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astro-ph.GA2025
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
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
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…