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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…
ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
Jianhang Chen, R. J. Ivison, Martin A. Zwaan +8
Wide, deep, blind continuum surveys at submillimetre/millimetre (submm/mm) wavelengths are required to provide a full inventory of the dusty, distant Universe. However, conducting…
ALMACAL VIII: A pilot survey for untargeted extragalactic CO emission lines in deep ALMA calibration data
Aleksandra Hamanowicz, Martin A. Zwaan, Céline Péroux +6
We present a pilot, untargeted extragalactic carbon monoxide (CO) emission-line survey using ALMACAL, a project utilizing ALMA calibration data for scientific purposes. In 33 deep…
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. IV. Calibration of Dust Depletions vs Abundance Ratios in the Milky Way and Magellanic Clouds and Application to Damped Lyman-alpha Systems
Julia Roman-Duval, Edward B. Jenkins, Kirill Tchernyshyov +9
The evolution of the metal content of the universe can be tracked through rest-frame UV spectroscopy of damped Ly- systems (DLAs). Gas-phase abundances in DLAs must be corrected…
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity
J. Roman-Duval, E. B. Jenkins, K. Tchernyshyov +9
The metallicity and gas density dependence of interstellar depletions, the dust-to-gas (D/G), and dust-to-metal (D/M) ratios have important implications for how accurately we can t…