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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240312T080000
DTEND;TZID=Europe/Paris:20240315T190000
DTSTAMP:20260421T011807
CREATED:20240313T091624Z
LAST-MODIFIED:20240313T092151Z
UID:20539-1710230400-1710529200@www.iaa.csic.es
SUMMARY:ESA's Vigil PMI instrument kick-off consortium meeting
DESCRIPTION:Kickoff meeting del instrumento PMI (Photospheric Magnetic field Imager). PMI es uno de los tres instrumentos postfocales de la misión de meteorología espacial de la ESA\, Vigil. 
URL:https://www.iaa.csic.es/evento/esas-vigil-pmi-instrument-kick-off-consortium-meeting/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Congresos
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/03/vigil.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240307T123000
DTEND;TZID=Europe/Paris:20240307T133000
DTSTAMP:20260421T011807
CREATED:20240307T081945Z
LAST-MODIFIED:20250912T080248Z
UID:20504-1709814600-1709818200@www.iaa.csic.es
SUMMARY:SO Colloquium: Stars and their close-by planets: clues of magnetic interactions
DESCRIPTION:Stars interact with their close-in planets through the gravitational and magnetic fields and with their radiation. After a general introduction to those interactions\, I shall review some observational clues of magnetic star-planet interactions considering data obtained in the optical\, X-ray\, and radio domains. Based on a stellar force-free coronal field or the excitation of Alfven waves by an orbiting planet\, some analytical models will be introduced to explore the energetics of the interactions. Some numerical models will be discussed to show their potential and drawbacks in predicting the interactions. The information on stellar magnetic fields that can be derived from magnetic star-planet interactions will be briefly considered and some preliminary results will be presented in the framework of the analytical models. \nFecha: 07/03/2024 – 12:30Conferenciante: Dr. Antonino Francesco LanzaFiliación: INAF-Osservatorio Astrofisico di Catania\, Catania\, Italy \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-stars-and-their-close-by-planets-clues-of-magnetic-interactions/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240306T003000
DTEND;TZID=Europe/Paris:20240306T020000
DTSTAMP:20260421T011807
CREATED:20240305T085243Z
LAST-MODIFIED:20250123T225759Z
UID:20480-1709685000-1709690400@www.iaa.csic.es
SUMMARY:8M: Día Internacional de la Mujer 2024
DESCRIPTION:El Instituto de Astrofísica de Andalucía participa en la celebración del Día Internacional de la Mujer celebrando la mesa redonda «Vocaciones en áreas STEM: El caso de la Física». \nEl día 8 de marzo se conmemora el Día Internacional de las Mujeres\, que fue adoptado por la Asamblea General de la Organización de las Naciones Unidas el 16 de diciembre de 1977\, con el objetivo de eliminar toda forma de discriminación hacia las mujeres\, promover su empoderamiento y conseguir su plena participación en la sociedad. \nEn el marco del 8M\, el Instituto de Astrofísica de Andalucía participa este 2023 en la celebración del Día Internacional de la Mujer con la celebración de la mesa redonda «Vocaciones en áreas STEM: El caso de la Física»\, que tendrá lugar el día 6 de marzo en el Salón de Actos del IAA-CSIC a las 12:30h y se retransmitirá online. \n \nEl objetivo de esta mesa redonda es analizar el recorrido curricular\, desde secundaria\, pasando por la Universidad\, para acabar con la trayectoria investigadora y en ella participan: \n\nMaría José Cano Úbeda. Docente de Física y Química en el IES Pedro Soto de Rojas de Granada\nM. Carmen Carrión. Decana de la Facultad de Ciencias de la Universidad de Granada\nAscensión del Olmo Orozco. Científica Titular del Instituto de Astrofísica de Andalucía\n\nLa dirección de la mesa estará a cargo de la Comisión de Igualdad del IAA-CSIC \n 
URL:https://www.iaa.csic.es/evento/8m-dia-internacional-de-la-mujer-2024/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Workshops
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/03/poster_8m-1.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240305T123000
DTEND;TZID=Europe/Paris:20240305T133000
DTSTAMP:20260421T011807
CREATED:20240307T081624Z
LAST-MODIFIED:20250912T080253Z
UID:20498-1709641800-1709645400@www.iaa.csic.es
SUMMARY:SO Colloquium: A new digitized age of SETI – interferometric commensal observations and machine learning
DESCRIPTION:The search for technosignatures – remotely observable indicators of advanced extraterrestrial life – addresses one of the most profound questions in science: are we alone in the universe as intelligent life? The Breakthrough Listen program is leading the most concerted search for extraterrestrial intelligence (SETI) effort to-date through radio and optical surveys of nearby stars\, nearby galaxies and the Milky Way galactic plane\, thus representing the best chance the human race has ever had to detect a technosignature. Recently\, Breakthrough Listen has partnered with the SETI Institute to develop commensal SETI capabilities on some of the most sensitive radio inteferometers\, including the Very Large Array (VLA) and MeerKAT. Interferometric radio telescopes have the advantage