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

Research output: Contribution to journalJournal articleResearchpeer-review

12 Downloads (Pure)

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

Fingerprint

Dive into the research topics of 'GOODS-ALMA: The slow downfall of star formation in z = 2-3 massive galaxies'. Together they form a unique fingerprint.

Cite this