Design and development of the SOXS calibration unit
Hanindyo Kuncarayakti, Jani Achren, Sergio Campana, Riccardo Claudi,, Pietro Schipani, Matteo Aliverti, Andrea Baruffolo, Sagi Ben-Ami, Federico, Biondi, Giulio Capasso, Rosario Cosentino, Francesco D'Alessio, Paolo, D'Avanzo, Ofir Hershko, Marco Landoni, Matteo Munari

TL;DR
The paper details the design, development, and testing of the calibration unit for the SOXS spectrograph, which employs multiple calibration lamps and modes to ensure accurate wavelength calibration and flat-field correction for transient object observations.
Contribution
It introduces a comprehensive calibration unit design with innovative features like dual modes, homogeneous illumination, and safety interlocks, advancing spectrograph calibration technology.
Findings
Calibration unit successfully integrated with SOXS spectrograph
Homogeneous illumination variation less than 1%
Unit in the test and verification stage
Abstract
SOXS is a new spectrograph for the New Technology Telescope (NTT), optimized for transient and variable objects, covering a wide wavelength range from 350 to 2000 nm. SOXS is equipped with a calibration unit that will be used to remove the instrument signatures and to provide wavelength calibration to the data. The calibration unit will employ seven calibration lamps: a quartz-tungsten-halogen and a deuterium lamp for the flat-field correction, a ThAr lamp and four pencil-style rare-gas lamps for the wavelength calibration. The light from the calibration lamps is injected into the spectrograph mimicking the f/11 input beam of the NTT, by using an integrating sphere and a custom doublet. The oversized illumination patch covers the length of the spectrograph slit homogeneously, with variation. The optics also supports the second mode of the unit, the star-simulator mode that…
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