74 citations · 365 across the 18 of their papers we have counts for
18 papers
MUSE-ALMA Haloes X: The stellar masses of gas-rich absorbing galaxies
Ramona Augustin, Céline Péroux, Arjun Karki +13
The physical processes by which gas is accreted onto galaxies, transformed into stars and then expelled from galaxies are of paramount importance to galaxy evolution studies. Obser…
ALMACAL. XI. Over-densities as signposts to proto-clusters? A cautionary tale
Jianhang Chen, R. J. Ivison, Martin A. Zwaan +6
It may be unsurprising that the most common approach to finding proto-clusters is to search for over-densities of galaxies. Upgrades to submillimetre (submm) interferometers and th…
MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
Arjun Karki, Varsha P. Kulkarni, Simon Weng +15
Understanding how galaxies interact with the circumgalactic medium (CGM) requires determining how galaxies morphological and stellar properties correlate with their CGM properties.…
ALMACAL X: Constraints on molecular gas in the low-redshift circumgalactic medium
Anne Klitsch, Timothy A. Davis, Aleksandra Hamanowicz +3
Despite its crucial role in galaxy evolution, the complex circumgalactic medium (CGM) remains underexplored. Although it is known to be multi-phase, the importance of the molecular…
MUSE-ALMA Haloes VIII: Statistical Study of Circumgalactic Medium Gas
Simon Weng, Céline Péroux, Arjun Karki +15
The distribution of gas and metals in the circumgalactic medium (CGM) plays a critical role in how galaxies evolve. The MUSE-ALMA Halos survey combines MUSE, ALMA and HST observati…
MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
Céline Péroux, Simon Weng, Arjun Karki +16
The gas cycling in the circumgalactic regions of galaxies is known to be multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength observational sample of absorptio…