The ALMA REBELS survey: cosmic dust temperature evolution out to z ~ 7

Author(s):
Sommovigo, L.; Ferrara, A.; Pallottini, A.; Dayal, P.; Bouwens, R.J. (0000-0002-4989-2471); Smit, R.; da Cunha, E.; De Looze, I.; Bowler, R.A.A.; Hodge, J.A. (0000-0001-6586-8845); Inami, H.; Oesch, P.; Endsley, R.; Gonzalez, V.; Schouws, S.T.M.; Stark, D.; Stefanon, M. (0000-0001-7768-5309); Aravena, M.; Graziani, L.; Riechers, D.; Schneider, R.; Werf, P.P. van der (0000-0002-4389-832x); Algera, H.; Barrufet, L.; Fudamoto, Y.; Hygate, A.P.S.; Labbé, I.; Li, Y.; Nanayakkara, T.; Topping, M.
Published
2022
Publication type
Article / Letter to editor
Methods - analyticalMethods - data analysisDustExtinctionGalaxies - high-redshiftInfrared - ISMAstrophysics - astrophysics of galaxies
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 513, no. 3, p. 3122-3135
hdl
1887/3514929
doi
10.1093/mnras/stac302
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.513.3122S