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Estimated LIR of the sources before quenching as a function of the median LIR of a reference sample with similar stellar mass. The cyan squares are the HRS quenched galaxies while the dots are the COSMOS ones. COSMOS galaxies with a diamond are sources with a 24 μm detection. Red dots are COSMOS quenched galaxies that are spectroscopically confirmed. The error bars show the dispersion of the LIR distribution of each reference sample. The solid line shows the one-to-one relationship while the dashed-dotted and dotted lines show a factor three and a factor ten above it, respectively.
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