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An extremely young massive clump forming by gravitational collapse in a primordial galaxy
A. Zanella, E. Daddi, E. Le Floc'h +9
When the cosmic star formation history peaks (z ~ 2), galaxies vigorously fed by cosmic reservoirs are gas dominated and contain massive star-forming clumps, thought to form by vio…
Star formation and quenching among the most massive galaxies at z~1.7
Chiara Mancini, Alvio Renzini, Emanuele Daddi +5
We have conducted a detailed object-by-object study of a mass-complete (M*>10^11 M_sun) sample of 56 galaxies at 1.4 < z < 2 in the GOODS-South field, showing that an accurate de-b…
Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028
M. Brusa, C. Feruglio, G. Cresci +16
Gas outflows are believed to play a pivotal role in shaping galaxies, as they regulate both star formation and black hole growth. Despite their ubiquitous presence, the origin and…
A Physical Approach to the Identification of High-z Mergers: Morphological Classification in the Stellar Mass Domain
Anna Cibinel, Emeric Le Floc'h, Valentin Perret +6
At z>1, the distinction between merging and 'normal' star-forming galaxies based on single band morphology is often hampered by the presence of large clumps which result in a distu…
The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxies
Matthieu Béthermin, Carlos De Breuck, Mark Sargent +1
We interpret the large variety of redshift distributions of galaxies found by far-infrared and (sub-)millimeter deep surveys depending on their depth and wavelength using the Béthe…
A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43
Mark T. Sargent, E. Daddi, F. Bournaud +6
Gas and dust in star-forming galaxies at the peak epoch of galaxy assembly are presently the topic of intense study, but little is known about the interstellar medium (ISM) of dist…