L-band nulling interferometry at the VLTI with Asgard/NOTT: status and plans
Denis Defrère (Katholieke Universiteit Leuven)
Romain Laugier (Katholieke Universiteit Leuven)
Marc-Antoine Martinod (Katholieke Universiteit Leuven)
Germain Garreau (Katholieke Universiteit Leuven)
Kwinten Missiaen (Katholieke Universiteit Leuven)
Muhammad Salman (Katholieke Universiteit Leuven)
Gert Raskin (Katholieke Universiteit Leuven)
Colin Dandumont (Université de Liège)
J.J.D. Loicq (TU Delft - Spaceborne Instrumentation)
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Abstract
NOTT (formerly Hi-5) is the L’-band (3.5-4.0μm) nulling interferometer of Asgard, an instrument suite in preparation for the VLTI visitor focus. The primary scientific objectives of NOTT include characterizing (i) young planetary systems near the snow line, a critical region for giant planet formation, and (ii) nearby mainsequence stars close to the habitable zone, with a focus on detecting exozodiacal dust that could obscure Earthlike planets. In 2023-2024, the final warm optics have been procured and assembled in a new laboratory at KU Leuven. First fringes and null measurements were obtained using a Gallium Lanthanum Sulfide (GLS) photonic chip that was also tested at cryogenic temperatures. In this paper, we present an overall update of the NOTT project with a particular focus on the cold mechanical design, the first results in the laboratory with the final NOTT warm optics, and the ongoing Asgard integration activities. We also report on other ongoing activities such as the characterization of the photonic chip (GLS, LiNbO3, SiO), the development of the exoplanet science case, the design of the dispersion control module, and the progress with the self-calibration data reduction software.