Stellar mass–halo mass relation. The red symbols with error bars show the SHMR calculated using the halo mass obtained from the fits to the stacked lensing mass profiles from the DECaLS shear catalog, while the black ones are based on the LcSK method. For clarity, we shift the black symbols slightly toward the left. The error bars reflect the 16% and 84% of the posterior distribution. The diamonds and squares show the results for star-forming and total populations, respectively. The shadow region represents the range covered by curves published in Yang et al. (2009), Moster et al. (2010), Leauthaud et al. (2012), Kravtsov et al. (2018), and Behroozi et al. (2019).