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STELLAR ASTROPHYSICS

An improved stellar yardstick in the shadows

Measurement of the diffraction pattern of starlight during an asteroid occultation opens up new territory in stellar angular size determinations.

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References

  1. 1.

    Boyajian, T. S. et al. Astrophys. J. 746, 101 (2012).

  2. 2.

    Brown, A. G. A. et al. (Gaia Collaboration). Astron. Astrophys. 616, A1 (2018).

  3. 3.

    Korngut, P. M. et al. Proc. SPIE 10698, 106981U (2018).

  4. 4.

    Michelson, A. A. & Pease, F. G. Astrophys. J. 53, 249–259 (1921).

  5. 5.

    Hanbury Brown, R., Davis, J. & Allen, L. R. Mon. Not. R. Astron. Soc. 167, 121–136 (1974).

  6. 6.

    Nather, R. E. & Evans, D. S. Astron. J. 75, 575–582 (1970).

  7. 7.

    Ridgway, S. T., Wells, D. C. & Joyce, R. R. Astron. J. 82, 414–430 (1977).

  8. 8.

    Whitford, A. E. Astrophys. J. 89, 472–481 (1939).

  9. 9.

    Benbow, W. et al. Nat. Astron. https://doi.org/10.1038/s41550-019-0741-z (2019).

  10. 10.

    Nather, R. E. & McCants, M. M. Astron. J. 75, 963–970 (1970).

  11. 11.

    Matthews, N., Clarke, O., Snow, S., LeBohec, S. & Kieda, D. Proc. SPIE 10701, 107010W (2018).

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Correspondence to Gerard T. van Belle.

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https://doi.org/10.1038/s41550-019-0758-3

Fig. 1

Steve Criswell, Smithsonian Astrophysical Observatory