of providing a larger field of view\, maximizing the SETI survey speed. The VLA search will be operating alongside latter portions of the third epoch of the VLA Sky Survey (VLASS)\, allowing us to monitor over 1 million nearby stars within the next few years. Moreover\, we are developing Machine Learning algorithms that will help reduce the number of false positives. A re-processing of the Green Bank archival SETI data revealed 8 signals-of-interest that were overlooked by previous analyses. In this talk\, we will present the latest updates on these projects and conclude with a refreshed outlook on SETI using next generation telescope facilities and machine learning algorithms. \nFecha: 05/03/2024 – 12:30Conferenciante: Dr. Cherry NgFiliación: Laboratoire de Physique et Chimie de l’Environnement et de l’Espace\, CNRS \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-a-new-digitized-age-of-seti-interferometric-commensal-observations-and-machine-learning/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20240304
DTEND;VALUE=DATE:20240306
DTSTAMP:20260421T011807
CREATED:20240215T200940Z
LAST-MODIFIED:20250912T081110Z
UID:20372-1709510400-1709683199@www.iaa.csic.es
SUMMARY:PySnacks 6: pyFIT3D/pyPipe3D: Resolved Properties of Stellar Populations and Ionized Gas with Galaxy IFS Data
DESCRIPTION:The present course focuses on explaining the functionality of the pyFIT3D routine package and the pyPipe3D pipeline\, and their practical use in deriving spatially resolved properties of stellar populations (using the population synthesis method) and ionized gas in galaxies observed through integral field spectroscopy. This applies to both large surveys (e.g.\, CALIFA\, MaNGA) and individual observations (WEAVE\, MUSE). The course is predominantly practical\, primarily aimed at young researchers and students with basic knowledge of the subject. A computer with Linux/Unix/Mac or similar operating system\, with Python3 installed\, is required\, and preferably\, the following package should be installed in advance. \nhttp://ifs.astroscu.unam.mx/pyPipe3D/ \nThis course is organized by Rubén Garcia Benito and it will be taught by Sebastián Sánchez (UNAM). \n 
URL:https://www.iaa.csic.es/evento/pysnacks-6-pyfit3d-pypipe3d-resolved-properties-of-stellar-populations-and-ionized-gas-with-galaxy-ifs-data/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/02/pysnacks.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240229T123000
DTEND;TZID=Europe/Paris:20240229T133000
DTSTAMP:20260421T011807
CREATED:20240222T092345Z
LAST-MODIFIED:20250912T080258Z
UID:20439-1709209800-1709213400@www.iaa.csic.es
SUMMARY:SO Colloquium: Eyes on the Invisible: Charting New Horizons with the Event Horizon Telescope
DESCRIPTION:The Event Horizon Telescope (EHT) collaboration has captured the first-ever image of a black hole’s event horizon in the galaxy M87\, and more recently\, in the supermassive black hole at the center of our Milky Way\, SgrA*. These images\, consistent with Kerr black holes as described by General Relativity\, provide the strongest evidence to date for the existence of supermassive black holes in galaxy nuclei. Notably\, the first polarization images of M87* at event horizon scales have revealed a dominant poloidal magnetic field\, confirming predictions from general relativistic magnetohydrodynamic simulations and highlighting magnetically arrested disks (MADs) as crucial in black hole accretion and relativistic jet formation processes. These achievements\, stemming from EHT’s 2017 inaugural observing campaign\, have set the stage for an array of new\, exhilarating findings from subsequent campaigns. These include finer details of the emission structure near black holes and pioneering real-time movies of black hole accretion and jet launching\, made possible by additional telescopes\, enhanced data rates\, and improved algorithms. Beyond these remarkable accomplishments\, the EHT’s journey is just beginning. The next-generation EHT (ngEHT) aims to significantly augment the current array with more stations\, multi-frequency simultaneous observations\, and extended time coverage. This expansion will dramatically enhance angular resolution\, dynamic range\, and temporal coverage\, solidifying the EHT as a paramount astronomical facility over the next decade\, and the only one capable of directly imaging black holes. \nFecha: 29/02/2024 – 12:30Conferenciante: Dr. Avery BroderickFiliación: Department of Physics & Astronomy at the University of Waterloo\, Canada \n 
URL:https://www.iaa.csic.es/evento/so-coloquium-demystifying-the-rings-meaning-and-paths-to-detection/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240227T123000
DTEND;TZID=Europe/Paris:20240227T133000
DTSTAMP:20260421T011807
CREATED:20240222T092316Z
LAST-MODIFIED:20250125T202542Z
UID:20435-1709037000-1709040600@www.iaa.csic.es
SUMMARY:Unraveling the Gamma-ray emission in radiogalaxies and their jets
