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Phase curve measurements can be used to characterize an exoplanet\u2019s longitude-dependent atmospheric composition and energy circulation patterns. EXCITE carries a 0.5\u00a0m primary mirror and a moderate resolution diffraction-limited spectrograph with spectral coverage from 0.8 to 3.5\u00a0\u03bcm. EXCITE is designed to fly from a long-duration balloon. EXCITE will observe through the peak of a target\u2019s spectral energy distribution and through spectral signatures of hydrogen and carbon-containing molecules. In this paper, we present the science goals of EXCITE, detail the as-built instrument, and discuss its performance during a 2024 engineering flight from Fort Sumner, New Mexico.<\/jats:p>","DOI":"10.1063\/5.0326026","type":"journal-article","created":{"date-parts":[[2026,7,20]],"date-time":"2026-07-20T12:54:19Z","timestamp":1784552059000},"update-policy":"https:\/\/doi.org\/10.1063\/aip-crossmark-policy-page","source":"Crossref","is-referenced-by-count":0,"title":["The EXoplanet Climate Infrared TElescope (EXCITE): A balloon-borne mission to measure spectroscopic phase curves of transiting hot Jupiters"],"prefix":"10.1063","volume":"97","author":[{"ORCID":"https:\/\/orcid.org\/0009-0001-1186-3018","authenticated-orcid":false,"given":"T. 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