Description
Euclid Wide Survey will observe tens of thousands of galaxies in the Local Universe within 100 Mpc with fantastic depth and spatial resolution. Such a dataset enables us to identify globular clusters (GCs) around these galaxies in a wide range of mass and environment, and gain unprecedented insight into the connection between star clusters and their host galaxies. In this talk, I present the ongoing work within the Euclid Consortium to study GCs of nearby galaxies. I will use the results of the recent works on the Euclid Early Release Observations (ERO) data to assess the Euclid capabilities in identifying GCs and examining their properties as a function of the host galaxy properties. Then, I will present the plans within the Euclid Consortium for studying GCs around galaxies with the Euclid first data release (DR1). Euclid DR1 is based on 1-year of Euclid observations, covering 1,900 deg^2 of the extragalactic sky.
