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A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies
A. Zanella, E. Le Floc'h, C. M. Harrison +14
We investigate the contribution of clumps and satellites to the galaxy mass assembly. We analyzed spatially-resolved Hubble Space Telescope observations (imaging and slitless spect…
Sunyaev-Zel'dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: the pressure profile in uv space
R. Gobat, E. Daddi, R. T. Coogan +9
We present Atacama Large Millimetre Array and Atacama Compact Array observations of the Sunyaev-Zel'dovich effect in the z = 2 galaxy cluster Cl J1449+0856, an X-ray-detected proge…
The Main Sequence at contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?
A. Puglisi, E. Daddi, D. Liu +20
ALMA measurements for 93 -selected galaxies at in COSMOS reveal a sizable (\%) population with compact star formation (SF) sizes, lyi…
Suppressed CO emission and high G/D ratios in z=2 galaxies with sub-solar gas-phase metallicity
R. T. Coogan, M. T. Sargent, E. Daddi +6
We study a population of significantly sub-solar enrichment galaxies at z=1.99, to investigate how molecular gas, dust and star-formation relate in low-metallicity galaxies at the…
Deciphering an evolutionary sequence of merger stages in infrared-luminous starburst galaxies at z ~ 0.7
Antonello Calabrò, Emanuele Daddi, Annagrazia Puglisi +18
Based on optical/near-IR Magellan FIRE spectra of 25 starburst galaxies at 0.5 < z < 0.9, Calabrò et al.(2018) showed that their attenuation properties can be explained by a single…