| DOI | Resolve DOI: https://doi.org/10.1117/12.2677510 |
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| Author | Search for: Jackson, Ollie; Search for: van Kooten, Maaike1; Search for: Perera, Saavidra; Search for: Jensen-Clem, Rebecca; Search for: Hinz, Phil |
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| Editor | Search for: Ruane, Garreth J. |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Conference | Techniques and Instrumentation for Detection of Exoplanets XI, August 20-25, 2023, San Diego, United States |
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| Subject | astronomical instrumentation; atmospheric profiling; Fried parameter; site testing; high contrast imaging |
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| Abstract | Optimal atmospheric conditions are beneficial for detecting exoplanets via high contrast imaging (HCI), as speckles from adaptive optics’ (AO’s) residuals can make it difficult to identify exoplanets. While AO systems greatly improve our image quality, having access to real-time estimates of atmospheric conditions could also help astronomers use their telescope time more efficiently in the search for exoplanets as well as aid in the data reduction process. The Shack-Hartmann Imaging Motion Monitor (SHIMM) is an atmospheric profiler that utilizes a Shack-Hartmann wavefront sensor to create spot images of a single star in order to reconstruct important atmospheric parameters such as the Fried parameter (r0), C²ₙ profile and coherence time. Due to its simplicity, the SHIMM can be directly used on a telescope to get in situ measurements while observing. We present our implementation of the Nickel-SHIMM design for the one meter Nickel Telescope at Lick Observatory. We utilize an HCIPy simulation of turbulence propagating across a telescope aperture to verify the SHIMM data reduction pipeline as we begin on-sky testing. We also used on-sky data from the AO system on the Shane Telescope to further validate our analysis, finding that both our simulation and data reduction pipeline are consistent with previously determined results for the Fried parameter at the Lick Observatory. Finally, we present first light results from commissioning of the Nickel-SHIMM. |
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| Publication date | 2023-10-05 |
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| Publisher | SPIE |
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| In | |
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| Series | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 33a6ed5d-fceb-4377-ae5d-27a8057642bd |
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| Record created | 2024-06-26 |
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| Record modified | 2024-06-26 |
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