Multiwavelength analysis of NGC 628 using ordinal pattern measures finds a ~200 pc characteristic scale separating star-formation-driven structures from larger dynamical morphology, with C-H trajectories converging to an isotropic Gaussian random field attractor.
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A Random Forest classifier on Chandra, Gaia, and CatWISE data identifies 1060 new quasar candidates behind the Galactic plane, with two spectroscopically confirmed at z~1.1-1.3.
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Morphological complexity of NGC 628 - a multiwavelength multiscale analysis using the ordinal pattern framework
Multiwavelength analysis of NGC 628 using ordinal pattern measures finds a ~200 pc characteristic scale separating star-formation-driven structures from larger dynamical morphology, with C-H trajectories converging to an isotropic Gaussian random field attractor.
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Finding Quasars behind the Galactic Plane. IV. Candidate Selection from Chandra with Random Forest
A Random Forest classifier on Chandra, Gaia, and CatWISE data identifies 1060 new quasar candidates behind the Galactic plane, with two spectroscopically confirmed at z~1.1-1.3.