Studying the atmospheres of exoplanets is a critical and rapid way to learn more about worlds outside our solar system. Highresolution spectroscopy (R≥100,000) is necessary to distinguish overlapping absorption features from different molecules, especially for ground-based observations. For molecular oxygen in the atmospheres of Earth-analogs, it is recommended to operate at R=300,000–400,000. A Virtually Imaged Phased Array (VIPA) offers structural simplicity and compact dimensions, rendering it highly suitable as the primary dispersing element in such ultra-high resolution narrow-band spectrometers. In this work, we aim for a high-throughput spectrograph: VIPA Instrument for Oxygen Loaded Atmospheres (VIOLA), a VIPA spectrograph using a Volume Phase Holographic Grating as a cross-disperser. Commercial, highperformance optical components will facilitate swift and efficient implementation. We present a preliminary optical design, resulting image quality and prospects for VIOLA in advancing high-resolution spectroscopy for the study of exoplanet atmospheres.
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