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Ultracool dwarf Science with MachIne LEarning (USMILE). I. Scalable Tree-based Models for Photometric Spectral Classification and New Discoveries from LSST Data Preview 1 and Euclid Quick Data Release 1

  • Authors: Zhoujian Zhang, 周健 张, Yanxia Li, 燕侠 李

Zhoujian Zhang et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 10.

Coordinates of the initial candidates (Section 4) selected from LSST DP1, VHS, and CatWISE (gray circles) within the Extended Chandra Deep Field South (ECDFS; left), Euclid Deep Field South (EDF-S; middle), and a field at low Galactic latitude (Rubin SV 95 -25; right). Orange stars mark the ultracool dwarf discoveries confirmed by Euclid spectroscopy, all located in the EDF-S field (Section 6). These discoveries span spectral types M6–L2. Guided by the Euclid spectroscopic validation of the USMILE models, we further identify a set of high-quality M6–L9 candidates that lack high-S/N Euclid spectroscopy (Section 7), shown as blue stars.

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