Galaxy Evolution is at the core of Extragalactic Astronomy. Star formation, environment, and AGN-feedback drive Galaxy Evolution. In the era of the large facilities and big data, Galaxy Surveys have an undeniable leading role to investigate how galaxies form and evolve. The purpose of this symposium is to discuss recent results in the field obtained by the Spanish community, with a special focus on findings delivered from current surveys on Galaxy Evolution led by Spanish facilities, such as CAVITY, J-PAS, J-PLUS, WEAVE, and SKA(-pathfinders). The symposium will consist of four sessions, covering the following topics:
Star formation and stellar content: Integrated and spatial resolved properties of galaxies and star formation history in nearby galaxies. Identification and characterization of galaxies populations and cosmic evolution. Connection morphology-galaxy populations at the local and far-way Universe.
Gas content and scaling laws: HI and molecular gas content in galaxies, and scaling laws: Gas accretion and the mass assembly history of galaxies. HI as a tracer of galaxy environment.
AGN-feedback: Outflows of ionized or neutral gas in galaxies with AGNs. Dust in AGNs: connection with winds. Co-evolution of star formation in galaxies and nuclear activity.
Properties of galaxies in voids, groups, and clusters: Identification of voids, groups, clusters and proto-clusters in galaxy surveys. Characterization of galaxy populations in proto-clusters, voids, and galaxy overdensities. The role of groups, clusters and proto-clusters in quenching the star formation in galaxies.