output
20162026
most citedGravitational waves from a first order electroweak phase transition: a brief review

178 citations

181 papers

astro-ph.GA2026

The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models

David A. Simon

The line spread function (LSF) of a spectrograph encodes the inherent broadening of a single spectral line. It is typically reported as a single number, the resolving power $R = λ/…

astro-ph.GA2026

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe

Connor Sant Fournier, Stephen M. Wilkins, Joseph Caruana +5

UV absorption line indices trace chemical enrichment and star formation histories in high-redshift galaxies, yet their reliability as quantitative stellar metallicity, Z*, diagnost…

astro-ph.CO2026

TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars

Ryan Brady, Xiang-Yu Huang, Simon Birrer +7

We present the first uniform gravitational lens modeling analysis of eight doubly imaged quasars from multi-band observations with the Hubble Space Telescope. Previous time-delay c…

astro-ph.CO2026

On combining estimated and analytic covariance matrices

Alan Heavens, Lorne Whiteway, Elena Sellentin

The statistical analysis of cosmological data often assumes a Gaussian sampling distribution and relies on covariance matrices estimated from simulations. In this setting, the like…

astro-ph.SR2026

White dwarf + M dwarf Detached Binaries in Long Period Radio Transients: Observed Binary Parameters, Evolution, and Population Constraints

Antonio C. Rodriguez, Kareem El-Badry, Iris de Ruiter +4

Long period radio transients (LPTs) are the slowest radio-pulsing sources ever found, with the current population spanning periods of seven minutes to over six hours. Two of the th…

astro-ph.GA2026★ 1 cited

Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not

Massimiliano Parente, Desika Narayanan, Paul Torrey

We present the first implementation of an evolving dust grain size distribution (GSD) within a semi-analytic cosmological model (SAM) of galaxy evolution. This flexible model self-…