The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.
A galaxy at a redshift z = 6.96
Open accessAbstract
When galaxy formation started in the history of the Universe remains unclear. Studies of the cosmic microwave background indicate that the Universe, after initial cooling (following the Big Bang), was reheated and reionized by hot stars in newborn galaxies at a redshift in the range 6 < z < 14 (ref. 1). Though several candidate galaxies at redshift z > 7 have been identified photometrically, galaxies with spectroscopically confirmed redshifts have been confined to z < 6.6 (refs 4–8). Here we report a spectroscopic redshift of z = 6.96 (corresponding to just 750 Myr after the Big Bang) for a galaxy whose spectrum clearly shows Lyman-α emission at 9,682 Å, indicating active star formation at a rate of ∼10M[circdot] yr-1, where M[circdot] is the mass of the Sun. This demonstrates that galaxy formation was under way when the Universe was only ∼6 per cent of its present age. The number density of galaxies at z ≈ 7 seems to be only 18–36 per cent of the density at z = 6.6.
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Cites
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Bruzual, G., & Charlot, S. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06897.x · Cited by 10,500
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
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Star Formation in Galaxies Along the Hubble Sequence
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Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Polarization Analysis
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Cited by
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The Hyper Suprime-Cam SSP Survey: Overview and survey design
Aihara, H., Arimoto, N., Armstrong, R., Arnouts, S., Bahcall, N. A., Bickerton, S., Bosch, J., Bundy, K., Capak, P. L., Chan, J. H. H., et al. (2018) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx066 · Cited by 1,087
Self-citationTHE CLUSTER LENSING AND SUPERNOVA SURVEY WITH HUBBLE: AN OVERVIEW
Postman, M., Coe, D., Benítez, N., Bradley, L., Broadhurst, T., Donahue, M., Ford, H., Graur, O., Graves, G., Jouvel, S., et al. (2012) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/199/2/25 · Cited by 849
A γ-ray burst at a redshift of z ≈ 8.2
Tanvir, N. R., Fox, D. B., Levan, A. J., Berger, E., Wiersema, K., Fynbo, J. P. U., Cucchiara, A., Krühler, T., Gehrels, N., Bloom, J. S., et al. (2009) · Nature · doi:10.1038/nature08459 · Cited by 624
Massive primordial black holes from hybrid inflation as dark matter and the seeds of galaxies
Clesse, S., & García-Bellido, J. (2015) · Physical Review D · doi:10.1103/physrevd.92.023524 · Cited by 471
Metadata
- Authors
- Iye, M., Ota, K., Kashikawa, N., Furusawa, H., Hashimoto, T., Hattori, T., Matsuda, Y., Morokuma, T., Ouchi, M., & Shimasaku, K.
- Venue
- Nature
- Published
- 2006-09
- Volume
- 443
- Issue
- 7108
- Pages
- 186-188
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2029178265
- Cited by
- 295
- References
- 23
- FWCI
- 20.63
- Type
- journal article
- Language
- en
- Open access
- green
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- Iye, M., Ota, K., Kashikawa, N., Furusawa, H., Hashimoto, T., Hattori, T., Matsuda, Y., Morokuma, T., Ouchi, M., & Shimasaku, K. (2006). A galaxy at a redshift z = 6.96. Nature. https://doi.org/10.1038/nature05104
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