activity
20242026
collaborators

6 papers

astro-ph.IM2026

NIRC2-Pol: First Light of Near-Infrared Polarimetry on Keck II

Briley L. Lewis, Manxuan Zhang, Maxwell A. Millar-Blanchaer +21

NIRC2, the Near Infrared Camera 2 on the Keck II telescope, was recently upgraded with a new suite of polarimetric observing modes. The new polarimetry modes (referred to as NIRC2-…

astro-ph.IM2026

Enabling Quantitative Polarimetry for Keck/NIRC2: Preliminary Mueller Matrix Model Calibration

Manxuan Zhang, Briley L. Lewis, Maxwell A. Millar-Blanchaer +27

The Keck/NIRC2 infrared imager was upgraded in 2025 with dual-beam polarimetric observing modes spanning approximately 1.1--4.1 microns (JHKL' bands). We present a preliminary JHK…

astro-ph.IM2026

Fundamental Noise Limits of Infrared Detectors in the Presence of Readout Glow

Michael Bottom, Gustav Pettersson, Pavaman Bilgi +5

Read noise in infrared sensor arrays remains a major obstacle for ground- and space-based astronomy. It has long been recognized that the upcoming extremely large telescopes cannot…

astro-ph.IM2025

Performance Simulations for Kola: Achieving High-Resolution, Visible-Light AO Correction Over a 1 Arcminute Field

Brianna Peck, Jessica R. Lu, Lianqi Wang +8

We present performance simulations for a proposed visible-light, multi-conjugate adaptive optics system for the 10-meter W. M. Keck I telescope that aims to deliver near diffractio…

astro-ph.IM2024

Glow reduction of ultra-low noise LmAPDs: towards photon counting infrared arrays

Guillaume Huber, Michael Bottom, Charles-Antoine Claveau +5

Spectroscopy and direct-imaging of ultra-faint targets such as Earth-like exoplanets and high redshift galaxies are among the primary goals of upcoming large scale astronomy projec…

astro-ph.IM2024

Progress towards a megapixel linear-mode avalanche photodiode array for ultra-low background shortwave infrared astronomy

Charles-Antoine Claveau, Michael Bottom, Shane Jacobson +12

Spectroscopy of Earth-like exoplanets and ultra-faint galaxies are priority science cases for the coming decades. Here, broadband source flux rates are measured in photons per squa…