The DOI matches its Crossref record; 173 of the 173 references it cites were found in a registry or an index.
Observational Constraints on Cosmic Reionization
Open accessAbstract
Observations have set the first constraints on the epoch of reionization (EoR), corresponding to the formation epoch of the first luminous objects. Studies of Gunn-Peterson (GP) absorption indicate a rapid increase in the neutral fraction of the intergalactic medium (IGM) from x HI< 10−4 at z ≤ 5.5, to x HI> 10−3, perhaps up to 0.1, at z∼6, while the large scale polarization of the cosmic microwave background (CMB) implies a significant ionization fraction extending to higher redshifts, z∼11 ± 3. These results, as well as observations of galaxy populations, suggest that reionization is a process that begins as early as z∼14, and ends with the “percolation” phase at z∼6 to 8. Low luminosity star-forming galaxies are likely the dominant sources of reionizing photons. Future low-frequency radio telescopes will make direct measurements of HI 21-cm emission from the neutral IGM during the EoR, and measurements of secondary CMB temperature anisotropy will provide details of the dynamics of the reionized IGM.
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Cited by
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New cosmological constraints on primordial black holes
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Constraints on primordial black holes
Carr, B., Kohri, K., Sendouda, Y., & Yokoyama, J. (2021) · Reports on Progress in Physics · doi:10.1088/1361-6633/ac1e31 · Cited by 1,156
Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
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Metadata
- Authors
- Fan, X., Carilli, C. L., & Keating, B.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2006-09-01
- Volume
- 44
- Issue
- 1
- Pages
- 415-462
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2136969532
- Cited by
- 788
- References
- 173
- FWCI
- 6.03
- Type
- journal article
- Language
- en
- Open access
- green
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