The ALMA REBELS survey: the dust content of z ~ 7 Lyman break galaxies

Author(s):
Dayal, P.; Ferrara, A.; Sommovigo, L.; Bouwens, R.J. (0000-0002-4989-2471); Oesch, P.A.; Smit, R.; Gonzalez, V.; Schouws, S.T.M.; Stefanon, M. (0000-0001-7768-5309); Kobayashi, C.; Bremer, J.; Algera, H.S.B.; Aravena, M.; Bowler, R.A.A.; da Cunha, E.; Fudamoto, Y.; Graziani, L.; Hodge, J.A. (0000-0001-6586-8845); Inami, H.; De Looze, I.; Pallottini, A.; Riechers, D.; Schneider, R.; Stark, D.; Endsley, R.
Published
2022
Publication type
Article / Letter to editor
DustExtinctionGalaxies - evolutionGalaxies - high-redshiftGalaxies - ISMGalaxies - luminosity functionMass functionAstrophysics - astrophysics of galaxies
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 512, no. 1, p. 989-1002
hdl
1887/3514937
doi
10.1093/mnras/stac537
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.512..989D