Image Details
Caption: Figure 5.
Results of the bootstrap procedure to compare Cepheid amplitudes derived from our work (red) and from (Monson & Pierce 2011, black). Top: Binned and phase-folded light curves; solid lines show the best-fit templates. The red and black shaded regions represent the 1σ intervals. Bottom: Results of 1000 bootstrap samplings (with replacement) to estimate the uncertainty on the best-fit amplitudes. We find agreement between the two data sets at the 1.1–1.4σ level.
© 2022. The Author(s). Published by the American Astronomical Society.