High-proper-motion objects detected in this work that do not have SIMBAD associations. Proper motions were estimated using both unTimely data and additional associations from several multiwavelength photometric catalogs. Effective temperatures are from the fit of these photometric data with the grid of BT-Settl (Allard 2014) model spectra, as is described in Section 2.3. Colored symbols represent known objects that we also detected and characterized, which have already been published in UltracoolSheet (Best et al. 2024a; Best et al. 2021, 2024b), Brooks et al. (2024), dal Ponte et al. (2023), or Burgasser et al. (2024b), and which thus are excluded from the final list. Vertical black vertical ticks at the bottom mark the proper motions of new objects that do not have enough multiwavelength associations for spectral fitting. The secondary vertical axis on the right shows the spectral types corresponding to the effective temperatures according to Pecaut & Mamajek (2013). Light gray points in the background show the Gaia DR3 stars within 100 pc with effective temperatures estimated using the GSP-Phot pipeline (Andrae et al. 2023).