Paper 13103-129
Observing strategies for using Keck-NIRC2 to conduct high-contrast imaging in the mid-infrared
18 June 2024 • 17:30 - 19:00 Japan Standard Time | Room G5, North - 1F
Abstract
The Keck-NIRC2 electronics underwent an upgrade in the fall of 2023 that dramatically increased the readout efficiency in the mid infrared (3-5 µm). We present an updated analysis of how this upgrade improved the sensitivity of Keck-NIRC2 in the modes most commonly used by the exoplanet direct imaging community. We provide on-sky testing results of the throughput measurements of the vector vortex coronagraph and an evaluation of the thermal background dynamical timescale. Our goal in this proceeding is to provide Keck-NIRC2 users with knowledge and recommendations for how the recent NIRC2 upgrade affects the optimal observing strategies in the mid-infrared high-contrast imaging application.
Presenter
Univ. of California, Santa Cruz (United States)
Rachel Bowens-Rubin recently earned their PhD from the University of California Santa Cruz. They research exoplanet formation through multi-method observations and develop instrumentation relevant to the exoplanet direct imaging in the mid-infrared.