Image Details
Caption: Figure 11.
Top panel: the iLSST − yLSST and zLSST − yLSST colors for the positive (colored) and negative (gray) samples in our labeled data set, with positive samples color-coded by spectral types. The 15 ultracool dwarf discoveries confirmed with Euclid spectroscopy are shown as orange stars (Section 6). For objects lacking high-S/N Euclid spectra, we identify 25 high-quality candidates based on our USMILE models, shown as blue stars (Section 7). The remaining rejected candidates are shown as black circles. Bottom panel: the zLSST − yLSST and yLSST − HVHS colors for objects plotted in the top panel.
© 2025. The Author(s). Published by the American Astronomical Society.