The NASA High-Resolution Speckle Interferometric Imaging Program: Validation and Characterization of Exoplanets and Their Stellar Hosts
Steve B. Howell, Nicholas J. Scott, Rachel A. Matson, Mark E. Everett,, Elise Furlan, Crystal L. Gnilka, David R. Ciardi, and Kathryn V. Lester

TL;DR
NASA's speckle interferometry program uses high-resolution optical imaging to validate and characterize exoplanets and their stellar environments, supporting multiple space missions and providing crucial data for accurate exoplanet analysis.
Contribution
This paper details NASA's speckle interferometry program, its implementation on major telescopes, and its role in exoplanet validation and characterization since 2008.
Findings
Identification of nearby stellar companions affecting exoplanet measurements
Support for TESS and other exoplanet discovery projects
Major scientific discoveries in exoplanet research
Abstract
Starting in 2008, NASA has provided the exoplanet community an observational program aimed at obtaining the highest resolution imaging available as part of its mission to validate and characterize exoplanets, as well as their stellar environments, in search of life in the universe. Our current program uses speckle interferometry in the optical (320-1000 nm) with new instruments on the 3.5-m WIYN and both 8-m Gemini telescopes. Starting with Kepler and K2 follow-up, we now support TESS and other space- and ground-based exoplanet related discovery and characterization projects. The importance of high-resolution imaging for exoplanet research comes via identification of nearby stellar companions that can dilute the transit signal and confound derived exoplanet and stellar parameters. Our observations therefore provide crucial information allowing accurate planet and stellar properties to…
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