collaborators

5 papers

astro-ph.HE2026

Weak emission line quasar SDSS J101353.45+492758.1 I. Continuum fitting

Laetitia Gibaud, Marek Nikołajuk, Piotr Życki +3

We present a broadband study of the WLQ SDSS J101353.45+492758.1, which displays a nearly featureless UV-optical spectrum with only a weak Mg II line alongside an exceptionally low…

astro-ph.HE2026

Population synthesis predictions of the Galactic compact binary gravitational wave foreground detectable by LISA

Jake McMillan, Adam Ingram, Cordelia Dashwood Brown +4

We use population synthesis modelling to predict the gravitational wave (GW) signal that the Laser Interferometer Space Antenna (LISA) will detect from the Galactic population of c…

astro-ph.IM2025

Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Mapping formation pathways of nuclear star clusters across galaxies

Francesca Pinna, Isabel Pérez, Anna Ferré-Mateu +21

Nuclear star clusters (NSCs) are dense, compact stellar systems only a few parsecs across, located at galaxy centers. Their small sizes make them difficult to resolve spatially. NS…

astro-ph.CO2025

The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision

H0DN Collaboration, Stefano Casertano, Gagandeep Anand +35

The direct, empirical determination of the local value of the Hubble constant (H0) has markedly advanced thanks to improved instrumentation, measurement techniques, and distance es…

astro-ph.SR2025

Characterizing the variability of a sample of massive stars in eclipsing binaries

C. I. Eze, G. Handler, F. Kahraman Aliçavuş +2

Massive stars exhibit a perplexing mismatch between their inferred masses from different observational techniques, posing a significant challenge to our understanding of stellar ev…