no code implementations • 4 Dec 2020 • Peter Lustig, Veronica Strazzullo, Chiara D'Eugenio, Emanuele Daddi, Maurilio Pannella, Alvio Renzini, Andrea Cimatti, Raphael Gobat, Shuowen Jin, Joseph J. Mohr, Masato Onodera
We study structural properties of spectroscopically confirmed massive quiescent galaxies at $z\approx 3$ with one of the first sizeable samples of such sources, made of ten $10. 8<\log(M_{\star}/M_{\odot})<11. 3$ galaxies at $2. 4 < z < 3. 2$ in the COSMOS field whose redshifts and quiescence are confirmed by HST grism spectroscopy.
Astrophysics of Galaxies
