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	<title>LESIA - Observatoire de Paris</title>
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	<description>De la conception des instruments d'astronomie &#224; l'exploitation des r&#233;sultats, les th&#233;matiques scientifiques d&#233;velopp&#233;es au LESIA couvrent de nombreux domaines de l'astrophysique. Les activit&#233;s sont organis&#233;es autour des projets (sol, espace ou mod&#233;lisation) dont de nombreuses r&#233;alisations instrumentales font la r&#233;putation du laboratoire.
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		<title>Nouvelles possibilit&#233;s d'analyses atmosph&#233;riques avec Monte Carlo</title>
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		<dc:date>2024-12-03T15:31:23Z</dc:date>
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&lt;a href="https://youtube.lesia.obspm.fr/-Saison-2024-2025-.html" rel="directory"&gt;Saison 2024-2025&lt;/a&gt;


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		<title>Gone with the stellar wind : characterizing atmospheric escape in exoplanets</title>
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		<dc:date>2024-11-26T13:27:55Z</dc:date>
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&lt;p&gt;Some exoplanets orbit so close to their star that their atmosphere can be partially &#8220;blown away&#8221; by intense stellar radiation. This phenomenon of atmospheric escape plays a key role in planetary evolution, shaping the structure of the upper atmosphere. Photo-evaporation may even lead to the formation of super-Earth planets through the complete evaporation of mini-Neptunes' atmospheres. In recent years, the study of the metastable helium triplet in the infrared (1083.3 nm) has made it possible (...)&lt;/p&gt;


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&lt;a href="https://youtube.lesia.obspm.fr/-Saison-2024-2025-.html" rel="directory"&gt;Saison 2024-2025&lt;/a&gt;


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 <content:encoded>&lt;div class='rss_texte'&gt;&lt;p&gt;Some exoplanets orbit so close to their star that their atmosphere can be partially &#8220;blown away&#8221; by intense stellar radiation. This phenomenon of atmospheric escape plays a key role in planetary evolution, shaping the structure of the upper atmosphere. Photo-evaporation may even lead to the formation of super-Earth planets through the complete evaporation of mini-Neptunes' atmospheres. In recent years, the study of the metastable helium triplet in the infrared (1083.3 nm) has made it possible to probe atmospheric escape processes from the ground using high-resolution spectrographs, enabling unprecedented measurements. We analyzed the transits of 15 exoplanets observed with SPIRou (CFHT, R=70,000), searching for helium signatures to characterize these atmospheric losses. In this seminar, I will present the physical processes at play in these extreme environments and the analytical tools and models we developed to interpret our observations.&lt;/p&gt;
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		<title>The Hubble Tension : Recent Results from HST and JWST by the SH0ES Team</title>
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&lt;p&gt;The 5-sigma tension between the local measurement and the early universe prediction of the Hubble constant (H0) may be the most exciting development in modern cosmology, pointing towards the possibility of new physics beyond lambda-CDM. In my talk, I will present the latest H0 measurement by the SH0ES team, based on the Cepheid and Type Ia supernova distance ladder, and will discuss recent improvements from Gaia, HST and (...)&lt;/p&gt;


-
&lt;a href="https://youtube.lesia.obspm.fr/-Saison-2024-2025-.html" rel="directory"&gt;Saison 2024-2025&lt;/a&gt;


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 <content:encoded>&lt;div class='rss_texte'&gt;&lt;p&gt;The 5-sigma tension between the local measurement and the early universe prediction of the Hubble constant (H0) may be the most exciting development in modern cosmology, pointing towards the possibility of new physics beyond lambda-CDM. In my talk, I will present the latest H0 measurement by the SH0ES team, based on the Cepheid and Type Ia supernova distance ladder, and will discuss recent improvements from Gaia, HST and JWST.&lt;/p&gt;&lt;/div&gt;
		
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