Amortized SBI with spatio-temporal embeddings infers seven CWB parameters from 10-frame Hα time series with well-calibrated posteriors on synthetic data.
10.1051/0004-6361/202243531
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The authors produce a new all-sky Galactic emission model with synchrotron amplitude at 4.76 GHz roughly twice the Planck 2015 value, derived via Commander fitting to recent radio and microwave surveys.
Interstellar objects may contribute enough baryonic mass to reduce the local dark matter halo density to 0.24 GeV/cm³.
citing papers explorer
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Amortized Simulation-Based Inference of Colliding-Wind Binaries from Short, Noisy Image Time Series
Amortized SBI with spatio-temporal embeddings infers seven CWB parameters from 10-frame Hα time series with well-calibrated posteriors on synthetic data.
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All-sky modeling of Galactic emission at radio and microwave frequencies
The authors produce a new all-sky Galactic emission model with synchrotron amplitude at 4.76 GHz roughly twice the Planck 2015 value, derived via Commander fitting to recent radio and microwave surveys.
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Contribution of interstellar objects to local dark matter density
Interstellar objects may contribute enough baryonic mass to reduce the local dark matter halo density to 0.24 GeV/cm³.