The evolution of compact massive quiescent and star-forming galaxies derived from the R<SUB>e</SUB>-R<SUB>h</SUB> and M<SUB>star</SUB>-M<SUB>h</SUB> relations
The mean size (effective radius R e) of massive galaxies (MGs; M star > 10 11.2M ⊙) is observed to increase steadily with cosmic time. It is still unclear...
The evolution of compact supernova remnants in a strongly magnetized medium
Two-dimensional simulations of the evolution of supernova remnants in a uniform, high-density medium are presented. The medium is magnetized, and its magnetic...
The evolution of early-type galaxies in clusters from z˜ 0.8 to z ˜ 0: the ellipticity distribution and the morphological mix
We present the ellipticity distribution and its evolution for early-type galaxies in clusters from z˜ 0.8 to the current epoch, based on the WIde-field Nearby...
We present a study of galaxy sizes in the local Universe as a function of galaxy environment, comparing clusters and the general field. Galaxies with radii and...
The Evolution of Passive Galaxies since z=1: Major Mergers vs Secular Processes
We study the evolution of the red sequence and the blue cloud since z ~ 1 to present in GOODS-S field for MB ≤ -20 and M* ≥ 1010 M&sun; selected galaxies. We...
The evolution of quiescent galaxies at high redshifts (z≥ 1.4)
The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ˜1.7 deg2 in the COSMOS field. Galaxies...
The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ̃ 2-6 for SC4K LAEs
We explore deep rest-frame UV to FIR data in the COSMOS field to measure the individual spectral energy distributions (SED) of the ̃4000 SC4K (Sobral et al.)...
The Evolution of Spiral, S0, and Elliptical Galaxies in Clusters
We quantify the evolution of the spiral, S0 and elliptical fractions in galaxy clusters as a function of cluster velocity dispersion (σ) and X-ray luminosity...