High-resolution Infrared Spectrograph for Exoplanet Characterization with the Keck and Thirty Meter Telescopes
by Dimitri Mawet, Michael Fitzgerald, Quinn Konopacky, Charles Beichman, Nemanja Jovanovic, Richard Dekany, David Hover, Eric Chisholm, David Ciardi, Étienne Artigau, Ravinder Banyal, Thomas Beatty, Björn Benneke, Geoffrey A. Blake, Adam Burgasser, Gabriela Canalizo, Guo Chen, Tuan Do, Greg Doppmann, René Doyon, Courtney Dressing, Min Fang, Thomas Greene, Lynne Hillenbrand, Andrew Howard, Stephen Kane, Tiffany Kataria, Eliza Kempton, Heather Knutson, Takayuki Kotani, David Lafrenière, Chao Liu, Shogo Nishiyama, Gajendra Pandey, Peter Plavchan, Lisa Prato, S. P. Rajaguru, Paul Robertson, Colette Salyk, Bun’ei Sato, Everett Schlawin, Sujan Sengupta, Thirupathi Sivarani, Warren Skidmore, Motohide Tamura, Hiroshi Terada, Gautam Vasisht, Ji Wang, and Hui Zhang
Published onSep 30, 2019
High-resolution Infrared Spectrograph for Exoplanet Characterization with the Keck and Thirty Meter Telescopes
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Abstract
HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffraction-limited spectrograph for the W.M. Keck Observatory, and a pathfinder for the MODHIS facility project (Multi-Object Diffraction-limited High-resolution Infrared Spectrograph) on the Thirty Meter Telescope.
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