McPartland, C.Sanders, D BKewley, LisaLeslie, S K2022-05-062022-05-060035-8711http://hdl.handle.net/1885/264575Local galaxies from the Sloan Digital Sky Survey (SDSS) are used to provide additional support for an evolutionary pathway in which active galactic nucleus activity is associated with star formation quenching. Composite, Seyfert 2, and LINER galaxies account for ∼60 per cent of all star formation in massive galaxies (M > 1010.5 M). Inclusion of these galaxies results in a ‘turnover’ in the star formation rate and stellar mass (SFR−M) relation for massive galaxies. Our analysis shows that bulge growth has already occurred in the most massive galaxies (M > 1010.5 M), and bulges continue to grow as galaxies quench and redden, (g − r) = 0.5→0.75. Significant bulge growth is also occurring in low mass starburst galaxies (M < 1010.5 M) at 0.5 dex above the ‘main sequence’ (MS), where we find an increase in B/T from 0.1→0.3 and bluer colours, (g − r) < 0.25 compared to low-mass galaxies on the MS.Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS web site is http://www.sdss.org/. DS would like to thank the Distinguished Visitor Program at the Research School for Astronomy and Astrophysics, Australian National University for their generous support while in residence at the Mount Stromlo Observatory, Weston Creek, ACT. CM and DS also acknowledge support from National Science Foundation grant number 1716994. The work of DS was performed in part at the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1607611.application/pdfen-AU© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societygalaxies: star-formationgalaxies: evolutiongalaxies: activegalaxies: Seyfertgalaxies: bulgesgalaxies: structureDissecting the main sequence: AGN activity and bulge growth in the local Universe201910.1093/mnrasl/sly2022020-12-27