Abstract
We present first on-sky performance results of KalAO, the natural guide star adaptive optics imager on the 1.2m Swiss telescope in La Silla, Chile. It is designed to reach at least 30% Strehl in order to detect stellar companions as close as the 150mas in visible-light, at diffraction limit. KalAO was built to search for binarity in planet hosting stars by following-up planet candidates primarily from the TESS satellite survey. The optical design is optimised for the 450-900 nm wavelength range and is fitted with SDSS griz filters. Wavefront control works down to I-magnitude 10 stars in order to probe the same parameter space as radial velocity instruments such as HARPS and NIRPS. The system first closed the loop on sky in November 2023 and reached diffraction limit imaging in February 2024. It can carry out AO corrected observation of up to 500 targets in one night, with a Strehl ratio of ≈ 30%.
Original language | English (US) |
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Title of host publication | Adaptive Optics Systems IX |
Editors | Kathryn J. Jackson, Dirk Schmidt, Elise Vernet |
Publisher | SPIE |
ISBN (Electronic) | 9781510675179 |
DOIs | |
State | Published - 2024 |
Event | Adaptive Optics Systems IX 2024 - Yokohama, Japan Duration: Jun 16 2024 → Jun 22 2024 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 13097 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Conference
Conference | Adaptive Optics Systems IX 2024 |
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Country/Territory | Japan |
City | Yokohama |
Period | 6/16/24 → 6/22/24 |
Keywords
- Adaptive optics
- astronomy
- exoplanets
- optics
- wave-front sensing
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering