activity
20192026
most citedUsing the Gerchberg-Saxton algorithm to reconstruct non-modulated pyramid wavefront sensor measurements

13 citations · 15 across the 19 of their papers we have counts for

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Showing 2025Show all

5 papers · 1 filter

astro-ph.IM2025

On-sky demonstration of second-stage wavefront control with a photonic lantern

Aditya R. Sengupta, Jordan Diaz, Matthew DeMartino +14

Ground-based direct imaging of exoplanets at high contrast requires precise correction of atmospheric turbulence using adaptive optics (AO). The planet-to-star contrast ratio at sm…

astro-ph.IM2025

The Santa Cruz Extreme AO Lab (SEAL) 2.0: A reflective, multi-wavelength rebuild

Rebecca Jensen-Clem, Vincent Chambouleyron, Prince Javier +20

The Santa cruz Extreme Adaptive optics Lab (SEAL) is a visible/near-infrared wavelength testbed designed to support technology development for high contrast imaging on large, segme…

astro-ph.IM2025

Exploring the Capabilities of Astrophotonics for the Precise Alignment of Segmented Telescopes

Maria Cuevas, Aditya R. Sengupta, Vincent Chambouleyron +9

The next generation of large telescopes for direct imaging of exoplanets will require segmented primary mirrors. Over both long and short timescales, these telescopes experience se…

astro-ph.IM2025

Experimental validation of photonic lantern imaging and wavefront sensing performance

Aditya R. Sengupta, Vincent Chambouleyron, Jordan Diaz +15

Photonic lanterns (PLs) are fiber-based waveguides that are capable of focal-plane wavefront sensing while simultaneously directing light to downstream science instruments. The opt…

astro-ph.IM2025

Developments on LLNL's high contrast testbed and Lick/ShaneAO

Benjamin L. Gerard, Dominic F. Sanchez, Aditya R. Sengupta +15

LLNL has recently setup a High Contrast Testbed (HCT) for AO and exoplanet imaging technology development. We present the various HCT technologies currently under development, incl…