Astronomia UDP

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The ALMA CRISTAL large program

The ALMA CRISTAL large program (PI: R. Herrera-Camus; co-PIs: M. Aravena, J. González-López et al.) is designed to provide unique constraints on the morphologies, kinematics, existence of outflows, and ISM properties of galaxies at z=4-6. Our group is focused on the study of the interplay between the ISM and CGM of galaxies by characterizing the full baryonic cycle through observations of Ly-alpha, [CII], H-alpha, etc. with ALMA, VLT/MUSE, Keck/KCWI and JWST.

Type of project: Research – actively recruiting new young researchers
Status: Ongoing
Researchers: Manuel Aravena, Jorge Gonzalez-Lopez, Manuel Solimano, Ana Posses, Kseniia Telikova, Meghana Killi, Roberto Assef
Funding source: FONDECYT Regular, ALMA-ANID, Basal CATA2, NASA

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