Fig. 4.
Left panel: M gas/M ⋆ vs. redshift (where M gas = 100M dust). Circled points are the “extreme” starbursts, those with SFR > 5000 M ⊙ yr−1. Right panel: M ⋆/SFR (or, the time-scale needed to make the observed mass of stars at the present star-formation rate) vs. redshift for HerMES galaxies. The source are labelled by their dominant infrared template type. The candidate extreme starbursts are shown circled.
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