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DTSTART;VALUE=DATE:20251215
DTEND;VALUE=DATE:20251220
DTSTAMP:20260613T080207
CREATED:20251212T223545Z
LAST-MODIFIED:20251212T223545Z
UID:10000564-1765756800-1766188799@spacecalendar.com
SUMMARY:High-Resolution Spectroscopy for Exoplanet Atmospheres Workshop
DESCRIPTION:Over the next few decades\, the exoplanet community is poised to advance closer to answering a fundamental question about the universe and humanity’s place in it: Are we alone? High-resolution spectroscopy of exoplanets with the Extremely Large Telescopes (> 25 m) offers a unique opportunity to answer this question.  The high spectral resolutions and large apertures enable high signal-to-noise measurements of spectrally resolved lines of key atmospheric gases.  Current observational programs with 3 – 10 m class telescopes (e.g.\, TNG\,  ESO 3.6 m\, LDT\, CFHT\, Gemini N/S\, VLT\, Keck) and high resolution spectrographs (R>~15\,000\, e.g.\,  HARPS\, GIANO\, SPIRou\, ESPRESSO\, MAROON-X\, GHOST\, IGRINS\, CRIRES+) have and are continuing to reveal unique insights into the composition\, chemistry\, and climates of large gas giant planets.    \nHowever\, in order to maximize the science return from current instrumentation and the upcoming ELT’s\, there is a pressing need to train the next generation of scientists in this challenging but powerful observational method.  In particular\,  the pool of experts in this area within the US exoplanet community is rather small. Hence\, there is a pressing need to train US-based junior scientists in ground-based high spectral resolution observational and analysis techniques so that we maximize the science return from current and upcoming platforms.  \nThe goal of this week-long workshop is to provide sufficient background via lectures and hands-on activities such that attendees will be able to: \n\n\nOpen and read in pipeline processed data from a variety of US (e.g.\, IGRINS\, MAROON-X\, GHOST) and European-led (e.g\, ESPRESSO\, CRIRES+) instruments. \n\n\nApply common telluric removal methods like PCA\, SYSREM\, and forward modeling. \n\n\nPerform model template-data cross-correlation analyses to detect atmospheric gases in both the transmission and emission geometries. \n\n\nApply publicly available atmospheric retrieval tools combined with various CCF-to-log-likelihood mappings to obtain atmospheric parameter constraints. \n\n\nPlan and execute observations with a variety of instruments. \n\n\nThe workshop will be structured like the Sagan Summer Workshops\, with a mix of pedagogical lectures and hands-on activities\, as well as an opportunity for attendees to present their own work via daily poster sessions. 
URL:https://spacecalendar.com/event/high-resolution-spectroscopy-for-exoplanet-atmospheres-workshop/
LOCATION:Tempe AZ\, USA
CATEGORIES:Meeting / Conference / Symposium
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BEGIN:VEVENT
DTSTART;VALUE=DATE:20251208
DTEND;VALUE=DATE:20251213
DTSTAMP:20260613T080207
CREATED:20250620T233024Z
LAST-MODIFIED:20251017T205256Z
UID:10000060-1765152000-1765583999@spacecalendar.com
SUMMARY:33rd Texas Symposium on Relativistic Astrophysics
DESCRIPTION:22 plenary speakers are confirmed\, and 200+ contributed abstracts are accepted. At Arizona State University. \nThe symposium will cover all major topics on high-energy and particle astrophysics\, cosmology\, and relativity. It will include morning plenary sessions and afternoon parallel sessions\, which will function as mini-symposia in each sub-field. The plenary sessions will consist of ~45-minute review talks. The afternoon sessions will feature oral talks (about 15-30 minutes) and poster contributions.
URL:https://spacecalendar.com/event/33rd-texas-symposium-on-relativistic-astrophysics/
LOCATION:Tempe AZ\, USA
CATEGORIES:Meeting / Conference / Symposium
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