Fig. 3.
Download original image
Host galaxy photometry based on GALEX (Martin et al. 2005), DECaLS (Dey et al. 2019), and WISE (Wright et al. 2010; Mainzer et al. 2011). We also include the post-peak aperture photometry in the UVOT B- and U-band. We show samples from the posterior distribution of population synthesis galaxy models (Conroy et al. 2009; Johnson & Leja 2017), following the method outlined in van Velzen et al. (2021). The predicted magnitudes (including UVOT W1, M2, and W2) are shown with open circles.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.