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SUMMARY:Invited talk: Infrared high-resolution spectroscopy of exoplanets:
  state-of-the art and prospects for the 2020s
DTSTART;VALUE=DATE-TIME:20220908T070000Z
DTEND;VALUE=DATE-TIME:20220908T074500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115915Z
UID:indico-contribution-148@meetings.aip.de
DESCRIPTION:Speakers: Matteo Brogi (University of Warwick)\nMeasuring the 
 chemical and thermal properties of planetary atmospheres is the main goal 
 of current exoplanet science. It allows us to understand their true nature
 \, origin\, and eventually the ability to support life. Ground-based\, hig
 h-resolution spectroscopy (HRS\, R>25\,000) has emerged as one of the lead
 ing methods to detect atomic and molecular species in the atmospheres of e
 xoplanets. At infrared wavelengths\, it allows us to resolve molecular ban
 ds into the individual spectral lines and extract their signal through cro
 ss correlation with model templates. As an added bonus\, HRS can measure p
 lanet rotation\, winds and orbital motion directly.\nHRS has produced a ra
 pidly growing inventory of detected species. Furthermore\, recent developm
 ents of the technique have unlocked the ability to measure absolute abunda
 nces and temperatures\, at a level comparable to expected JWST observation
 s but using different and complementary spectral information. This ability
  sets the stage for a strong synergy between space and ground observations
  of hot and warm gaseous planets during the current decade.\n\nhttps://mee
 tings.aip.de/event/16/contributions/148/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/16/contributions/148/
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