Figure 1 from Rotation Curve of the Milky Way from Classical Cepheids

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Rotation Curve of the Milky Way from Classical Cepheids

Authors: Przemek Mróz, Andrzej Udalski, Dorota M. Skowron, Jan Skowron, Igor Soszyński, Paweł Pietrukowicz, Michał K. Szymański, Radosław Poleski, Szymon Kozłowski, and Krzysztof Ulaczyk

2019 The Astrophysical Journal Letters 870 L10.

Provider: AAS Journals

Caption: Figure 1.

The black line shows the cumulative distribution of residuals from the best-fit model (model 2 with the prior on R₀). This distribution is compared to a standard Gaussian distribution, and we quote the p-value of the Kolmogorov–Smirnov (KS) test. The gray line shows the cumulative distribution function of the normal distribution.

Other Images in This Article

Copyright and Terms & Conditions