The Legacy of Henrietta Leavitt: A Re-analysis of the First Cepheid Period-Luminosity Relation
Louise Breuval, Caroline D. Huang, Adam G. Riess

TL;DR
This paper re-analyzes Henrietta Leavitt's original Cepheid variable star data using modern techniques, confirming her findings and demonstrating improvements in the Period-Luminosity relation's precision, thus reinforcing its importance in cosmology.
Contribution
The study applies contemporary data and methods to Leavitt's original observations, reducing scatter and identifying biases, thereby validating and extending her foundational work.
Findings
Modern analysis reduces scatter of the Period-Luminosity relation by a factor of two.
Leavitt's original results are consistent with current measurements.
Identified bias at short periods due to plate non-linearity and crowding.
Abstract
Henrietta Swan Leavitt's discovery of the relationship between the period and luminosity (hereafter the Leavitt Law) of 25 variable stars in the Small Magellanic Cloud, published in 1912, revolutionized cosmology. These variables, eventually identified as Cepheids, became the first known "standard candles" for measuring extragalactic distances and remain the gold standard for this task today. Leavitt measured light curves, periods, and minimum and maximum magnitudes from painstaking visual inspection of photographic plates. Her work paved the way for the first precise series of distance measurements that helped set the scale of the Universe, and later the discovery of its expansion by Edwin Hubble in 1929. Here, we re-analyze Leavitt's first Period-Luminosity relation using observations of the same set of stars but with modern data and methods of Cepheid analysis. Using only data from…
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