HST grism spectroscopy of z ∼ 3 massive quiescent galaxies. Approaching the metamorphosis
Tracing the emergence of the massive quiescent galaxy (QG) population requires the build-up of reliable quenched samples by distinguishing these systems from red, dusty star-forming sources. We present Hubble Space Telescope WFC3/G141 grism spectra of ten quiescent galaxy candidates selected at 2.5 < z < 3.5 in the COSMOS field. Spectroscopic
D'Eugenio, C. et al.
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2021