The paper is a science case for a UV integral field spectrograph on the Habitable Worlds Observatory, arguing it is the only planned capability able to resolve Lyman continuum escape from star-forming galaxies at cluster scales.
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How Do Ionizing Photons Escape from Star-Forming Galaxies?
The paper is a science case for a UV integral field spectrograph on the Habitable Worlds Observatory, arguing it is the only planned capability able to resolve Lyman continuum escape from star-forming galaxies at cluster scales.