A Problem with the Clustering of Recent Measures of the Distance to the Large Magellanic Cloud
Bradley E. Schaefer

TL;DR
This paper highlights a problematic over-concentration of recent distance measurements to the Large Magellanic Cloud around a widely accepted value, suggesting potential biases or systematic issues in the field.
Contribution
It identifies and analyzes the abnormal clustering of recent LMC distance measurements, revealing possible biases or systematic errors affecting the field.
Findings
Recent measurements cluster too tightly around the HSTKP value
Statistical tests show the clustering deviates from expected distributions
Potential correlations and biases may influence published distance estimates
Abstract
The distance to the Large Magellanic Cloud (LMC) has long been of key importance for the distance ladder and the distances to all galaxies, and as such many groups have provided measurements of its distance modulus (\mu) with many methods and various means of calibrating each method. Before the year 2001, the many measures spanned a wide range (roughly 18.1 < \mu < 18.8) with the quoted error bars being substantially smaller than the spread, and hence the consensus conclusion being that many of the measures had their uncertainties being dominated by unrecognized systematic problems. In 2001, the Hubble Space Telescope Key Project (HSTKP) on the distance scale made an extensive analysis of earlier results and adopted the reasonable conclusion that the distance modulus is 18.50+-0.10 mag, and the community has generally accepted this widely popularized value. After 2002, 31 independent…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
