MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues

Monthly Notices of the Royal Astronomical Society, Volume 516, Issue 4, November 2022, Pages 5618-5636 November 2022 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 absorption a...

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Hauptverfasser: Péroux, Céline, Weng, Simon, Karki, Arjun, Augustin, Ramona, Kulkarni, Varsha P, Szakacs, Roland, Klitsch, Anne, Hamanowicz, Aleksandra, Fresco, Alejandra Y, Zwaan, Martin A, Biggs, Andrew, Fox, Andrew J, Hayes, Mattjew, Howk, J. Christopher, Kacprzak, Glenn G, Kassin, Susan, Kuntschner, Harald, Nelson, Dylan, Pettini, Max
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Sprache:eng
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Zusammenfassung:Monthly Notices of the Royal Astronomical Society, Volume 516, Issue 4, November 2022, Pages 5618-5636 November 2022 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 absorption and emission data with the goal to significantly advance our understanding of the physical properties of such CGM gas. A key component of the MUSE-ALMA Haloes survey is the multi-facility observational campaign conducted with VLT/MUSE, ALMA and HST. MUSE-ALMA Haloes targets comprise 19 VLT/MUSE IFS quasar fields, including 32 $z_{\rm abs}
DOI:10.48550/arxiv.2211.16517