Kavli Affiliate: Roberto Maiolino | Summary:We measure the fraction of clumpy galaxies ($f_rm clumpy$) over the redshift range $z=1-9$ and stellar masses $log_10(M_star/rm M_odot) geq 8$ using JWST/NIRCam imaging from JADES. We define clumps as compact off-centre surface-brightness peaks with characteristic sizes of a few hundred parsecs, and develop a dendrogram-based clump-finding method with astrodendro […]
Continue.. The clumpy fraction of galaxies at $z=1-9$ with JADES: evidence for a mass-dependent transition in clump origin