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The evolution of the OII, H\beta and OIII emission-line luminosity functions

, , , , , , , , , , , , , , и . (2016)cite arxiv:1605.02875Comment: 11 pages. Submitted to MNRAS. Data available at http://projects.ift.uam-csic.es/skies-universes/ via the page emission line luminosity functions.

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Gabriele Norberg

Kurt Norberg

Madlena Norberg

Bertel Norberg

Ulf Norberg

 

Другие публикации лиц с тем же именем

The evolution of the OII, H\beta and OIII emission-line luminosity functions, , , , , , , , , и 5 other автор(ы). (2016)cite arxiv:1605.02875Comment: 11 pages. Submitted to MNRAS. Data available at http://projects.ift.uam-csic.es/skies-universes/ via the page emission line luminosity functions.The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes, , , , , , , , , и 10 other автор(ы). (2017)cite arxiv:1706.02704Comment: 11 pages, 8 figures. Submitted for publication in A&A.