Star-formation rate as a function of the stellar mass of the BBs of this work (purple circles), the BBs of Yang et al. (2017) (blue squares), the GPs of Cardamone et al. (2009) (green rhombuses), the BDGs of Izotov et al. (2011) (red X’s), and the SFGs of HECATE (gray dots). The blue dashed, magenta dashed-dotted, yellow dotted, and red dashed-dotted lines respectively show the main sequence fits of Elbaz et al. (2007), Speagle et al. (2014), Popesso et al. (2019), and Kouroumpatzakis et al. (2021). The thin black dashed lines indicate some constant values of log sSFR.