Fig. 3.
Offset of 210 isolated barred galaxies from the main sequence relation derived using GSWLC plotted against scaled bar length. Here the number of data points is limited and hence instead of binning the data we bootstrapped the data with confidence intervals shown in grey and the best-fit relation shown in black. The passive population of galaxies below the main sequence is shown in red. Galaxies on and above the relation are shown in blue.
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