activity
20232026
most citedPolarized thermal emission from dust in a galaxy at redshift 2.6

40 citations · 62 across the 8 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2026

MUSE-ALMA Haloes XIV: The ALMA Large Programme Data Release

Céline Péroux, Jianhang Chen, Victoria Bollo +10

The interactions between gas and galaxies are of paramount importance to our understanding of structure formation. A fundamental element of such baryon cycle studies is a complete…

astro-ph.GA2026★ 1 cited

MUSE-ALMA Haloes XIII. Molecular gas in HI-selected galaxies

Victoria Bollo, Celine Peroux, Martin Zwaan +11

We present new results from the MUSE-ALMA Haloes survey, covering 79 galaxies associated with strong HI absorption at redshift about 0.5. Our ALMA Cycle 10 observations add 39 syst…

astro-ph.GA2025

ALMACAL XIV: X-Shooter Spectroscopy, Infrared Properties and Radio SEDs of Calibrators

Simon Weng, Elaine M. Sadler, Emily Kerrison +8

The ALMACAL-22 survey includes over 2700 hours of observations of ALMA phase and amplitude calibrators, spanning frequencies from 84 to 950 GHz across bands 3 to 10. In total, 687…

astro-ph.GA2025★ 5 cited

ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to ~ 6

Victoria Bollo, Céline Péroux, Martin Zwaan +7

Cold molecular gas, largely traced by CO emission, is the primary fuel for star formation, making it essential for understanding galaxy evolution. ALMA has made significant progres…

astro-ph.GA2024★ 3 cited

Deep kiloparsec view of the molecular gas in a massive star-forming galaxy at cosmic noon

Sebastián Arriagada-Neira, Rodrigo Herrera-Camus, Vicente Villanueva +10

We present deep ( 20 hr), high-angular resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations of the and transitions,…

astro-ph.GA2024

ALMACAL XII. Data characterisation and products

Victoria Bollo, Martin Zwaan, Celine Peroux +5

The ALMACAL survey is based on a database of reprocessed ALMA calibration scans suitable for scientific analysis, observed as part of regular PI observations. We present all the da…

astro-ph.GA2024★ 13 cited

A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6

Jianhang Chen, Enrique Lopez-Rodriguez, R. J. Ivison +4

Magnetic fields are widely observed in various astronomical contexts, yet much remains unknown about their significance across different systems and cosmic epochs. Our current know…

astro-ph.GA2024

Licking the plate: dusty star-forming galaxies buried in the ALMA calibration data

Jianhang Chen, R. J. Ivison, M. Zwaan +2

Deep, unbiased surveys are essential to decipher the cosmic evolution of galaxies. The submillimetre (submm) and millimetre (mm) windows complement the UV/optical waveband and are…

astro-ph.GA2023★ 40 cited

Polarized thermal emission from dust in a galaxy at redshift 2.6

J. E. Geach, E. Lopez-Rodriguez, M. J. Doherty +5

Magnetic fields are fundamental to the evolution of galaxies, playing a key role in the astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic fie…