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. 2022 Mar;603(7903):815-818.
doi: 10.1038/s41586-022-04449-y. Epub 2022 Mar 30.

A highly magnified star at redshift 6.2

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Free article

A highly magnified star at redshift 6.2

Brian Welch et al. Nature. 2022 Mar.
Free article

Erratum in

  • Author Correction: A highly magnified star at redshift 6.2.
    Welch B, Coe D, Diego JM, Zitrin A, Zackrisson E, Dimauro P, Jiménez-Teja Y, Kelly P, Mahler G, Oguri M, Timmes FX, Windhorst R, Florian M, de Mink SE, Avila RJ, Anderson J, Bradley L, Sharon K, Vikaeus A, McCandliss S, Bradač M, Rigby J, Frye B, Toft S, Strait V, Trenti M, Sharma S, Andrade-Santos F, Broadhurst T. Welch B, et al. Nature. 2023 Aug;620(7972):E10. doi: 10.1038/s41586-023-06125-1. Nature. 2023. PMID: 37468641 No abstract available.

Abstract

Galaxy clusters magnify background objects through strong gravitational lensing. Typical magnifications for lensed galaxies are factors of a few but can also be as high as tens or hundreds, stretching galaxies into giant arcs1,2. Individual stars can attain even higher magnifications given fortuitous alignment with the lensing cluster. Recently, several individual stars at redshifts between approximately 1 and 1.5 have been discovered, magnified by factors of thousands, temporarily boosted by microlensing3-6. Here we report observations of a more distant and persistent magnified star at a redshift of 6.2 ± 0.1, 900 million years after the Big Bang. This star is magnified by a factor of thousands by the foreground galaxy cluster lens WHL0137-08 (redshift 0.566), as estimated by four independent lens models. Unlike previous lensed stars, the magnification and observed brightness (AB magnitude, 27.2) have remained roughly constant over 3.5 years of imaging and follow-up. The delensed absolute UV magnitude, -10 ± 2, is consistent with a star of mass greater than 50 times the mass of the Sun. Confirmation and spectral classification are forthcoming from approved observations with the James Webb Space Telescope.

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References

    1. Rivera-Thorsen, T. E. et al. The Sunburst Arc: direct Lyman α escape observed in the brightest known lensed galaxy. Astron. Astrophys. 608, L4 (2017). - DOI
    1. Johnson, T. L. et al. Star formation at z = 2.481 in the lensed galaxy SDSS J1110+6459: star formation down to 30 pm scales. Astrophys. J. Lett. 843, L21 (2017). - PubMed - PMC - DOI
    1. Kelly, P. L. et al. Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens. Nat. Astron. 2, 334–342 (2018). - DOI
    1. Rodney, S. A. et al. Two peculiar fast transients in a strongly lensed host galaxy. Nat. Astron. 2, 324–333 (2018). - DOI
    1. Chen, W. et al. Searching for highly magnified stars at cosmological distances: discovery of a redshift 0.94 supergiant in archival images of the galaxy cluster MACS J0416.1-2403. Astrophys. J. 881, 8 (2019). - DOI

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