DESCRIPTION:The Transient HIgh-Energy Sky and Early Universe Surveyor (THESEUS) is a mission concept developed by a large European collaboration under study by ESA since 2018 and currently one of the three candidate M7 mission for a launch in mid ’30s. THESEUS aims at fully exploiting Gamma-Ray Bursts for investigating the early Universe and as key phenomena for multi-messenger astrophysics. By providing an unprecedented combination of X-/gamma-ray monitors\, on-board IR telescope and spacecraft autonomous fast slewing capabilities\, THESEUS would be a wonderful machines for the detection\, multi-wavelength characterization and redshift measurement of any kind of GRBs and many classes of X-ray transients\, including high-redshift GRBs for cosmology (pop-III stars\, cosmic reionization\, SFR and metallicity evolution up to the «cosmic dawn») and electromagnetic counterparts to sources of gravitational waves\, especially short GRBs\, possible soft X-ray emission and KN emission from NS-NS / NS-BH mergers. THESEUS would thus provide an ideal synergy with the very large astronomical facilities of the future working in the e.m. (e.g.\, ELT\, CTA\, SKA\, Athena) and multi-messenger (e.g.\, Einstein Telescope\, Cosmic Explorer\, km3NET). \nFecha: 27/02/2024 – 12:30Conferenciante: Mireia Nievas RosilloFiliación: Instituto de Astrofísica de Canarias\, Spain \n 
URL:https://www.iaa.csic.es/evento/unraveling-the-gamma-ray-emission-in-radiogalaxies-and-their-jets/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240222T190000
DTEND;TZID=Europe/Paris:20240222T200000
DTSTAMP:20260421T011808
CREATED:20240219T104658Z
LAST-MODIFIED:20250125T010709Z
UID:20410-1708628400-1708632000@www.iaa.csic.es
SUMMARY:Ciencia abierta y la crisis de la reproducibilidad
DESCRIPTION:La ciencia es una fantástica y gigantesca empresa humana en la que se estima que están implicadas mas de nueve millones de personas y en la que actualmente se invierte en el mundo más de un billón y medio de euros anualmente. El método científico es el instrumento que ha caracterizado a la ciencia para alcanzar su objetivo de conocer y comprender el mundo natural que nos rodea. \nLa reproducibilidad es una propiedad fundamental de la actividad científica\, ya sea observacional o experimental\, pues sin ella los resultados obtenidos de los estudios científicos carecen de la validez requerida lo que lleva aparejado el descrédito de la ciencia ante la sociedad y el derroche de recursos invertidos en llevar a cabo tales investigaciones irreproducibles. \nLa falta de reproducibilidad en la ciencia no es un problema nuevo\, pero sí que últimamente ha tomado unas dimensiones como para admitir que existe la llamada crisis de la reproducibilidad; este es un problema que no se da por igual en todas las ramas de la ciencia\, pero en todas es importante. La causa principal es el no cumplimiento estricto del método científico\, motivada por razones de índole muy diversa. \nLa Ciencia Abierta es un nuevo paradigma que\, entre otros objetivos\, trata de superar los problemas mencionados mediante la mejora en la forma de producir\, financiar\, comunicar y evaluar la producción científica. \nFecha: 22/02/2024 – 19:00Conferenciante: Emilio Sánchez-CantalejoFiliación: Profesor jubilado de la Escuela de Salud Publica y ateneísta. \n 
URL:https://www.iaa.csic.es/evento/ciencia-abierta-y-la-crisis-de-la-reproducibilidad/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/02/lucas_lara_0.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20240219
DTEND;VALUE=DATE:20240224
DTSTAMP:20260421T011808
CREATED:20240118T103029Z
LAST-MODIFIED:20250912T081114Z
UID:20281-1708300800-1708732799@www.iaa.csic.es
SUMMARY:English for Academic Purposes
DESCRIPTION:Within the  Severo Ochoa Training Initiative of the IAA-CSIC we are offering the 2024 edition of «English for Academic Purposes»\, imparted by Ms. Marie Waltie of the University of Leipzig. The workshop will be in-person. Key aspects of the use of English for academic purposes will be highlighted and correct usage encouraged. Participants will comprehensively expand their competence in the academic use of English. The course will cover the following topics:  \n• Common Errors in Academic English• Writing up Results and Methods in English• Pronunciation Practice in English• Academic Discussions in English• Presenting your Academic Project in English \nFundamental knowledge of the English language as well as high motivation of the participants is a requirement because the course will be interactive. We can accommodate up to 30 participants. In case of over-subscription\, we will give preference to students and young postdocs and/or may lead selection interviews. If you are interested in participating\, please register before 31 January 2024 indicating whether you are interested in an INDIVIDUAL session of 20-25 min.
URL:https://www.iaa.csic.es/evento/english-for-academic-purposes/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/01/tips-improve-english.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240208T123000
DTEND;TZID=Europe/Paris:20240208T133000
DTSTAMP:20260421T011808
CREATED:20240215T200605Z
LAST-MODIFIED:20250125T202615Z
UID:20367-1707395400-1707399000@www.iaa.csic.es
SUMMARY:The Transient High-Energy Sky and Early Universe Surveyor (THESEUS)
