On the AGN nature of two UV bright sources at z_spec~5.5 in the CANDELS fields: an update of the AGN...
On the AGN nature of two UV bright sources at z_spec~5.5 in the CANDELS fields: an update of the AGN space density at M1450~-22.5
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Author / Creator
Grazian, A , Giallongo, E , Fiore, F , Boutsia, K , Civano, F , Cristiani, S , Cupani, G , Dickinson, M , Fontanot, F , Menci, N and Romano, M
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
It is a widespread opinion that hydrogen reionization is mainly driven by primeval star-forming galaxies, with a minor role of high-z active galactic nuclei. Recent observations, however, challenge this notion, indicating a number of issues related to a galaxy-driven reionization scenario. We provide here an updated assessment of the space density...
Alternative Titles
Full title
On the AGN nature of two UV bright sources at z_spec~5.5 in the CANDELS fields: an update of the AGN space density at M1450~-22.5
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Record Identifier
TN_cdi_proquest_journals_2409767520
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2409767520
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2006.02451
