Abstract
Abstract We present Hubble Space Telescope (HST) photometry of a selected sample of 50 long-period, low-extinction Milky Way Cepheids measured on the same WFC3 F555W-, F814W-, and F160W-band photometric system as extragalactic Cepheids in Type Ia supernova host galaxies. These bright Cepheids were observed with the WFC3 spatial scanning mode in the optical and near-infrared to mitigate saturation and reduce pixel-to-pixel calibration errors to reach a mean photometric error of 5 mmag per observation. We use the new Gaia DR2 parallaxes and HST photometry to simultaneously constrain the cosmic distance scale and to measure the DR2 parallax zeropoint offset appropriate for Cepheids. We find the latter to be −46 ± 13 μas or ±6 μas for a fixed distance scale, higher than found from quasars, as expected for these brighter and redder sources. The precision of the distance scale from DR2 has been reduced by a factor of 2.5 because of the need to independently determine the parallax offset. The best-fit distance scale is 1.006 ± 0.033, relative to the scale from Riess et al. with H 0 = 73.24 km s−1 Mpc−1 used to predict the parallaxes photometrically, and is inconsistent with the scale needed to match the Planck 2016 cosmic microwave background data combined with ΛCDM at the 2.9σ confidence level (99.6%). At 96.5% confidence we find that the formal DR2 errors may be underestimated as indicated. We identify additional errors associated with the use of augmented Cepheid samples utilizing ground-based photometry and discuss their likely origins. Including the DR2 parallaxes with all prior distance-ladder data raises the current tension between the late and early universe route to the Hubble constant to 3.8σ (99.99%). With the final expected precision from Gaia, the sample of 50 Cepheids with HST photometry will limit to 0.5% the contribution of the first rung of the distance ladder to the uncertainty in H 0.
Highlights
Measurements of cosmic distances from standard candles form a cornerstone of our cosmological model
We present Hubble Space Telescope (HST) photometry of a selected sample of 50 long-period, lowextinction Milky Way Cepheids measured on the same WFC3 F 555W, F 814W, and F 160W -band photometric system as extragalactic Cepheids in Type Ia supernova host galaxies
We have presented an analysis of the Gaia DR2 parallax values and their uncertainties for a carefully selected sample of 50 Cepheids with precise, consistent photometry obtained with HST using spatial scanning observations
Summary
Measurements of cosmic distances from standard candles form a cornerstone of our cosmological model. Spatial scanning with HST’s WFC3 has provided relative astrometry with 30–40 μas precision to extend the useful range of Cepheid parallaxes to 2–4 kpc, measuring 8 with P ≥ 10 days with an error in the mean distance of 3% and providing a calibration more applicable to extragalactic Cepheid samples (Riess et al 2014; Casertano et al 2016; Riess et al 2018). To retain the precision of Gaia’s Cepheid parallaxes when they are used as standard candles it is necessary to measure their mean brightness on the same photometric systems used to measure their extragalactic counterparts By using such purely differential flux measurements of Cepheids along the distance ladder, it is possible to circumvent systematic uncertainties related to zeropoints and transmission functions which otherwise incur a systematic uncertainty of ∼ 2–3% in the determination of H0, nearly twice the target goal, even before including additional uncertainties along the distance ladder.
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