摘要：Assessing the significance and implications of the recently established Hubble tension requires the comprehensive identification, quantification, and mitigation of uncertainties and/or biases affectingH0measurements. Here, we investigate the previously overlooked distance scale bias resulting from the interplay between redshift and Leavitt laws in an expanding Universe: Redshift-Leavitt bias (RLB). Redshift dilates oscillation periods of pulsating stars residing in supernova-host galaxies relative to periods of identical stars residing in nearby (anchor) galaxies. Multiplying dilated logPwith Leavitt Law slopes leads to underestimated absolute magnitudes, overestimated distance moduli, and a systematic error onH0. Emulating the SH0ES distance ladder, we estimate an associatedH0bias of (0.27 ± 0.01)% and obtain a correctedH0 = 73.70 ± 1.40 km s−1Mpc−1. RLB becomes increasingly relevant as distance ladder calibrations pursue greater numbers of ever more distant galaxies hosting both Cepheids (or Miras) and type-Ia supernovae. The measured periods of oscillating stars can readily be corrected for heliocentric redshift (e.g. of their host galaxies) in order to ensureH0measurements free of RLB.
