An individual star at extremely high redshift is observed due to gravitational lensing by a foreground galaxy cluster, magnifying it by a factor of over a thousand.
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References
Kelly, P. L. et al. Nat. Astron 2, 334–342 (2018).
Welch, B. et al. Nature https://doi.org/10.1038/s41586-022-04449-y (2022).
Coe, D. et al. Astrophys. J. 884, 85 (2019).
Rivera-Thorsen, T. E. et al. Astron. Astrophys. 608, L4 (2017).
Abbott, B. P. et al. Phys. Rev. Lett. 125, 101102 (2020).
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Wong, K.C. A star from the dawn of the Universe. Nat Astron 6, 527–528 (2022). https://doi.org/10.1038/s41550-022-01674-3
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DOI: https://doi.org/10.1038/s41550-022-01674-3