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BEGIN:VEVENT
UID:20260517T181733-04-1905VEuR4F@https://astronomia.uc.cl/2jucext1/institu
 toastrofisica/
DTSTAMP:20260517T221733Z
DESCRIPTION:I will present results on the latest planet to be studied by th
 e Low Resolution Ground-Based Exoplanet Atmosphere Survey using Transmissi
 on Spectroscopy (LRG-BEASTS\, “large beasts”)\, the hot Saturn-mass planet
  WASP-39b. WASP-39b has one of the most cloud- and haze-free atmospheres o
 f hot\, giant planets\, which show a remarkable diversity across the popul
 ation\, from clear to cloudy atmospheres. LRG-BEASTS will sample this dive
 rsity with observations of 17 exoplanets covering a broad range of tempera
 tures and masses. LRG-BEASTS is pioneering the use of 4-metre class telesc
 opes for low resolution transmission spectroscopy and has demonstrated tha
 t such telescopes can provide precision comparable to VLT and HST. https:/
 /astronomia.uc.cl/2jucext1/institutoastrofisica/en/instituto-2/seminars/ev
 ent/337-the-lrg-beasts-transmission-spectroscopy-survey-wasp-39b-dr-james-
 kirk-harvard-smithsonian-center-for-astrophysics
DTSTART:20190311T171500Z
DTEND:20190311T174500Z
LOCATION:Seminar Room (Instituto de Astrofísica\, Pontificia Universidad Ca
 tólica\, Vicuña Mackenna 4860\, Santiago\, Chile)
SUMMARY:The LRG-BEASTS transmission spectroscopy survey: WASP-39b (Dr. Jame
 s Kirk\; Harvard & Smithsonian Center for Astrophysics)
URL:https://astronomia.uc.cl/2jucext1/institutoastrofisica/en/instituto-2/s
 eminars/event/337-the-lrg-beasts-transmission-spectroscopy-survey-wasp-39b
 -dr-james-kirk-harvard-smithsonian-center-for-astrophysics
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