DESCRIPTION:The Transient HIgh-Energy Sky and Early Universe Surveyor (THESEUS) is a mission concept developed by a large European collaboration under study by ESA since 2018 and currently one of the three candidate M7 mission for a launch in mid ’30s. THESEUS aims at fully exploiting Gamma-Ray Bursts for investigating the early Universe and as key phenomena for multi-messenger astrophysics. By providing an unprecedented combination of X-/gamma-ray monitors\, on-board IR telescope and spacecraft autonomous fast slewing capabilities\, THESEUS would be a wonderful machines for the detection\, multi-wavelength characterization and redshift measurement of any kind of GRBs and many classes of X-ray transients\, including high-redshift GRBs for cosmology (pop-III stars\, cosmic reionization\, SFR and metallicity evolution up to the «cosmic dawn») and electromagnetic counterparts to sources of gravitational waves\, especially short GRBs\, possible soft X-ray emission and KN emission from NS-NS / NS-BH mergers. THESEUS would thus provide an ideal synergy with the very large astronomical facilities of the future working in the e.m. (e.g.\, ELT\, CTA\, SKA\, Athena) and multi-messenger (e.g.\, Einstein Telescope\, Cosmic Explorer\, km3NET). \nFecha: 08/02/2024 – 12:30Conferenciante: Dr. Lorenzo AmatiFiliación: INAF – OAS Bologna\, Italy \n 
URL:https://www.iaa.csic.es/evento/the-transient-high-energy-sky-and-early-universe-surveyor-theseus/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240125T190000
DTEND;TZID=Europe/Paris:20240125T200000
DTSTAMP:20260421T011808
CREATED:20240124T195127Z
LAST-MODIFIED:20250125T010849Z
UID:20325-1706209200-1706212800@www.iaa.csic.es
SUMMARY:Planificación virtual e impresión 3D en cirugía Craneomaxilofacial
DESCRIPTION:Cada año en todo el mundo muchos pacientes requieren reconstrucción quirúrgica de deformidades craneales y faciales adquiridas y congénitas. La reconstrucción de estos defectos son siempre un desafío para el cirujano debido a una anatomía compleja donde asientan funciones vitales\, así como la apariencia facial. \nLa cirugía craneomaxilofacial\, en la última década\, ha experimentado un profundo cambio conceptual en la planificación y en la mesa de quirófano con la incorporación de tecnologías: software de PV e impresión 3D. Esto ha tenido un impacto particularmente significativo en precisión y en mejora de resultados respecto a modos de hacer convencionales. \n¡Bienvenidos a la cirugía 4.0! \nFecha: 25/01/2024 – 19:00Conferenciante: Adoración Martínez PlazaFiliación: Cirujana Oral y Maxilofacial / Co-directora de la Unidad de Malformaciones Craneofaciales y Fisura Labio Palatina / H. U. Virgen de las Nieves (Granada)
URL:https://www.iaa.csic.es/evento/planificacion-virtual-e-impresion-3d-en-cirugia-craneomaxilofacial/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/01/planificacion.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240125T123000
DTEND;TZID=Europe/Paris:20240125T133000
DTSTAMP:20260421T011808
CREATED:20240125T113159Z
LAST-MODIFIED:20250125T202651Z
UID:20332-1706185800-1706189400@www.iaa.csic.es
SUMMARY:Stellar population studies in the J-PAS survey
DESCRIPTION:The Javalambre Physics of the Accelerating Universe Astrophysical Survey (J-PAS) is a large scale multi-filter survey that has started to observe 8500 deg² of the northern sky with 54 narrow-band filters in the optical range (3500-9600Å). In our Galaxy Evolution group at IAA-CSIC\, we aimed at developing and testing methodologies in order to perform stellar populations studies using this kind of data. More precisely\, I will introduce our SED-fitting codes and the potential of J-PAS to determine the integrated properties of the stellar content of galaxies up to redshift z~1 (including age\, metallicity\, stellar mass\, etc.)\, techniques for the determination of the stellar mass and luminosity functions of galaxies in this kind of surveys\, and how to constrain the stellar population properties of spatially resolved galaxies up to 2-3 half light radius only using the miniJPAS/J-PAS images by means of a tool that we are developing in our group (IFU-like studies). \nFecha: 25/01/2024 – 12:30Conferenciante: Dr. Luis Alberto Díaz GarcíaFiliación: IAA – CSIC \n 
URL:https://www.iaa.csic.es/evento/stellar-population-studies-in-the-j-pas-survey/
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
BEGIN:VEVENT
DTSTART;VALUE=DATE:20240124
DTEND;VALUE=DATE:20240125
DTSTAMP:20260421T011808
CREATED:20240123T081104Z
LAST-MODIFIED:20240123T081537Z
UID:20313-1706054400-1706140799@www.iaa.csic.es
SUMMARY:COSMIC DUST WORKSHOP
DESCRIPTION:Informal workshop on Cosmic Dust (Wednesday 24th at Salón de Actos). The workshop is meant to trigger further discussions/collaborations with our visitors  Johannes Markkanen (SO-incoming visit)\, Karri Muinonen\,  Antti Penttilä and Gorden Videen (CODULAB visitors).
URL:https://www.iaa.csic.es/evento/cosmic-dust-workshop/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Workshops
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/congresscover-1-e1752660209538.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240118T123000
DTEND;TZID=Europe/Paris:20240118T123000
DTSTAMP:20260421T011808
CREATED:20240115T112605Z
LAST-MODIFIED:20250125T202711Z
UID:20258-1705581000-1705581000@www.iaa.csic.es
SUMMARY:A Year Beyond the Horizon: Advancing Our Understanding of M87* with New EHT Observations.
