SHIMM as an atmospheric profiler on the Nickel telescope

Ollie Jackson; Maaike A. M. van Kooten; Saavidra Perera; Rebecca Jensen-Clem; Phil Hinz

doi:10.1117/12.2677510

5 October 2023 SHIMM as an atmospheric profiler on the Nickel telescope

Ollie Jackson, Maaike A. M. van Kooten, Saavidra Perera, Rebecca Jensen-Clem, Phil Hinz

Proceedings Volume 12680, Techniques and Instrumentation for Detection of Exoplanets XI; 126801V (2023) https://doi.org/10.1117/12.2677510
Event: SPIE Optical Engineering + Applications, 2023, San Diego, California, United States

Conference Poster

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), C²_n 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.

(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.

Citation Download Citation

Ollie Jackson, Maaike A. M. van Kooten, Saavidra Perera, Rebecca Jensen-Clem, and Phil Hinz "SHIMM as an atmospheric profiler on the Nickel telescope", Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126801V (5 October 2023); https://doi.org/10.1117/12.2677510

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