The Gaia ultracool dwarf sample – V: the ultracool dwarf companion catalogue

Author:

Baig Sayan12ORCID,Smart R L12,Jones Hugh R A1,Gagné Jonathan34,Pinfield D J1,Cheng Gemma1ORCID,Moranta Leslie345

Affiliation:

1. School of Physics, Astronomy and Mathematics, University of Hertfordshire , College Lane, Hatfield, AL10 9AB , UK

2. Istituto Nazionale di Astrofisica , Osservatorio Astrofisico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese , Italy

3. Planétarium Rio Tinto Alcan , Espace pour la Vie, 4801 av. Pierre-de Coubertin, Montréal, Québec , Canada

4. Institute for Research on Exoplanets, Université de Montréal , Département de Physique, C.P. 6128 Succ. Centre-ville, Montréal, QC H3C 3J7 , Canada

5. Department of Astrophysics, American Museum of Natural History , Central Park West at 79th St, New York, NY 10024 , USA

Abstract

ABSTRACT We present the Ultracool Dwarf Companion Catalogue of 278 multiple systems, 32 of which are newly discovered, each with at least one spectroscopically confirmed Ultracool Dwarf, within a 100 pc volume-limited sample. This catalogue is compiled using the Gaia Catalogue of Nearby Stars for stellar primaries and the Gaia Ultracool Dwarf Sample for low-mass companions and includes 241 doubles, 33 triples, and 4 higher-order systems established from positional, proper motion, and parallax constraints. The catalogue seeks to identify probable benchmark systems within 100 pc to obtain model-independent astrophysical parameters of Ultracool Dwarfs. Chance alignment probabilities are calculated to evaluate the physical nature of each system. Astrometric and photometric data from Gaia Data Release 3 and the Two Micron All Sky Survey are included for all objects. We identify potential unseen companions using a combination of the renormalized unit weight error, image parameter determination statistics, non-single star solutions, and photometric blending as provided by Gaia, identifying hierarchical Ultracool triple systems. Our catalogue includes 17 White Dwarf – Ultracool Dwarf systems, whose ages are determined using cooling models. We also use the Gaia FLAME results and the BANYAN Σ procedures to age 40 and 34 systems, respectively, and derive mass estimates from evolutionary models.

Funder

Science & Technology Facilities Council

European Space Agency

Publisher

Oxford University Press (OUP)

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