Chronos: A NIR spectroscopic survey to target the most important phases of galaxy evolution across cosmic time
I. Ferreras, M. Cropper, R. Sharples, J. Bland-Hawthorn, G. Bruzual,, S. Charlot, C.J. Conselice, S. Driver, J. Dunlop, A. M. Hopkins, S. Kaviraj,, T. Kitching, F. La Barbera, O. Lahav, A. Pasquali, S. Serjeant, J. Silk, R., Windhorst

TL;DR
Chronos is a proposed space-based NIR spectroscopic survey targeting key epochs in galaxy evolution, aiming to produce a million high-quality spectra to study galaxy formation and evolution across cosmic time.
Contribution
It introduces a dedicated, ultra-deep space-based NIR spectroscopic survey to explore galaxy evolution during cosmic dawn and noon, surpassing ground-based limitations.
Findings
Targeting z>6 and 1<z<3 epochs with NIR spectroscopy.
Producing about 1 million high-quality galaxy spectra.
Providing a comprehensive legacy database for galaxy evolution studies.
Abstract
(Abridged summary) Responding to ESA's Voyage 2050 call to define the long-term plan for the future space missions that will address the astrophysics science questions during the 2035-2050 cycle, we propose a dedicated, ultra-deep spectroscopic survey in the near infrared (NIR), that will target a mass-limited sample of galaxies during two of the most fundamental epochs of cosmic evolution: the formation of the first galaxies (at z>6; cosmic dawn), and at the peak of galaxy formation activity (between redshift z=1 and 3; cosmic noon). By way of NIR observations, it is possible to study the Lyman-alpha region in the former, and the optical rest-frame in the latter, allowing us to extract fundamental observables such as gas and stellar kinematics, chemical abundances, and ages, providing a unique legacy database covering these two crucial stages of cosmic evolution. A dedicated,…
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