A substantial population of previously unknown massive dusty galaxies during the first two billion years after the Big Bang have been identified with submillimetre observations. They may solve some outstanding puzzles related to the formation and evolution of most massive galaxies in the Universe today.
This is a preview of subscription content, access via your institution
Access options
Access Nature and 54 other Nature Portfolio journals
Get Nature+, our best-value online-access subscription
$29.99 / 30 days
cancel any time
Subscribe to this journal
Receive 12 digital issues and online access to articles
$119.00 per year
only $9.92 per issue
Buy this article
- Purchase on SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Springel, V. et al. Nature 435, 629–636 (2005).
Dekel, A. et al. Nature 457, 451–454 (2009).
Wang, T. et al. Nature 572, 211–214 (2019).
Wang, T. et al. Astrophys. J. 816, 84 (2016).
Grogin, N. A. et al. Astrophys. J. Suppl. Ser. 197, 35 (2011).
Riechers, D. A. et al. Nature 496, 329–333 (2013).
Walter, F. et al. Nature 486, 233–236 (2012).
Marrone, D. P. et al. Nature 553, 51–54 (2018).
Battersby, C. et al. Nat. Astron. 2, 596–599 (2018).
Daddi, I. et al. Astrophys. J. 713, 686–707 (2010).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Cooray, A.R. Optically dark massive galaxies. Nat Astron 3, 885–886 (2019). https://doi.org/10.1038/s41550-019-0894-9
Published:
Issue Date:
DOI: https://doi.org/10.1038/s41550-019-0894-9