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astro-ph.IM2026
A scalable Bayesian framework for galaxy emission line detection and redshift estimation
Alexander Kuhn, Bonnabelle Zabelle, Sara Algeri +2
Estimating galaxy redshifts is crucial for constraining key physical quantities like those in the equation of state of dark energy. Modern telescopes such as the James Webb Space T…
astro-ph.IM2025
On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions
Xiangyu Zhang, Erik Floden, Hongru Zhao +4
It is demonstrated that estimators of the angular power spectrum commonly used for the stochastic gravitational-wave background (SGWB) lack a closed-form analytical expression for…