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.
E., Tacchella, S., Johnson, B
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Neo, a cGAN, super-resolves HSC images to HST-like quality and improves galaxy morphological parameter accuracy by factors of 2-10.
Super-Eddington accretion boosts predicted LISA detections of high-redshift black hole binaries to ~64 per year while dropping ET detections to ~4 per year, compared to ~32 and ~64 under Eddington-limited growth.
citing papers explorer
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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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Photometric Super-Resolution for Improving Galaxy Morphological Measurements using Conditional Generative Adversarial Networks
Neo, a cGAN, super-resolves HSC images to HST-like quality and improves galaxy morphological parameter accuracy by factors of 2-10.
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Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA
Super-Eddington accretion boosts predicted LISA detections of high-redshift black hole binaries to ~64 per year while dropping ET detections to ~4 per year, compared to ~32 and ~64 under Eddington-limited growth.