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most citedARES I: WASP-76 b, A Tale of Two HST Spectra

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astro-ph2000

Jupiter's hydrocarbons observed with ISO-SWS: vertical profiles of C2H6 and C2H2, detection of CH3C2H

T. Fouchet, E. Lellouch, B. Bezard +3

We have analysed the ISO-SWS spectrum of Jupiter in the 12-16 micron range, where several hydrocarbons exhibit rovibrational bands. Using temperature information from the methane a…