102 citations · 763 across the 21 of their papers we have counts for
21 papers
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
C. Karoumpis, B. Magnelli, E. Romano-Díaz +2
We predict the three-dimensional intensity power spectrum (PS) of the [CII] 158m line throughout the epoch of (and post) reionization at redshifts from 3.5 to 8. We…
Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
Kevin C. Harrington, Axel Weiss, Min S. Yun +26
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and coo…
The "Red Radio Ring": Ionised and Molecular Gas in a Starburst/Active Galactic Nucleus at
K. C. Harrington, A. Vishwas, A. Weiss +13
We report the detection of the far-infrared (FIR) fine-structure line of singly ionised nitrogen, \Nplusa, within the peak epoch of galaxy assembly, from a strongly lensed galaxy,…
Lyman alpha Properties of Simulated Galaxies in Overdense Regions: Effects of Galactic Winds at z > 6
Raphael Sadoun, Emilio Romano-Diaz, Isaac Shlosman +1
We perform Monte-Carlo radiative transfer calculations to model the Lyman alpha properties of galaxies in high-resolution, zoom-in cosmological simulations at z ~ 6.6. The simulati…
On the radial acceleration relation of CDM satellite galaxies
Enrico Garaldi, Emilio Romano-Díaz, Cristiano Porciani +1
The radial acceleration measured in bright galaxies tightly correlates with that generated by the observed distribution of baryons, a phenomenon known as the radial acceleration re…
ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
Emilio Romano-Diaz, Enrico Garaldi, Mikolaj Borzyszkowski +1
The growth-rate and the internal dynamics of galaxy-sized dark-matter haloes depend on their location within the cosmic web. Haloes that sit at the nodes grow in mass till the pres…