BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Instituto de Astrofísica de Andalucía - ECPv6.15.20//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Instituto de Astrofísica de Andalucía
X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Paris
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20240331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20241027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20250330T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20251026T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20260329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20261025T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250121T090000
DTEND;TZID=Europe/Paris:20251030T170000
DTSTAMP:20260418T093637
CREATED:20241219T121029Z
LAST-MODIFIED:20250912T080532Z
UID:22550-1737450000-1761843600@www.iaa.csic.es
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
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/12/academicspanish.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250715T123000
DTEND;TZID=Europe/Paris:20250715T133000
DTSTAMP:20260418T093637
CREATED:20250707T114712Z
LAST-MODIFIED:20250707T114745Z
UID:26020-1752582600-1752586200@www.iaa.csic.es
SUMMARY:A UV-to-IR view of a nearby high-z analog with JWST and HST to interpret the first galaxies
DESCRIPTION:In the current JWST era\, detailed observations of the first generation of galaxies have started to revolutionize our knowledge of the early Universe\, with outstanding but also puzzling discoveries. In particular\, high-z systems in the epoch of reionization (z>6) are generally found to be low-mass\, compact and metal-poor\, and show prominent emission lines\, indicating extreme radiation fields. However\, their properties are not trivial to be determined\, some seem to show intriguing chemical inhomogeneities and an unprecedented number of them may host massive accreting black holes (i.e.\, Active Galactic Nucleus\, AGN\, activity) already in the first billion years. Nearby blue compact dwarf galaxies such as SBS 0335-052 E share similar properties\, and thus represent the perfect local laboratories for the multi-wavelength detailed studies required to understand the properties and mechanisms driving such intriguing scenarios. In this talk\, I will show new MIRI/MRS data of SBS 0335-052 E\, mapping MIR lines (e.g.\, [NeII]\, [SIV]\, [NeIII]\, [OIV]\, [NeV])\, in combination with UV spectroscopy and imaging. These data map the ionized gas at different level of ionization and dust attenuation at sub-kpc scales in this system for the first time. Thus\, they allow us to investigate the main ionization sources of the gas (massive stars\, shocks or AGN) in this high-z analog\, revealing the presence of an extended very high ionization emission possibly due to an accreting intermediate massive black hole. Overall\, this study provides us with an extremely powerful toolkit\, pivotal for understanding the gas conditions and feedback from different ionization sources in the earliest galaxies that reionized the universe. \nFecha: 15/07/2025 – 12:30Dr. Matilde MingozziSpace Telescope Science Institute\, Baltimore\, USA \n 
URL:https://www.iaa.csic.es/evento/a-uv-to-ir-view-of-a-nearby-high-z-analog-with-jwst-and-hst-to-interpret-the-first-galaxies/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
END:VCALENDAR