AI Insight
Researchers have developed windsoCC, a new data processing pipeline that uses wavefront sensor telemetry to reconstruct and remove the wind-driven halo, a persistent noise artifact in adaptive optics imaging caused by atmospheric turbulence. The method cross-correlates wavefront sensor data to measure wind velocities in different atmospheric layers and uses this information to model and subtract the halo from individual images. Demonstration with MagAO-X coronagraphic images of the disk around star HR 4796A shows dramatic improvement in recovering astrophysical objects while preserving extended structure that would be lost with traditional spatial filtering methods.
Why it matters
This technique addresses a fundamental limitation in adaptive optics astronomy by enabling better detection and characterization of faint objects near bright stars, such as exoplanets and circumstellar disks. The method makes use of existing wavefront sensor data that is already being recorded, requiring no hardware modifications to current instruments.
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⚠️ Preprint – Noch nicht peer-reviewed
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Abstract: The wind-driven halo (WDH) is a persistent, low spatial frequency noise artifact that arises due to the servo-lag error inherent to all adaptive optics (AO) instruments. Spatial filtering may be employed to overcome this artifact, however, filtering out the WDH while simultaneously preserving signal from an extended astrophysical object of interest is exceptionally challenging. Additionally, since the WDH changes in intensity and position angle through an observation, data-driven algorithms (e.g., KLIP) that are commonly used to subtract the starlight need to be overly-aggressive to remove both the static and dynamic noise components. Since wavefront sensors (WFSs) continuously track the closed-loop residual wavefront error, WFS telemetry presents the ideal resource for combating this type of noise artifact through postprocessing. Using archival WFS telemetry from MagAO-X, which is the “extreme” AO instrument for the 6.5-meter Magellan-Clay telescope, we demonstrate a novel workflow for WDH reconstruction and removal in individual coronagraphic science images. MagAO-X is equipped with a pyramid WFS capable of recording wavefront telemetry at a high-cadence which is saved during data acquisition. Given this, we detail how our WFS data processing pipeline, windsoCC, cross-correlates the recorded closed-loop wavefront to measure the wind vectors of several turbulent layers of the atmosphere above Las Campanas Observatory. We then make use of the wind parameters learned through windsoCC to reconstruct the WDH footprint by leveraging a parametric model. Notably, we demonstrate a dramatic improvement in object recovery using on-sky MagAO-X images of the disk around HR~4796A at visible wavelengths.
Source: WindsoCC: reconstructing the wind-driven halo in MagAO-X images using wavefront sensor telemetry