No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-$α$ emitter 'CR7'
The z = 6.6 Lyman-$\alpha$ emitter 'CR7' has been claimed to have a Population III-like stellar population, or alternatively, be a candidate Direct Collapse Black Hole (DCBH). In this paper we investigate the evidence for these exotic scenarios using recently available, deeper, optical, ne...
| Hoofdauteurs: | , , , , , , |
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| Formaat: | Journal article |
| Gepubliceerd in: |
Oxford University Press
2017
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