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SUMMARY:Academic Spanish Course for Foreigners (2025)
DESCRIPTION:The Academic Spanish course for foreigners is designed to facilitate effective communication in academic and profesional contexts. Through a practical and personalized focus\, the participants will develop essential linguistic abilities to discuss scientific articles\, participate in conferences\, give presentations\, and collaborate in international projects. The program includes technical vocabulary\, beginner and advanced grammar\, and simulations of real-life situations. Moreover\, it will promote the cultural immersion to strengthen the comprehension of the Hispanic world\, and their impact on interdisciplinary investigation and collaboration. \nThis course will be taught throughout in the following blocks: \nJanuary 21st – February 27thApril 22nd – May 29thSeptember 23rd – October 30thThe course is taught by Prof. Nazira Ruíz
URL:https://www.iaa.csic.es/evento/academic-spanish-course-for-foreigners-2025/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
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SUMMARY:Study of the very high energy emission from star-forming regions and young massive star clusters
DESCRIPTION:Cosmic rays (CRs) are a fundamental component of the Cosmos. They can penetrate and ionise the dense gas core of molecular clouds\, affecting the dynamics of the cloud itself and triggering chemical reactions that lead to the creation of complex molecular compounds. In star-forming complexes\, CRs can be accelerated by the wind of newly born massive stars\, often found in young massive stellar clusters (YMSC). The amount of freshly injected CRs can be probed by the observations of high-energy and very-high-energy gamma-rays. In this regard\, the future Cherenkov Telescope Array Observatory (CTAO) will play a crucial role. CTAO will be composed of around 100 telescopes deployed on two sites\, one in Northern and one in the Southern Hemisphere. The arrays will cover a wide energy range from tens of GeV to hundreds of TeV employing telescopes of three sizes: the Large\, Medium and Small Sized Telescopes with 23 m\, 14 m and 4.5 m mirror diameters\, respectively. Each telescope is optimized for the detection of photons below 1 TeV (LST)\, between 1-10 TeV (MST) and above 10 TeV (SST). The first LST prototype\, LST-1\, is currently ending its commissioning phase and is starting to collect scientific data. During the present observational cycle\, two observational proposals on YMSC were submitted for the very first time. These observations are challenging due to the extension of the expected gamma-ray emission from YMSC and to the limited Field of View (FoV) of the Cherenkov telescopes (around 2.3° radius for LST-1). In this context is of paramount importance to optimise the reconstruction analysis chain (currently under development) for extended sources and to rank the best targets for the next observational campaigns both of LST-1 and of the upcoming 3 LSTs currently under construction at the CTAO-Northern site. \n​ \nFecha: 23/01/2025 – 12:30Conferenciante: Dr. Gaia VernaFiliación: Università degli Studi di Siena\, Italy
URL:https://www.iaa.csic.es/evento/study-of-the-very-high-energy-emission-from-star-forming-regions-and-young-massive-star-clusters/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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