DESCRIPTION:In this presentation\, we introduce the first follow-up Event Horizon Telescope (EHT) observations of M87*\, taken a year after the epoch-making first image. The enhanced imaging\, facilitated by additional antennas\, increased data rates\, and new imaging techniques\, not only provides greater detail but also enables us to study the dynamics of the black hole within a year. Due to the embargo\, specific results are not included in this abstract\, but will be disclosed in a press release scheduled for January 18 at 08:00 UT\, just hours before this talk\, enabling a detailed exploration of these findings and their contribution to our understanding of black hole physics. \nFecha: 18/01/2024 – 12:30Conferenciante: IAA-CSIC EHT groupFiliación: IAA – CSIC \n 
URL:https://www.iaa.csic.es/evento/a-year-beyond-the-horizon-advancing-our-understanding-of-m87-with-new-eht-observations/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240116T123000
DTEND;TZID=Europe/Paris:20240116T123000
DTSTAMP:20260421T011808
CREATED:20240111T120254Z
LAST-MODIFIED:20250125T202723Z
UID:20221-1705408200-1705408200@www.iaa.csic.es
SUMMARY:UGR bureocrazy for dummies: PhDs fight back
DESCRIPTION:Every year we all wonder about the UGR bureaucracy: did we miss something? how could we have known in advance? Let’s face it\, it’s a mess. To try to help us all\, especially those who are just starting\, I would like to invite everyone interested to a seminar dedicated to understanding what the PhDs have to go through every year (paperwork related)\, where to find the proper information\, who to contact in case of doubt and how to go through the PhD paperwork a bit more smoothly. \nFecha: 16/01/2024 – 12:30Conferenciante: Teresa ToscanoFiliación: IAA – CSIC \n 
URL:https://www.iaa.csic.es/evento/ugr-bureocrazy-for-dummies-phds-fight-back/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240111T123000
DTEND;TZID=Europe/Paris:20240111T133000
DTSTAMP:20260421T011808
CREATED:20231212T092434Z
LAST-MODIFIED:20250911T092757Z
UID:20148-1704976200-1704979800@www.iaa.csic.es
SUMMARY:SO Colloquium: MOSAIC the high multiplex and multi-IFU spectrograph for the ELT
DESCRIPTION:MOSAIC is the planned multi-object spectrograph for the 39m Extremely Large Telescope (ELT). Conceived as a multi-purpose instrument\, it offers both high multiplex and multi-IFU capabilities at a range of intermediate to high spectral resolving powers in the visible and the near-infrared. In this talk I will showcase the key science cases that drive the top-level requirements and the adopted instrument architecture. With a planned first light in the early 2030s\, MOSAIC will enable unique spectroscopic surveys of the faintest sources\, from the oldest stars in the Galaxy and beyond\, to the first populations of galaxies that completed the reionisation of the Universe–while simultaneously opening up a wide discovery space and providing enormous synergies with upcoming multi-wavelength facilities (e.g.\, Euclid\, Rubin\, Roman\, SKA). \nFecha: 11/01/2024 – 12:30Conferenciante: Dr Ruben Sánchez-JanssenFiliación: STFC UK Astronomy Technology Centre The Royal Observatory Edinburgh \n 
URL:https://www.iaa.csic.es/evento/mosaic-high-multiplex-and-multi-ifu-spectrograph-elt/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios,SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231219T123000
DTEND;TZID=Europe/Paris:20231219T133000
DTSTAMP:20260421T011808
CREATED:20231218T120233Z
LAST-MODIFIED:20250125T202746Z
UID:20173-1702989000-1702992600@www.iaa.csic.es
SUMMARY:Fundamental Physics From Ground-Based Gamma-Rays Observations
DESCRIPTION:Crucial topics in fundamental physics\, such as the existence of new particles\, or violations of the Lorentz Invariance arising at the Planck scale\, can be effectively tackled in the cosmic environment\, by means of ground-based observations in the VHE gamma-ray band. This includes both Particle showers detectors\, such as LHAASO and Imaging Atmospheric Cherenkov Telescopes\, such as MAGIC\, H.E.S.S.\, or the forthcoming CTA and ASTRI Mini-Array. I will introduce\, without any objective of exhaustiveness\, how the existence of Axion-Like Particles (ALPs) or Lorentz Invariance Violations (LIV) have been investigated in the past\, or will be in the future\, by means of observations of some extragalactic sources such as blazars or GRBs. \nFecha: 19/12/2024 – 12:30Conferenciante: Dr. Giacomo BonnoliFiliación: Istituto Nazionale di Astrofisica\, Italy \n 
URL:https://www.iaa.csic.es/evento/fundamental-physics-from-ground-based-gamma-rays-observations/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231214T193000
DTEND;TZID=Europe/Paris:20231214T203000
DTSTAMP:20260421T011808
CREATED:20231212T085624Z
LAST-MODIFIED:20250125T010906Z
UID:20131-1702582200-1702585800@www.iaa.csic.es
SUMMARY:Dinosaurios express
DESCRIPTION:¡Todo el mundo sabe qué es un dinosaurio! ¿Seguro…? Bastantes animales son llamados dinosaurios sin serlo\, mientras que hay dinosaurios que difícilmente se identificarían como tales. En un recorrido sucinto por un linaje del que se dispone una información tan abrumadora como no siempre precisa\, repasaremos brevemente qué podemos saber de los dinosaurios a partir de sus huesos fosilizados y cuántas cosas interesantes conocemos de ellos sin tener ni uno solo de sus huesos. \nFecha: 14/12/2023 – 19:00Conferenciante: Luis AlcaláFiliación: Parque de las Ciencias de Granada \n 
URL:https://www.iaa.csic.es/evento/dinosaurios-express/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2023/12/diciembre-1.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231130T193000
DTEND;TZID=Europe/Paris:20231130T203000
DTSTAMP:20260421T011809
CREATED:20231120T122405Z
LAST-MODIFIED:20250125T010922Z
UID:19961-1701372600-1701376200@www.iaa.csic.es
SUMMARY:Jugando con la luz
DESCRIPTION:He preparado para esta conferencia una corta colección de experimentos\, como muestra de mi actividad académica de divulgación de la Física. Algunos de ellos forman parte del laboratorio de los “Diez experimentos más bellos de la Física”\, que he tenido la gratificante tarea de montar en la Facultad de Ciencias de la UGr. Por supuesto\, desde aquí le invito a que vengan a visitarlo. \nLos experimentos que les mostraré son: \n1.- Sombras de colores2.- Interferómetro de Michelson3.- Óptica Schlieren4.- Prisma de Newton \nY algunos otros… \nFecha: 30/11/2023 – 19:00Conferenciante: Miguel CabrerizoFiliación: Universidad de Granada \n 
