Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
Abstract
The ongoing Euclid mission aims to measure spectroscopic redshifts for approximately two million galaxies using the H $α$ line emission detected in near-infrared slitless spectroscopic data from the Euclid Deep Fields (EDFs). These measurements will reach a flux limit of $5\times 10^{-17}\,{\rm erg}\,{\rm cm}^{-2}\,{\rm s}^{-1}$ in the redshift range $0.4
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Cosmology and Gravitation Theories
Astronomy and Astrophysical Research
Publication details
- Journal / source
- arXiv (Cornell University)
- Publication date
- 15 January 2026
- Document type
- Preprint