A.Q. acknowledge the support of the DFG priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets” (MU 4172/1-1 and QU 113/6-1). This research has made use of the Washington Double Star Catalog maintained at the U.S. Naval Observatory, and of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research made use of Astropy ( http://www.astropy.org ), a community-developed core Python package for Astronomy ( Astropy Collaboration 2013 , 2018 ).