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We introduce a new method for measuring the Hubble parameter from low-redshift large-scale observations that is independent of the comoving sound horizon.
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2022
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2011
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2013
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B. Audren, J. Lesgourgues, K. Benabed, and S. Prunet, JCAP 1302
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2014
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2024
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J. A. Kable and V. Miranda, arXiv e-prints , arXiv:2403.11916 (2024), arXiv:2403.11916 [astro-ph.CO]
2024
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2024
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2024
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2024
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N. Schöneberg, arXiv e-prints , arXiv:2401.15054 (2024) , arXiv:2401.15054 [astro-ph.CO]
2024
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A.-K. Burns, T. M. P. Tait, and M. Valli, European Physical Journal C 84
2024
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2024
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Removing the ∼ \sim 9000 deg 2 overlap between Euclid and DESI from the DESI effective volume, since Euclid has higher number density
2026
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