HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on H 0
astro-ph.CO, astro-ph.IM
Submitted: 2026-08-26
Updated: 2026-08-26
Comments: 17 pages, 12 figures, 10 tables
Journal ref: A&A 710, A258 (2026)
DOI: 10.1051/0004-6361/202555795
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- LSST Science Book, Version 2.0
- The Lazuli Space Observatory: Architecture & Capabilities
- Carnegie Supernova Project-I and -II: Measurements of $H_0$ using Cepheid, TRGB, and SBF Distance Calibration to Type Ia Supernovae
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation