FIR properties of some of our galaxies with individual FIR detections. All these galaxies have 1010.8 < M∗ [M⊙] < 1011. In the first column, galaxies have − 0.1 < Δlog (SSFR)MS < 0.1 while in the second column they have Δlog (SSFR)MS > MAX [Δlog (SSFR)MS] − 0.1. Black lines show the DH SED templates best-fitting these FIR flux densities. From these fits, we inferred the infrared luminosities and dust temperatures of our galaxies.
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.