Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning

Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine LearningDOI: info:10.3847/1538-4357/ab426fv. 88433
Green, Sheridan B., Ntampaka, Michelle, Nagai, Daisuke, Lovisari, Lorenzo, Dolag, Klaus, Eckert, Dominique, and ZuHone, John A. 2019. "Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning." The Astrophysical Journal, 884 33. https://doi.org/10.3847/1538-4357/ab426f.
ID: 154618
Type: article
Keywords: SAO