Poster + Paper
13 December 2020 Enhanced seeing mode: a technique for improving wide-field angular resolution in the near-infrared using adaptive optics
Author Affiliations +
Conference Poster
Abstract
The Adaptive Optics (AO) system at the Large Binocular Telescope (LBT) in conjunction with the f/30 camera on the LBT Utility Camera in the Infrared instruments (LUCI) can achieve diffraction limited image quality over a 30" × 30" field of view (FOV). The AO system also includes the ability to deliver only 11 modes of correction (including tip and tilt) to remove residual aberrations and jitter. When combined with the f/3.75 camera on either LUCI, this Enhanced Seeing Mode (ESM) can achieve an uniform angular resolution of 0".22 over a 4' × 4' FOV in the best natural seeing conditions. Further, unlike full AO, ESM can be used for binocular longslit and multi-object high-resolution spectroscopy (R~10,000). It has been further demonstrated that even in poor seeing conditions (θ << 1′′.5) the image quality delivered to the LUCI focal stations is improved by 2-3× from 1-2.5 microns. It is proposed that ESM should become a standard observational mode for near-Infrared LBT observations.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Barry Rothberg, Julian C. Christou, Douglas L. Miller, Dave Thompson, Gregory E. Taylor, Christian Veillet, and R. T. Gatto "Enhanced seeing mode: a technique for improving wide-field angular resolution in the near-infrared using adaptive optics", Proc. SPIE 11448, Adaptive Optics Systems VII, 114485I (13 December 2020); https://doi.org/10.1117/12.2563359
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KEYWORDS
Adaptive optics

Electronic support measures

Spatial resolution

Cameras

Imaging spectroscopy

Stars

Image quality

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