URL:https://www.iaa.csic.es/evento/jugando-con-luz/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/noviembre-1.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231130T123000
DTEND;TZID=Europe/Paris:20231130T133000
DTSTAMP:20260421T011809
CREATED:20231127T084519Z
LAST-MODIFIED:20250911T092808Z
UID:20033-1701347400-1701351000@www.iaa.csic.es
SUMMARY:SO Colloquium: Studying star-formation in 'collisional' galaxies with MUSE
DESCRIPTION:Galaxies in pre- and post-collisional stages are an excellent laboratory to study the evolution of galaxies\, particularly the triggering and suppression of star formation on galactic scales before and after such interactions. In order to analyze the star formation triggered in these systems\, we started a series of studies on ‘collisional’ galaxies with available integral field spectroscopy (IFS) observations. We use Very Large Telescope (VLT) Multi-Unit Spectroscopic Explorer (MUSE) observations to study the young star cluster complexes and H ii regions in the Antennae\, Cartwheel\, and the double-ring collisional galaxy AM 0644-741. MUSE datacubes offer the opportunity to address several problems that are particular to these galaxies\, such as studying the ionizing mechanisms and the chemical abundances in the star cluster complexes hosted in the H ii regions. IFS data also offers an opportunity to unveil the presence of populations of Wolf-Rayet stars and the sources of high ionization potential emission lines (e.g.\, He II 4686) in the nearby universe. We present our recent findings in this seminar. \nFecha: 30/11/2023 – 12:30Conferenciante: Dr. Victor Mauricio A. Gómez GonzálezFiliación: Institute for Physics and Astronomy\, University of Postdam\, Germany \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-studying-star-formation-collisional-galaxies-muse/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios,SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20231127
DTEND;VALUE=DATE:20231202
DTSTAMP:20260421T011809
CREATED:20231109T181908Z
LAST-MODIFIED:20250912T081117Z
UID:19914-1701043200-1701475199@www.iaa.csic.es
SUMMARY:Severo Ochoa Advanced School on Star Formation
DESCRIPTION:The IAA-CSIC Severo Ochoa Advanced School on Star Formation will be held in Granada\, from Monday\, November 27th\, to Friday\, December 1st\, 2023. It is directed at researchers of all levels who have a special interest in star formation. This school will include an overview of basic concepts\, but aims to go beyond textbook knowledge by providing insight into the current frontiers of research and will have a strongly interactive aspect with ample room for questions and discussions. Lectures will be short ‘flash lectures’\, no longer than 30 min\, followed by questions and discussions. \nSOC: Rainer SchödelLOC: Alicia Pelegrina López\, Manuel González García
URL:https://www.iaa.csic.es/evento/severo-ochoa-advanced-school-on-star-formation/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/starformationso.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231123T123000
DTEND;TZID=Europe/Paris:20231123T133000
DTSTAMP:20260421T011809
CREATED:20231109T162054Z
LAST-MODIFIED:20250911T092822Z
UID:19809-1700742600-1700746200@www.iaa.csic.es
SUMMARY:SO Colloquium: The transition between super-Earths and sub-Neptunes: Interior and atmosphere modelling of the low-mass planet population
DESCRIPTION:Low-mass exoplanets are showing a diversity in their densities\, ranging from silicate-dominated super-Earths to volatile-rich sub-Neptunes. We have developed a coupled interior-atmosphere model that estimates the composition and interior structure of super-Earths and sub-Neptunes assuming water and CO2 atmospheres. The applications of the model include the homogenous analysis of a sample of multi-planetary systems\, as well as the assessment of the observability of emission spectra for rocky exoplanets with the James Webb Space Telescope. I will explain how their compositions connect to their possible formation site in the protoplanetary disk and their formation mechanisms\, including atmospheric escape\, and how we can break degeneracies with new atmospheric characterisation data. \nFecha: 23/11/2023 – 12:30Conferenciante: Dr. Lorena AcuñaFiliación: Max-Planck-Institute for astronomy\, Germany \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-the-transition-between-super-earths-and-sub-neptunes-interior-and-atmosphere-modelling-of-the-low-mass-planet-population/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios,SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231116T123000
DTEND;TZID=Europe/Paris:20231116T133000
DTSTAMP:20260421T011809
CREATED:20231109T160244Z
LAST-MODIFIED:20250912T071036Z
UID:19786-1700137800-1700141400@www.iaa.csic.es
SUMMARY:SO Colloquium: The evolution of the accretion process: investigating the protostellar phase to constraints planet formation
DESCRIPTION:The accretion process is responsible for the mass building during the star formation phase\, but our knowledge of this phenomenon is still not totally understood. On one side\, the magnetospheric accretion scenario describes the accretion on pre-main sequence (Class II/III) low-mass stars. However\, most of the material is supposed to be accreted during the earliest stages\, i.e. the protostellar phase (Class 0/I)\, when the forming star and its disk are embedded into a dusty envelope. The presence of the envelope and short lifetimes make the observations of these sources and their analysis challenging\, preventing us from testing this and other scenarios during the early stages. On the other hand\, the Gaia data alert project is increasing the number of the so-called «eruptive sources» (FUor\, EXors..)\, which were thought to represent only an exception in the accretion paradigm\, suggesting their presence in the stellar mass building to be more important than we thought. In the last decade\, thanks to new instruments and analysis techniques\, we’re starting to unveil the secrets of accretion on low-mass protostars\, finding many similarities between these sources and the eruptive stars and finally being able to provide quantitative information about accretion parameters during the overall star formation evolution. In this talk I will present the most recent results about the stellar mass building during the early stages and how they impact the planet formation. \nFecha: 16/11/2023 – 12:30Conferenciante: Dr. Fiorellino\, EleonoraFiliación: Istituto di Astrofisica e Planetologia Spaziali di Roma and Istituto Nazionale di Astrofisica \n 
