The case for an Astrometric Mission Extension of Euclid. Extending Gaia by 6 magnitudes with Euclid covering one-third of the sky
Luigi "Rolly'' BEDIN (Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Padova)

TL;DR
Extending Euclid's mission by six years to cover one-third of the sky would significantly enhance astrometric data, enabling proper motion measurements of faint stars and advancing our understanding of the universe.
Contribution
This paper advocates for a six-year extension of Euclid's mission, demonstrating its potential to improve astrometric measurements and scientific outcomes beyond the original plan.
Findings
Proper motions for stars as faint as V~27 could be derived.
A six-year baseline between two epochs enhances astrometric precision.
Using only the VIS channel maximizes astrometric capability and depth.
Abstract
The nominal duration of Euclid's main mission is six years, but current best estimates indicate that the observatory has sufficient propellant to operate for up to ~14 years in total. In this work, we advocate dedicating six of these ~8 additional years to repeating the main survey, covering approximately one-third of the sky. This repetition would not only improve the sampling, signal-to-noise, quality, and depth of the survey, but -- most importantly -- would provide a six-year time baseline between two epochs if executed in the same sequence. The availability of multiple epochs would enable the derivation of proper motions for stars as faint as V~27, i.e., more than five magnitudes fainter than those measured by the Gaia mission. Although it may seem early to propose such a mission extension, in this work we quantitatively illustrate its immense scientific potential. We therefore…
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