Is the Bremer Deep Field reionized, at z ∼ 7?
Author:
Affiliation:
1. Instituto de Astrofísica de Canarias, E-38205 La Laguna, Spain
2. Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain
3. Departamento de Astrofísica, Centro de Astrobiología (CSIC-INTA), E-28850 Madrid, Spain
Abstract
Funder
Agencia Estatal de Investigación
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stab545/36422490/stab545.pdf
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3. z∼ 7 GALAXY CANDIDATES FROM NICMOS OBSERVATIONS OVER THE HDF-SOUTH AND THE CDF-SOUTH AND HDF-NORTH GOODS FIELDS
4. UV LUMINOSITY FUNCTIONS AT REDSHIFTSz∼ 4 TOz∼ 10: 10,000 GALAXIES FROMHSTLEGACY FIELDS
5. THE LYMAN-CONTINUUM PHOTON PRODUCTION EFFICIENCYξIONOFz∼ 4–5 GALAXIES FROM IRAC-BASED HαMEASUREMENTS: IMPLICATIONS FOR THE ESCAPE FRACTION AND COSMIC REIONIZATION
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1. Lyα Emitting Galaxies (LAEs) at Cosmic Dawn: Implications and Predictions;The Astrophysical Journal;2022-09-01
2. The ionizing properties of two bright Lyα emitters in the Bremer Deep Field reionized bubble at z = 7;Astronomy & Astrophysics;2022-06
3. Strong Lyman-α emission in an overdense region at z = 6.8: a very large (R ∼ 3 physical Mpc) ionized bubble in COSMOS?;Monthly Notices of the Royal Astronomical Society;2022-02-25
4. Near-IR narrow-band imaging with CIRCE at the Gran Telescopio Canarias: Searching for Lyalpha-emitters at z~9.3;Astronomy & Astrophysics;2021-12-24
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