activity
20152020
most citedStarburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at

83 citations · 180 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020★ 7 cited

A comparison of formation models at high redshift

Alexander Schäbe, Emilio Romano-Díaz, Cristiano Porciani +2

Modelling the molecular gas that is routinely detected through CO observations of high-redshift galaxies constitutes a major challenge for ab initio simulations of galaxy formation…

astro-ph.GA2019★ 41 cited

Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25

E. F. Jiménez-Andrade, B. Magnelli, A. Karim +18

We present the first systematic study of the radio continuum size evolution of star-forming galaxies (SFGs) over the redshift range . We use the VLA COSMOS 3GHz map (n…

astro-ph.GA2018★ 83 cited

Starburst to quiescent from HST/ALMA: Stars and dust unveil minor mergers in submillimeter galaxies at

C. Gómez-Guijarro, S. Toft, A. Karim +32

Dust-enshrouded, starbursting, submillimeter galaxies (SMGs) at have been proposed as progenitors of compact quiescent galaxies (cQGs). To test this connectio…

astro-ph.GA2017★ 17 cited

Molecular gas in AzTEC/C159: a star-forming disk galaxy 1.3Gyr after the Big Bang

E. F. Jiménez-Andrade, B. Magnelli, A. Karim +23

We studied the molecular gas properties of AzTEC/C159, a star-forming disk galaxy at . We secured CO molecular line detections for the and trans…

astro-ph.GA2017★ 23 cited

ZOMG III: The effect of Halo Assembly on the Satellite Population

Enrico Garaldi, Emilio Romano-Díaz, Mikolaj Borzyszkowski +1

We use zoom hydrodynamical simulations to investigate the properties of satellites within galaxy-sized dark-matter haloes with different assembly histories. We consider two classes…

astro-ph.GA2015★ 9 cited

The Baryon Cycle at High Redshifts: Effects of Galactic Winds on Galaxy Evolution in Overdense and Average Regions

Raphael Sadoun, Isaac Shlosman, Jun-Hwan Choi +1

We employ high-resolution cosmological zoom-in simulations focusing on a high-sigma peak and an average cosmological field at , in order to investigate the influence of…