Mugnai, L;
Al-Refaie, A;
Bocchieri, A;
Changeat, Q;
Pascale, E;
Tinetti, G;
(2021)
Alfnoor: Assessing the Information Content of Ariel's Low-resolution Spectra with Planetary Population Studies.
The Astronomical Journal
, 162
(6)
, Article 288. 10.3847/1538-3881/ac2e92.
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Abstract
The Ariel Space Telescope will provide a large and diverse sample of exoplanet spectra, performing spectroscopic observations of about 1000 exoplanets in the wavelength range 0.5–7.8 μm. In this paper, we investigate the information content of Ariel's Reconnaissance Survey low-resolution transmission spectra. Among the goals of the Ariel Reconnaissance Survey is also to identify planets without molecular features in their atmosphere. In this work, (1) we present a strategy that will allow us to select candidate planets to be reobserved in Ariel's higher-resolution tier, (2) we propose a metric to preliminary classify exoplanets by their atmospheric composition without performing an atmospheric retrieval, and (3) we introduce the possibility to find other methods to better exploit the data scientific content.
Type: | Article |
---|---|
Title: | Alfnoor: Assessing the Information Content of Ariel's Low-resolution Spectra with Planetary Population Studies |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.3847/1538-3881/ac2e92 |
Publisher version: | https://doi.org/10.3847/1538-3881/ac2e92 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | Science & Technology, Physical Sciences, Astronomy & Astrophysics, MOLECULAR LINE LISTS, ATMOSPHERE, EXOPLANET, RETRIEVAL, ABSORPTION, EMISSION, MODELS |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/10140344 |
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