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Found 3 papers, 1 papers with code
Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
By listening to gravity in the low frequency band, between 0. 1 mHz and 1 Hz, the future space-based gravitational-wave observatory LISA will be able to detect tens of thousands of astrophysical sources from cosmic dawn to the present.
General Relativity and Quantum Cosmology Instrumentation and Methods for Astrophysics 83C35, 62-07 I.6; G.3
Benchmarking Quality-Dependent and Cost-Sensitive Score-Level Multimodal Biometric Fusion Algorithms
The cost-sensitive evaluation, on the other hand, investigates how well a fusion algorithm can perform given restricted computation and in the presence of software and hardware failures, resulting in errors such as failure-to-acquire and failure-to-match.
Short-Period Variables in TESS Full-Frame Image Light Curves Identified via Convolutional Neural Networks
The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ~85% of the sky throughout its two-year primary mission, resulting in millions of TESS 30-minute cadence light curves to analyze in the search for transiting exoplanets.
