GOODS-ALMA: The slow downfall of star formation in z = 2-3 massive galaxies

M. Franco*, D. Elbaz, L. Zhou, B. Magnelli, C. Schreiber, L. Ciesla, M. Dickinson, N. Nagar, G. Magdis, D. M. Alexander, M. Béthermin, R. Demarco, E. Daddi, T. Wang, J. Mullaney, M. Sargent, H. Inami, X. Shu, F. Bournaud, R. CharyR. T. Coogan, H. Ferguson, S. L. Finkelstein, M. Giavalisco, C. Gómez-Guijarro, D. Iono, S. Juneau, G. Lagache, L. Lin, K. Motohara, K. Okumura, M. Pannella, C. Papovich, A. Pope, W. Rujopakarn, J. Silverman, M. Xiao

*Corresponding author for this work

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    Abstract


    We investigate the properties of a sample of 35 galaxies, detected with the Atacama Large Millimeter/Submillimeter Array (ALMA) at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin2, resolution = 0.60″, rms ≃ 0.18 mJy beam−1). Using the ultraviolet-to-radio deep multiwavelength coverage of the GOODS–South field, we fit the spectral energy distributions of these galaxies to derive their key physical properties.
    Original languageEnglish
    Article numberA30
    JournalAstronomy and Astrophysics
    Volume643
    Number of pages17
    ISSN0004-6361
    DOIs
    Publication statusPublished - 2020

    Keywords

    • Galaxies: active
    • Galaxies: evolution
    • Galaxies: fundamental parameters
    • Galaxies: high-redshift
    • Galaxies: star formation
    • Submillimeter: galaxies

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