Fig. 4.

Atomic gas depletion timescale (≡ MHI/SFR) as a function of the ratio of the sSFR to the main-sequence sSFR at a given redshift and stellar mass (Speagle et al. 2014). CGCG 137-068 and GRB/SN hosts (Michałowski et al. 2015, 2018a) are shown as a black square and red circles and arrows, respectively. The main sequence and its scatter are shown as a blue vertical solid line and the hatched region, respectively. For each galaxy, a black or green star shows the predicted gas depletion time for its SFR from the MHI-SFR relation (Michałowski et al. 2015). The errors include both the uncertainty in the SFRs and in the parameters of the relation.
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.