Understanding how galaxies assemble their structure and evolve morphologically over cosmic time is a central goal of galaxy evolution studies. In particular, the morphological evolution of quiescent and star-forming galaxies provides key insights into the mechanisms that regulate star formation and quenching. We present a new catalog of morphological measurements for more than 340000 sources spanning 0<z3. Quiescent galaxies also show significantly higher stellar mass surface densities, nearly an order of magnitude greater at z~4 than at z~1. Our results confirm a strong and evolving link between morphology and star formation activity and support a scenario in which bulge growth and quenching are closely connected. This work is a highly valuable addition to the DJA, adding a morphological dimension to this rich dataset and thus enabling a wider scientific application.

Cone search capability for table J/A+A/699/A343/good-ser (Sersic model-fitting)

Cone search capability for table J/A+A/699/A343/good-bd (Bulge+Disk model fitting)