Direct spectroscopy is a very promising approach to characterizing the atmospheres of nearby rocky exoplanets, but non-common path aberrations (NCPA), which are differential aberrations between the science optical path and the adaptive optics optical path, can leak through the coronagraph and create speckles that mimic...
S. Haffert, J. Liberman, J. Males et al.· Astronomy & Astrophysics· 0 citations
We report on the goals, design, and ongoing development of the Netherlands EXoplanet Testbed (NEXT), a high-contrast imaging testbed under construction in Leiden. NEXT is designed to develop and validate technologies and algorithms for extreme adaptive optics (XAO) and coronagraphy at the performance levels required by...
R. Landman, S. Haffert, L. Desdoigts et al.· Astronomical Telescopes + In...· 1 citation
Current high-contrast imaging instruments are limited by wavefront errors originating from non-common path aberrations (NCPAs) due, for example, to manufacturing errors in the optics and temperature drifts in the system. These create quasi-static speckles in the final science image that are difficult to distinguish fro...
E. Tonucci, S. Haffert, J. Males et al.· Astronomical Telescopes + In...· 1 citation
The Giant Magellan Adaptive Optics eXtreme (GMagAO-X) instrument has now been selected as an official part of the Giant Magellan Telescope’s (GMT) instrument suite. The instrument will be ready at first-light of the GMT in the mid 2030s. The instrument is now progressing towards its final design with a final design rev...
S. Haffert, J. Males, L. Close et al.· Astronomical Telescopes + In...· 3 citations
A lingering technical challenge for pyramid wavefront sensors (PyWFS) is their change in response between calibration and correction residuals, a quantity known as optical gain (OG). Given the prevalent use of PyWFSs in current and planned high contrast adaptive optics (AO), understanding and reliably measuring OG for...
E. McEwen, J. Males, O. Guyon et al.· Astronomical Telescopes + In...· 1 citation
Incoming starlight is refracted as it enters Earth’s atmosphere from the vacuum of space. The wavelength dependence of atmospheric refraction causes elongation of the broadband PSF of ground-based telescopes, especially in the visible spectrum. The result is degraded image quality alongside reduced coronagraph light-bl...
K. Twitchell, S. Haffert, J. Males et al.· Astronomical Telescopes + In...· 4 citations
By combining a physical optics model with a flexible machine learning model, this work can avoid introducing unphysical features in the resulting PSF estimate and explores the temporal coherence of structures in telemetry and the limitations of learning this relationship from data sampled on such different timescales.
Joseph D. Long, S. Haffert, J. Males et al.· Astronomical Telescopes + In...· 1 citation
One of the main limitations of ground-based extreme adaptive optics systems (XAO) is the balance between the temporal and photon noise error. The unmodulated Pyramid Wavefront Sensor (uPWFS) promises significant gains in sensitivity over its modulated counterpart, but its practical use is limited by its linearity range...
R. Landman, Liam Koning, S. Haffert et al.· Astronomical Telescopes + In...· 1 citation
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