Abstract
The SH0ES collaboration Hubble constant determination is in a ∼5σ difference with the Planck value, known as the Hubble tension. The accuracy of the Hubble constant measured with extragalactic Cepheids depends on robust stellar-crowding background estimation. Riess et al. (R20) compared the light-curve amplitudes of extragalactic and MW Cepheids to constrain an unaccounted systematic blending bias, γ = −0.029 ± 0.037 mag, which cannot explain the required, γ = 0.24 ± 0.05 mag, to resolve the Hubble tension. Further checks by Riess et al. demonstrate that a possible blending is not likely related to the size of the crowding correction. We repeat the R20 analysis, with the following main differences: (1) we limit the extragalactic and MW Cepheids comparison to periods P ≲50 d, since the number of MW Cepheids with longer periods is minimal; (2) we use publicly available data to recalibrate amplitude ratios of MW Cepheids in standard passbands; (3) we remeasure the amplitudes of Cepheids in NGC 5584 and NGC 4258 in two Hubble Space Telescope filters (F555W and F350LP) to improve the empirical constraint on their amplitude ratio A555/A350. We show that the filter transformations introduce an ≈0.04 mag uncertainty in determining γ, not included by R20. While our final estimate, γ = 0.013 ± 0.057 mag, is consistent with the value derived by R20 and is consistent with no bias, the error is somewhat larger, and the best-fitting value is shifted by ≈0.04 mag and closer to zero. Future observations, especially with JWST, would allow better calibration of γ.
Original language | English |
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Pages (from-to) | 6861-6880 |
Number of pages | 20 |
Journal | Monthly notices of the Royal Astronomical Society |
Volume | 528 |
Issue number | 4 |
Early online date | 14 Feb 2024 |
DOIs | |
Publication status | Published - 1 Mar 2024 |
Bibliographical note
We thank Ondřej Pejcha, Dan Scolnic, Stefano Casertano, Eli Waxman, Boaz Katz, and Eran Ofek for useful discussions. DK is supported by the Israel Atomic Energy Commission – The Council for Higher Education – Pazi Foundation, by a research grant from The Abramson Family Center for Young Scientists, by ISF grant, and by the Minerva Stiftung. This research has made use of the International Variable Star Index (VSX) data base, operated at AAVSO, Cambridge, Massachusetts, USA.Publisher Copyright:
© 2024 The Author(s).
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science