The ArmazoNes High Dispersion Echelle Spectrograph, or ANDES, is a second-generation instrument designed for use at the Extremely Large Telescope (ELT). As a fiber-fed echelle spectrograph, it consists of three spectral arms covering a wavelength range from 0.4 up to 1.8 μm, with the potential to extend coverage from 0.35 to 2.4 μm. This versatile instrument delivers an impressive spectral resolution of approximately 100,000, enabling highly sensitive observations of astronomical objects and phenomena, including exoplanets, fundamental scientific inquiries, and various cutting-edge research applications in astronomy. This article will describe the opto-mechanical design of the three cameras inside the YJH spectrograph. The mechanical design is based on an improved strategy used in instruments like CPAPIR, WIRCAM, SPIROU and NIRPS. The optical design is highly efficient and straightforward, employing the same four lenses for each band (Y, J, and H). The expected performance for the H-band will also be presented.
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