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Paper: Center-Surround Application to JWST NIRISS Aperture Masking Interferometry Observations of Io
Volume: 538, ADASS XXXII
Page: 85
Authors: Deepashri Thatte; Anand Sivaramakrishnan; Kevin Volk; Imke de Pater; Thierry Fouchet; Albert Conrad; John Stansberry; Joel Sánchez-Bermúdez; Bryan Holler; Mike Wong; Ned Molter; Rachel Cooper
DOI: 10.26624/ZQCZ5337
Abstract: We present center-surround application to James Webb Space Telescope (JWST), Near Infrared Imager and Slitless Spectrograph (NIRISS) observations of Io, Jupiter’s innermost moon. This project is part of the JWST Early Release Science pro- gram ERS1373 (Co-PI’s Imke de Pater, Thierry Fouchet) on the Jovian system. Io is the most geologically active body in our solar system; however, the locations of tidal heating in the interior and temperature of Io’s magma leading to the volcanic eruptions are not well constrained (Keszthelyi et al. 2016). NIRISS’s Aperture Masking Interferometry (AMI) mode that utilizes a 7-hole non-redundant mask (NRM) in its pupil plane provides high-resolution imaging with moderate contrast and better astrometric accuracy over a wide field of view than conventional imaging. We present interferometric observations of Io from ERS1373 using NRM and filter F430M that is well matched to the emission from Io’s 500 K to ~1500 K lava flows. Convolution of Io images with the center-surround kernel emphasizes fine structure on Io’s disk. This convolved image is used as a ’prior’ to reconstruct images from Io’s interferometric data, thus helping to provide new measurements of the global distribution of vulcanism on Io.
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