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From the 1 of 8 linked papers with an AI index.

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8 papers

astro-ph.GA2026

J-ATLAS: Javalambre Andromeda and Triangulum Legacy Astrophysical Survey

Borja Anguiano, Andres del Pino

J-ATLAS is a proposed wide-field optical photospectroscopic survey of the Andromeda (M31) and Triangulum (M33) galaxies that will obtain low‑resolution spectral energy distribution…

astro-ph.GA2026

Reconstructing the orbits of Milky Way dwarf galaxies: An LMC perspective

Alberto Manuel Martínez-García, Andrés del Pino, Roeland P. van der Marel +14

The orbital histories of the dwarf satellites of the Milky Way (MW) are key to understanding their evolution and placing their present-day properties in a dynamical context. We pre…

astro-ph.IM2026

Hubble Astrometry for the Local Group and Beyond in the 2030s

S. Tony Sohn, Paul Bennet, Kevin Andrew McKinnon +23

Hubble's long, stable astrometric baseline creates a rare opportunity for discovery in the Local Group and beyond. Many nearby galaxies, streams, and star clusters already have arc…

astro-ph.IM2025

GALATEA: The 15-m Galactic Archaeology Spectroscopic Surveyor

Borja Anguiano, David Valls-Gabaud, Andrés del Pino +5

\textsc{GALATEA} (the \emph{Galactic Archaeology and Local-group Astrophysics Telescope for Extended Areas}) is a concept for a dedicated 15-m, wide-field, 10,000-fibre spectroscop…

astro-ph.IM2025

Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Galactic Archaeology from the Northern Sky

Borja Anguiano, David Valls-Gabaud, Guillaume F. Thomas +7

By the 2040s--50s, facilities such as \emph{Gaia}, WEAVE, 4MOST, Rubin, \emph{Euclid}, \emph{Roman}, and the ESO ELT will have transformed our global view of the Milky Way. Yet key…

astro-ph.IM2025

Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Resolved Stellar Populations Studies in M31 and its Satellites

C. Gallart, E. Fernández-Alvar, A. B. A. Queiroz +48

A 30 m class optical/near-IR telescope in the Northern Hemisphere, equipped for diffraction-limited imaging and high-resolution, multi-object spectroscopy of faint stars, would ena…