{"paper":{"title":"The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Aaron Brown, Adam Burgasser, Aidan Gibbs, Andrew Howard, Ashley D. Baker, Ben Sappey, Bjorn Benneke, Bunei Sato, Chao Liu, Charles Beichman, Chikako Yasui, Christopher Johnson, Colette Salyk, Courtney Dressing, David Anderson, David Lafreniere, Dimitri Mawet, Eliza Kempton, Eric Wang, Etienne Artigau, Evan Kress, Evertt Schlawin, Gabriela Canalizo, Gajendra Pandey, Garreth Ruane, Gautam Vasisht, Geoffrey A. Blake, Greg Doppmann, Greg Herczeg, Guo Chen, Heather Knutson, Hiroshi Terada, Huihao Zhang, Hui Zhang, Jason Fucik, Jason Wang, Jean-Baptiste Ruffio, Jerome Maire, Jim Thorne, Ji Wang, Kenneth Magnone, Larry Lingvay, Lynne Hillenbrand, Marc Kassis, Max Millar-Blanchaer, Michael P. Fitzgerald, Michael Porter, Min Fang, Mitsuko Roberts, Motohide Tamura, Nemanja Jovanovic, Norio Narita, Paul Robertson, Peter Plavchan, Quinn M. Konopacky, Rene Doyon, Richard Dekany, Rishi Pahuja, Rob Bertz, Rose Gibson, Sam Halverson, Shogo Nishiyama, Sonia Karkar, S.P. Rajaguru, Stanimir Metchev, Stephanie Leifer, Stephen Kane, Sujan Sengupta, Takayuki Kotani, Thirupathi Sivarani, Thomas Beatty, Thomas Greene, Tiffany Kataria, Tuan Do, Warren Skidmore","submitted_at":"2023-09-20T03:59:52Z","abstract_excerpt":"HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R=100,000 between 0.98 - 2.5 um, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close orbits, direct high-contrast detection and spectroscopy of spatially separated substellar companions, and exoplanet dynamical mass and orbit measurements using precision radial velocity monitoring calibrated with a suite of state-of-the-art absolute and relative wavelength references. MODHIS is the counterpart to HISPEC for the Thirty Meter Telesco"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.11050","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2309.11050/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}