Image Details

Choose export citation format:

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies

  • Authors: Manuel Aravena, Roberto Decarli, Jorge Gónzalez-López, Leindert Boogaard, Fabian Walter, Chris Carilli, Gergö Popping, Axel Weiss, Roberto J. Assef, Roland Bacon, Franz Erik Bauer, Frank Bertoldi, Richard Bouwens, Thierry Contini, Paulo C. Cortes, Pierre Cox, Elisabete da Cunha, Emanuele Daddi, Tanio Díaz-Santos, David Elbaz, Jacqueline Hodge, Hanae Inami, Rob Ivison, Olivier Le Fèvre, Benjamin Magnelli, Pascal Oesch, Dominik Riechers, Ian Smail, Rachel S. Somerville, A. M. Swinbank, Bade Uzgil, Paul van der Werf, Jeff Wagg, and Lutz Wisotzki

2019 The Astrophysical Journal 882 136.

  • Provider: AAS Journals

Caption: Figure 2.

CO line emission profiles obtained from the ALMA 3 mm data cube, toward the 16 most significant CO-selected detections. The spectra are centered at the identified line, and shown at a width of 7.813 MHz per channel (∼25 km s−1). For the sources in the bottom row, the spectra have been rebinned by a factor of 2. The red solid line, represents a one-dimensional Gaussian fit to the profiles. The profiles are obtained by extracting the spectra in the original cube, at the location of the peak position identified in the moment-0 image. The gray shaded area corresponds to the velocity range used to obtain the moment-0 images used in Figure 1.

Other Images in This Article

Show More

Copyright and Terms & Conditions