URL:https://www.iaa.csic.es/evento/mosaic-the-high-multiplex-and-multi-ifu-spectrograph-for-the-elt/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20231116
DTEND;VALUE=DATE:20231118
DTSTAMP:20260421T011809
CREATED:20231109T182152Z
LAST-MODIFIED:20250912T081122Z
UID:19922-1700092800-1700265599@www.iaa.csic.es
SUMMARY:Severo Ochoa Basics of Neural Networks 2023
DESCRIPTION:Deep learning (DL) is a family of techniques widely used in multiple fields with excellent results. Unfortunately\, due to its steep learning curve\, its use is not as extended as desirable. Several domain-specific libraries have been developed to facilitate the use of these DL models with modest success. For the widespread adoption of these techniques\, researchers should be able to design and use their own DL models. Image classification is one of the main problems in astrophysics. \nSOCRainer Schödel (Chair)\, IAA-CSIC\, SpainLaura Darriba\, IAA-CSIC\, SpainJavier Moldón\, IAA-CSIC\, Spain
URL:https://www.iaa.csic.es/evento/severo-ochoa-basics-of-neural-networks-2023/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/neuralso.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231114T110000
DTEND;TZID=Europe/Paris:20231114T120000
DTSTAMP:20260421T011809
CREATED:20231109T180632Z
LAST-MODIFIED:20250912T081127Z
UID:19899-1699959600-1699963200@www.iaa.csic.es
SUMMARY:PySnacks 5: ASTROALIGN
DESCRIPTION:ASTROALIGN is a python module that can serve to align two astronomical images. It determines the solution by finding similar 3-point asterisms (triangles) in both images and estimating the affine transformation between them. ASTROALIGN is particularly useful when there is no WCS information available or when the images to be aligned have been taken at different wavelengths and initial “by eye” alignment is very challenging. In this 1h workshop I will impart a brief introduction into the capabilities of ASTROALIGN and how to use it. \n 
URL:https://www.iaa.csic.es/evento/pysnacks-5-astroalign/
LOCATION:On line
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/AstroAlign.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231114T080000
DTEND;TZID=Europe/Paris:20231115T190000
DTSTAMP:20260421T011809
CREATED:20231109T165952Z
LAST-MODIFIED:20250912T080419Z
UID:19840-1699948800-1700074800@www.iaa.csic.es
SUMMARY:Meeting on Light Pollution: Challenges and Responses for Monitoring it
DESCRIPTION:Light pollution has a direct impact on the environment\, on astronomical observations and on the starry sky as a heritage resource of humanity. Excessive light confuses the biological clocks of humans\, animals and plants with its spectral composition similar to daylight. As a result\, it makes it difficult to distinguish between day and night and between the seasons to which living organisms are physiologically attuned. Light pollution is therefore an environmental problem caused by the inappropriate use of artificial light (the pollutant) with a strong transboundary character because\, under the right conditions\, light can spread up to hundreds of kilometres away from its source. It can therefore affect habitats far away from the pollutant sources. \nFor this reason\, the Ministry of Science and Innovation of the Spanish government\, through the Instituto de Astrofísica de Andalucía of the Consejo Superior de Investigaciones Científicas\, is organising\, in collaboration with the Spanish Network of Studies on Light Pollution\, this international scientific meeting dedicated to addressing the pressing issues surrounding light pollution and its monitoring\, which is a matter of significant environmental and legal concern. This meeting is dedicated to addressing the pressing issues surrounding light pollution and its monitoring\, which is a matter of significant environmental and legal concern. \nThe program is structured into four insightful sessions: \nLegal and Environmental Justification for Monitoring Light Pollution: This session will delve into the legal frameworks and environmental imperatives driving the need for vigilant monitoring of light pollution. \nMeasurement of Light Pollution on Ground: Experts will share methodologies and latest technologies employed in measuring light pollution at the terrestrial level. \nSatellite Measurement of Light Pollution: This session will focus on the advancements in satellite technology aiding in the monitoring of light pollution from space. \nNeeds for Modelling Light Pollution: Discussions in this session will center around the requirements and strategies for accurate modelling of light pollution to aid in policy formulation and implementation. \n  \nNota de prensa \n			\n			\n				\n				\n				\n				\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				Advisory CommitteeAlejandro Sánchez (Head of AC)Salvador BaráJaime ZamoranoHelena VancovaFrank HolkerAndreas JechowKevin GastonManolis KogevinasKarolina Zielińska-DąbkowskaToñi VarelaFabio FalchiBenedikt HugginsYana YakushinaSusana MartinDavid GaladíPaco Colomer \n			\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				Local Organizing CommitteeAlicia Pelegrina (Head of LOC)Antxon AlberdiFrancisco Javier Moreno FuentesJose Manuel VílchezJose Luis OrtízSusana MartínMáximo BustamanteEmilio GarcíaCelia Navas \n			\n			\n				\n				\n				\n				\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				ORGANIZADO POR \n \n  \nLa Red Española de estudios sobra la contaminación lumínica y esta reunión están apoyados por la Ayuda RED2022-134733-T financiada por MICIU/AEI /10.13039/501100011033. Esta actividad también es parte de los proyectos PID2021-123417OB-I00 y PID2021-122842OB-C21\, financiado por MICIU/AEI/10.13039/501100011033/FEDER\, UE.
