Image Details
Caption: Figure 7.
Scarlet scene model from LS DR10 imaging (grz). Each labeled source was modeled as a monotonically decreasing profile except for the host galaxy, which was modeled by a double pseudo-Sérsic in order to best account for the diffuse extended emission. We show the model rendered to match the LS imaging (left), the coadded LS grz image (center), and the data–model residual (right). The central box showed the region used to estimate an upper limit on an NSC cluster associated with the TDE position.
© 2026. The Author(s). Published by the American Astronomical Society.