Imaging low-mass planets within the habitable zones of nearby stars with ground-based mid-infrared imaging
Kevin Wagner, Steve Ertel, Jordan Stone, Jarron Leisenring, D\'aniel, Apai, Markus Kasper, Olivier Absil, Laird Close, Denis Defr\`ere, Olivier, Guyon, and Jared Males

TL;DR
This paper reviews recent advances in ground-based mid-infrared imaging techniques for detecting low-mass, potentially habitable exoplanets around nearby stars, highlighting technological innovations and future prospects.
Contribution
It introduces new mid-IR imaging strategies and instrumentation, including lessons learned from the NEAR campaign and the design of the LESSONS survey, to improve exoplanet detection capabilities.
Findings
Successful implementation of a mid-IR optimized coronagraph and adaptive optics at VLT
Development of noise mitigation strategies through chopping techniques
Enhanced sensitivity in mid-IR imaging for exoplanet detection
Abstract
Giant exoplanets on 10-100 au orbits have been directly imaged around young stars. The peak of the thermal emission from these warm young planets is in the near-infrared (~1-5 microns), whereas mature, temperate exoplanets (i.e., those within their stars' habitable zones) radiate primarily in the mid-infrared (mid-IR: ~10 microns). If the background noise in the mid-IR can be mitigated, then exoplanets with low masses--including rocky exoplanets--can potentially be imaged in very deep exposures. Here, we review the recent results of the Breakthrough Watch/New Earths in the Alpha Centauri Region (NEAR) program on the Very Large Telescope (VLT) in Chile. NEAR pioneered a ground-based mid-IR observing approach designed to push the capabilities for exoplanet imaging with a specific focus on the closest stellar system, Alpha Centauri. NEAR combined several new optical technologies--including…
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