Table D.1.
Results from the Photometric parallax method with the MCMC algorithm for the WHVI magnitude applied to the sample of DCEPs by Riess et al. (2021) (see text).
| α | β | γ | ϵ | source |
|---|---|---|---|---|
| -5.915±0.030 | -3.28±0.06 | -0.20±0.13 | -0.014±0.006 | R21 |
| -5.960±0.035 | -3.33±0.07 | -0.18±0.13 | -0.024±0.007 | HM25 |
| -5.960±0.035 | -3.33±0.07 | -0.18±0.13 | -0.024±0.007 | TW |
Notes. R21=Riess et al. (2021); HM25=Högås & Mörtsell (2025); TW=This Work.
Note that we have rounded central values and the errors for the β and γ parameters compared with Fig. D.1, to be homogeneous with the literature results. The units of α, β, γ, ϵ and of their uncertainties are mag, mag/dex, mag/dex and mas, respectively.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.