Cross-method analysis of co-rotation radii dataset

本数据集名为‘Cross-method analysis of co-rotation radii dataset’，由斯特恩伯格天文研究所与罗蒙诺索夫莫斯科国立大学合作创建。数据集包含1711个共转半径测量，覆盖547个旋涡星系，采用12种不同的测量方法。这些数据对于理解星系中共转半径的位置及其对星系动力学和化学演化的影响至关重要。数据集已公开在GitHub上，供未来研究使用，旨在解决星系中共转半径测量的不一致性问题，并探索星系中旋涡结构的性质。

This dataset, titled 'Cross-method analysis of co-rotation radii dataset', was co-developed by the Sternberg Astronomical Institute and Lomonosov Moscow State University. It encompasses 1,711 co-rotation radius measurements across 547 spiral galaxies, employing 12 different measurement methods. These data are crucial for comprehending the locations of co-rotation radii in galaxies and their impacts on galactic dynamics and chemical evolution. The dataset has been publicly made available on GitHub to facilitate future research, with the aims of addressing inconsistencies in co-rotation radius measurements within galaxies and investigating the properties of galactic spiral structures.