JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8 sigma Confidence
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Riess, AG; Anand, GS; Yuan, W; Macri, LM; Casertano, S; Dolphin, A; Breuval, L; Scolnic, D; Perrin, M; Anderson, RI
January 9, 2024
Duke Scholars
Publication Date
January 9, 2024
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Riess, A. G., Anand, G. S., Yuan, W., Macri, L. M., Casertano, S., Dolphin, A., … Anderson, R. I. (2024). JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as
an Explanation for the Hubble Tension at 8 sigma Confidence.
Riess, Adam G., Gagandeep S. Anand, Wenlong Yuan, Lucas M. Macri, Stefano Casertano, Andrew Dolphin, Louise Breuval, Dan Scolnic, Marshall Perrin, and Richard I. Anderson. “JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as
an Explanation for the Hubble Tension at 8 sigma Confidence,” January 9, 2024.
Riess AG, Anand GS, Yuan W, Macri LM, Casertano S, Dolphin A, et al. JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as
an Explanation for the Hubble Tension at 8 sigma Confidence. 2024.
Riess, Adam G., et al. JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as
an Explanation for the Hubble Tension at 8 sigma Confidence. 9 Jan. 2024.
Riess AG, Anand GS, Yuan W, Macri LM, Casertano S, Dolphin A, Breuval L, Scolnic D, Perrin M, Anderson RI. JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as
an Explanation for the Hubble Tension at 8 sigma Confidence. 2024.
Publication Date
January 9, 2024