arXiv · 2607.22388
ANDES, the high-resolution spectrograph for the ELT: design and performance analysis of the YJH spectrograph
Abstract
The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is a powerful second-generation high-resolution spectroscopic instrument for the Extremely Large Telescope (ELT). The UBV, RIZ, and YJH modules comprise fibre-fed spectrographs of the ANDES baseline design and will offer continuous wavelength coverage of 0.35-1.8 $\mu$m, with the addition of a K-band channel providing coverage up to 2.4 $\mu$m. Coupled with a spectral resolution of $\sim$100,000, ANDES must deliver the required wavelength calibration stability of 1 m/s over 24 hours, with a goal of 0.02 m/s across 10 years. These requirements establish the framework for the infrared module of ANDES, the YJH Spectrograph, leading to what will likely be the largest cryogenic, ultra-stable, high-resolution spectrograph ever built, and will offer the unique ability to observe in both seeing- and diffraction-limited modes interchangeably. We present the current design and performance analysis of the ANDES YJH Spectrograph, outlining the engineering challenges encountered alongside the corresponding strategies adopted to navigate them. In particular, we detail the technology development of the primary dispersing element, an echelle grating mosaic that will span over a metre in length.
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Vinooja Thurairethinam, David Lee, James Stevenson, Étienne Artigau, Frédérique Baron, Ciarán Breen, Bella Boyd, Denis Brousseau, David Buscher, Neil J. Cook, René Doyon, Martin Fisher, Bradley Frank, Vincent Geers, Rory Gillespie, Oscar Gonzalez, Éamonn J. Harvey, Wei Li, Roberto Maiolino, Lison Malo, Thomas Marquart, David Montgomery, Alan O'Brien, Ernesto Oliva, Jonathan St-Antoine, Jay Stephan, Simon Thibault, Philippe Vallée, Chris Waring, Sandi Wilson, Junyi Zhou, Paolo Di Marcantonio. 2026-07-24. ANDES, the high-resolution spectrograph for the ELT: design and performance analysis of the YJH spectrograph. https://arxiv.org/abs/2607.22388
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