Towards a 1% Measurement of the Hubble Constant: Accounting for Time Dilation in Variable Star Light Curves
arXiv:1909.10847 · doi:10.1051/0004-6361/201936585
Abstract
Assessing the significance and implications of the recently established Hubble tension requires the comprehensive identification, quantification, and mitigation of uncertainties and/or biases affecting measurements. 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 with Leavitt Law slopes leads to underestimated absolute magnitudes, overestimated distance moduli, and a systematic error on . Emulating the SH0ES distance ladder, we estimate an associated bias of % and obtain a corrected . 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 ensure measurements free of RLB.
Astronomy & Astrophysics in press. 6 pages, 5 figures, 1 table; V2 contains minor corrections following proofing stage
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