Search results for "Exoplanet atmospheric composition"

showing 2 items of 2 documents

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

2020

We analyse the transmission and emission spectra of the ultra-hot Jupiter WASP-76b, observed with the G141 grism of the Hubble Space Telescope's Wide Field Camera 3 (WFC3). We reduce and fit the raw data for each observation using the open-source software Iraclis before performing a fully Bayesian retrieval using the publicly available analysis suite TauRex 3. Previous studies of the WFC3 transmission spectra of WASP-76 b found hints of titanium oxide (TiO) and vanadium oxide (VO) or non-grey clouds. Accounting for a fainter stellar companion to WASP-76, we reanalyse this data and show that removing the effects of this background star changes the slope of the spectrum, resulting in these vi…

Brightness010504 meteorology & atmospheric sciencesExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope; Astrophysics - Earth and Planetary AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & AstrophysicsExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope01 natural sciencesSpectral lineAtmosphereJupiterHAT-P-7B0103 physical sciencesHubble Space TelescopeAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMOLECULAR LINE LISTS010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHOTPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Science & TechnologyAstronomy and AstrophysicsATMOSPHEREGIANT EXOPLANETGrismRESOLUTIONTransmission (telecommunications)Exoplanet atmospheric composition13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Physical SciencesINFERENCEAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Wide Field Camera 3STARSExoplanet atmospheresAstrophysics - Earth and Planetary Astrophysics
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Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX

2020

We present the first detection of atomic emission lines from the atmosphere of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq $\sim$ 4, 000 K). We combined thousands of spectrally resolved lines observed during one night with the HARPS-N spectrograph (R $\sim$ 115, 000), mounted at the Telescopio Nazionale Galileo. We introduce a novel statistical approach to extract the planetary parameters from the binary mask cross-correlation analysis. We also adapt the concept of contribution function to the context of high spectral resolution observations, to identify the location in the planetary atmosphere where the detected emission originates. The average planetary li…

astro-ph.SR010504 meteorology & atmospheric sciencesContinuum (design consultancy)FOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesExoplanet atmospheres; Exoplanet atmospheric composition; High resolution spectroscopyAtmosphereHigh resolution spectroscopy0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumSpectral resolution010303 astronomy & astrophysicsSpectrographInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Settore FIS/05Astronomy and AstrophysicsExoplanetAstrophysics - Solar and Stellar AstrophysicsExoplanet atmospheric composition13. Climate actionSpace and Planetary Scienceastro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresastro-ph.IM
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