Spectroscopic and imaging data for low metallicity galaxies observed during the peak epoch of star formation offer detailed insights into the most distant galaxies discovered to date.
References
Bouwens, R. J. et al. Astrophys. J. 803, 34 (2015).
Finkelstein, S. L. et al. Astrophys. J. 810, 71 (2015).
Stark, D. P. et al. Mon. Not. R. Astron. Soc. 450, 1846–1855 (2015).
Stark, D. P. et al. Mon. Not. R. Astron. Soc. 454, 1393–1403 (2015).
Stark, D. P. et al. Mon. Not. R. Astron. Soc. 464, 469–479 (2017).
Amorín, R. et al. Nat. Astron. 1, 0052 (2017).
Dunlop, J. S. et al. Mon. Not. R. Astron. Soc. 432, 3520–3533 (2013).
Smit, R. et al. Astrophys. J. 784, 58 (2014).
Oesch, P. A. et al. Astrophys. J. Lett. 709, L21–L25 (2010).
Le Fèvre, O. et al. Astron. Astrophys. 576 A79 (2015).
Heckman, T. M. Astron. Soc. Pac. Conf. Proc. 254, 292–304 (2002).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Shapley, A. Galaxies: Primeval twins. Nat Astron 1, 0054 (2017). https://doi.org/10.1038/s41550-017-0054
Published:
DOI: https://doi.org/10.1038/s41550-017-0054
- Springer Nature Limited