The KMOS Cluster Survey – KCS: Timing the formation of passive galaxies in clusters with 1.4<z<1.8

Beifiori, Alessandra

Publication date

March 2019

DOI

Abstract

In this talk I will discuss recent progress studying the rest-frame optical properties of quiescent galaxies at 1.4 < z < 1.8 using KMOS. I will highlight recent results form the KMOS Custer Survey (KCS), whose aim is to provide a census of quiescent galaxy kinematics at 1.4 < z < 1.8 in know overdensities. The combination of kinematic measurements from KMOS and structural parameters measured from deep HST imaging allowed us to place constraints on the formation ages of passive galaxies at 1.4 < z <1.8 and on the evolution of galaxy properties and scaling relations at high redshift

Extracted data

We use cookies to provide a better user experience.

Data Protection

The KMOS Cluster Survey – KCS: Timing the formation of passive galaxies in clusters with 1.4<z<1.8

Abstract

Extracted data

The KMOS Cluster Survey – KCS: Timing the formation of passive galaxies in clusters with 1.4<z<1.8

Abstract

Extracted data

Related items

Related items