130 citations · 614 across the 29 of their papers we have counts for
6 papers · 1 filter
Compact, bulge dominated structures of spectroscopically confirmed quiescent galaxies at z~3
Peter Lustig, Veronica Strazzullo, Chiara D'Eugenio +8
We study structural properties of spectroscopically confirmed massive quiescent galaxies at with one of the first sizeable samples of such sources, made of ten $10.8<\…
HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
C. D'Eugenio, E. Daddi, R. Gobat +6
Tracing the emergence of the massive quiescent galaxy (QG) population requires the build-up of reliable quenched samples. We present Hubble Space Telescope WFC3/G141 grism spectra…
The evolution of the gas fraction of quiescent galaxies modeled as a consequence of their creation rate
Raphael Gobat, Georgios Magdis, Chiara D'Eugenio +1
We discuss the evolution of the interstellar medium of quiescent galaxies, currently emerging from recent analyses, with the help of a simple model based on well-established empiri…
The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4
I. Delvecchio, E. Daddi, M. T. Sargent +25
Several works in the past decade have used the ratio between total (rest 8-1000m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q), often referre…
Three Lyman-alpha emitting filaments converging to a massive galaxy group at z=2.91: discussing the case for cold gas infall
E. Daddi, F. Valentino, R. M. Rich +21
We have discovered a 300kpc-wide giant Lya nebula centered on the massive galaxy group RO-1001 at z=2.91 in the COSMOS field. Keck Cosmic Web Imager observations reveal three cold…
The Typical Massive Quiescent Galaxy at z3 is a Post-starburst
C. D'Eugenio, E. Daddi, R. Gobat +10
We have obtained spectroscopic confirmation with Hubble Space Telescope WFC3/G141 of a first sizeable sample of nine quiescent galaxies at 2.4<z<3.3. Their average near-UV/optical…