{"id":26782,"date":"2020-11-12T11:28:13","date_gmt":"2020-11-12T10:28:13","guid":{"rendered":"https:\/\/cab.inta-csic.es\/proyectos\/exoplanets-a\/"},"modified":"2022-08-08T12:12:49","modified_gmt":"2022-08-08T10:12:49","slug":"exoplanets-a","status":"publish","type":"proyectos","link":"https:\/\/cab.inta-csic.es\/en\/proyectos\/exoplanets-a\/","title":{"rendered":"EXOPLANETS-A"},"content":{"rendered":"\n

Project website<\/strong>: https:\/\/www.explore-exoplanets.eu\/<\/a><\/p>\n\n

General information<\/strong>: https:\/\/exoplanet-atmosphere.eu\/<\/a><\/p>\n\n

Principal investigator:<\/strong> David Barrado Navascu\u00e9s<\/p>\n\n

<\/div>\n\n

The Exoplanet Atmosphere New Emission Transmission Spectra Analysis (Exoplanets-A) collaboration is led by the CEA, a leading centre in France. CAB’s contribution focuses on the characterisation of the central star and data visualisation tools. Funded by the European Union under the H2020-COMPET-2017-RIA- 776403 programme, its main objective is to provide European researchers with a series of techniques that allow them to study the properties and evolution of exoatmospheres in greater depth.<\/p>\n\n

<\/div>\n\n
\"Planet
Planet crossing the disc of its star. Using the technique of planetary transits, the properties of atmospheres can be studied.<\/figcaption><\/figure><\/div>\n\n
<\/div>\n\n

Publications<\/strong>: https:\/\/www.explore-exoplanets.eu\/resource\/project-publications\/<\/a><\/p>\n\n

Planetary property settings<\/strong>: http:\/\/svo2.cab.inta-csic.es\/theory\/exovosa\/index.php<\/a><\/p>\n\n

Database<\/strong>: http:\/\/svo2.cab.inta-csic.es\/vocats\/v2\/exostars\/<\/a><\/p>\n\n

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