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SUMMARY:A systematic analysis of exoplanet transmission spectra with JWST-
 MIRI - Martin Binet
DTSTART:20260311T131500Z
DTEND:20260311T134000Z
UID:TALK245590@talks.cam.ac.uk
CONTACT:Xander Byrne
DESCRIPTION:The launch of JWST has enabled atmospheric characterisation of
  sub-Neptunes more precise than ever. Specifically\, its MIRI instrument a
 llows to look for extra absorbers that are hard to find in the near-infrar
 ed. Recently this has been showed on temperate sub-Neptunes K2-18 b and TO
 I-732 c\, with potential signs of complex molecules\, although the signifi
 cance of these results has been contested in subsequent works. According t
 o these\, the findings could be due to instrument systematics\, or even me
 re random noise. In this context\, we aim to disentangle these possibiliti
 es by looking at multiple MIRI transit observations\, and check whether co
 mplex molecules are also found in other planets like hot gas giants.
LOCATION:Hoyle Lecture theatre + Zoom 
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