Erratum: Filament Formation due to Diffusive Instabilities in Dusty Protoplanetary Disks (Astrophysical Journal (2024) 961 (183) DOI: 10.3847/1538-4357/ad1114)

In the published article, there is a sign error, specifically in Equation (13), that propagates throughout the paper and warrants modification of several equations and figures. The term in question becomes significant only in the limit of τs 1. The primary conclusions concerning the formation of axisymmetric filaments in dusty protoplanetary disks are based on the more physically relevant limit of τs 1 and are therefore unaffected. However, quantitative discussion needs to be corrected, in particular for τs 1 and Sc=1. In this erratum, we present all updated equations and figures and point out where the drawn conclusions need be modified. (Formula Presented) (Figure Presented).