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We present here the results relating to the ultracool regime within 100pc from the Gaia Catalogue of Nearby Stars, published as a science verification paper of the recent Gaia early data release 3. We provide updated evidence for the stellar/ substellar boundary being around L3 via the volume limited luminosity function. We estimate completeness of Gaia and show how thousands of new ultracool dwarf candidates have been selected.
{"references": ["Gaia Collaboration., et al., 2020, arXiv, arXiv:2012.02061", "Bardalez Gagliuffi, D. C., et al. 2019, ApJ, 883, 205", "Smart, R. L., et al. 2019, MNRAS, 485, 4423", "Reyl\u00e9, C. 2018, A&A, 619, L8"]}
ultracool dwarfs, Very low mass stars
ultracool dwarfs, Very low mass stars
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