activity
20202026
most citedMeasuring Phase Errors in the Presence of Scintillation

23 citations · 36 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

10 papers · 1 filter

astro-ph.IM2026

Performance Comparison of the Nonlinear Curvature and Shack-Hartmann Wavefront Sensors in Strong Turbulence

Sam J. Potier, Arlene J. Aleman, Justin R. Crepp +1

Strong turbulence induces spatial variations in beam intensity that hinder the reconstruction process of many commonly deployed adaptive optics (AO) systems that use gradient-based…

astro-ph.IM2026

Laboratory characterization of iLocater

Marcelo Tala Pinto, Marshall C. Johnson, Julia Brady +18

iLocater is a diffraction-limited, fiber-fed spectrograph designed for the Large Binocular Telescope (LBT), which targets high-precision radial velocity measurements in the near-in…

astro-ph.IM2026

Commissioning and on-sky performance verification of iLocater

Marshall C. Johnson, Marcelo Tala Pinto, Jonathan Crass +59

iLocater is a high-resolution near-infrared extreme precision radial velocity (EPRV) spectrograph that was deployed to the Large Binocular Telescope (LBT) in June 2026. iLocater op…

astro-ph.IM2026

The Calibration System of the iLocater Spectrograph

Sai Vidyud Senthil Nathan, Jonathan Crass, Julia E. Brady +21

iLocater is a new near-infrared, extreme precision radial velocity (EPRV) instrument delivered to the Large Binocular Telescope in the summer of 2026. The instrument utilizes singl…

astro-ph.IM2024

Centroiding and Extraction of Tip/Tilt Information from Nonlinear Curvature Wavefront Sensor Measurements

Caleb A. Abbott, Justin R. Crepp, Stanimir O. Letchev +1

The nonlinear curvature wavefront sensor (nlCWFS) uses multiple (typically four) out-of-focus images to reconstruct the phase and amplitude of a propagating light beam. Because the…

astro-ph.IM2024★ 1 cited

Performance of the Nonlinear Curvature Wavefront Sensor as a Function of Scintillation Strength

Stanimir Letchev, Justin R. Crepp, Caleb G. Abbott +3

Local amplitude aberrations caused by scintillation can impact the reconstruction process of a wavefront sensor (WFS) by inducing a spatially non-uniform intensity at the pupil pla…

astro-ph.IM2023

Developing an Error Budget for the Nonlinear Curvature Wavefront Sensor

Sam Potier, Justin Crepp, Stanimir Letchev

Consistent operation of adaptive optics (AO) systems requires the use of a wavefront sensor (WFS) with high sensitivity and low noise. The nonlinear curvature WFS (nlCWFS) has been…

astro-ph.IM2023★ 6 cited

Assessing Phase Reconstruction Accuracy for Different Nonlinear Curvature Wavefront Sensor Configurations

Stanimir Letchev, Jonathan Crass, Justin R. Crepp

The nonlinear curvature wavefront sensor (nlCWFS) offers improved sensitivity for adaptive optics (AO) systems compared to existing wavefront sensors, such as the Shack-Hartmann. T…

astro-ph.IM2022★ 6 cited

Spatial frequency response and sensitivity of the nonlinear curvature wavefront sensor

Stanimir Letchev, Jonathan Crass, Justin R. Crepp +1

The nonlinear curvature wavefront sensor (nlCWFS) has been shown to be a promising alternative to existing wavefront sensor designs. Theoretical studies indicate that the inherent…

astro-ph.IM2020★ 23 cited

Measuring Phase Errors in the Presence of Scintillation

Justin R. Crepp, Stanimir O. Letchev, Sam J. Potier +2

Strong turbulence conditions create amplitude aberrations through the effects of near-field diffraction. When integrated over long optical path lengths, amplitude aberrations (seen…