URL:https://www.iaa.csic.es/evento/meeting-on-light-pollution-challenges-and-responses-for-monitoring-it/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Meeting
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2023/11/LightPollution-scaled.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231109T120000
DTEND;TZID=Europe/Paris:20231109T123000
DTSTAMP:20260421T011809
CREATED:20240215T200403Z
LAST-MODIFIED:20250125T202834Z
UID:20362-1699531200-1699533000@www.iaa.csic.es
SUMMARY:Studying magnetic fields\, dynamics\, and fundamental physics near a black hole with current and future mm-VLBI instruments
DESCRIPTION:The Event Horizon Telescope (EHT) has imaged the black hole shadows of the supermassive black hole at the center of the galaxy M87 (M87*) and at the center of the Milky Way (Sgr A*). Polarimetric imaging of M87* with the EHT enabled significantly stronger inferences on the black hole and accretion parameters than total intensity data alone. Geometric modeling was a central tool for studying the structure of M87* and Sgr A* in total intensity. In the first part of the talk\, I will show the results of fitting a new polarimetric “m-ring” geometric model to EHT observations of M87*. Our geometric modeling results are generally consistent with imaging methods\, but they also enable studies of the black hole when imaging methods struggle\, such as nights with sparse coverage or weak signals. \nIn the second part of the talk\, I will focus on plans and science goals for future instruments. The Next-Generation EHT (ngEHT) will be a transformative enhancement of the EHT\, with array expansions and improvements allowing for\, e.g.\, high dynamic range imaging of AGN jets\, and for real-time movie reconstructions of variable sources like Sgr A*. With the ngEHT Analysis Challenges\, we explore the science capabilities of the ngEHT\, and develop new analysis algorithms capable of analyzing the large and complex ngEHT datasets. Finally\, I will give a brief overview of several proposals to image black holes using space-based telescopes\, which achieve order-of-magnitude angular resolution improvements compared to what is attainable from the ground and allow for high-precision tests of general relativity. \nFecha: 09/11/2023 – 12:30Conferenciante: Dr. Freek RoelofsFiliación: Center for Astrophysics\, Harvard & Smithsonian\, USA. \n 
URL:https://www.iaa.csic.es/evento/studying-magnetic-fields-dynamics-and-fundamental-physics-near-a-black-hole-with-current-and-future-mm-vlbi-instruments/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231031T123000
DTEND;TZID=Europe/Paris:20231031T133000
DTSTAMP:20260421T011809
CREATED:20231109T162310Z
LAST-MODIFIED:20250125T202844Z
UID:19814-1698755400-1698759000@www.iaa.csic.es
SUMMARY:Outflows from low to high luminous AGNs
DESCRIPTION:Outflows are believed to play a major role in the evolution of galaxies and are said to be ubiquitous within the active galactic nuclei (AGN) population. However\, we still lack a comprehensive view of their properties and impact in their host galaxies and the surrounding medium. If we focus on the low luminosity part of the AGN family\, in particular in low ionisation nuclear emission-line regions (LINERs)\, the impact of outflows is still largely unknown. I will present our recent work searching for outflows in LINERs using spatially resolved spectroscopy with the MEGARA/GTC instrument. We characterised the detected outflows and compared their properties with more luminous AGNs\, finding several discrepancies. Then I will focus on the case of a more luminous AGN\, the type-2 Seyfert NGC7172\, which was observed within the Galactic Activity\, Torus and Outflow Survey (GATOS) collaboration using MIRI/JWST data. I will present the first results on this galaxy\, for which an outflow was previously detected with both ionised and cold molecular gas in previous observations. \nFecha: 31/10/2023 – 12:30Conferenciante: Laura Hermosa MuñozFiliación: CAB\, INTA-CSIC\, Madrid\, Spain \n 
URL:https://www.iaa.csic.es/evento/outflows-from-low-to-high-luminous-agns/
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231024T090000
DTEND;TZID=Europe/Paris:20231025T200000
DTSTAMP:20260421T011809
CREATED:20231109T175024Z
LAST-MODIFIED:20250912T080633Z
UID:19882-1698138000-1698264000@www.iaa.csic.es
SUMMARY:ANDES technical meeting
DESCRIPTION:Reunión técnica del consorcio ANDES para el progreso en el diseño de los espectrografos UBV y RIZ de ANDES/ELT \n			\n			\n				\n				\n				\n				\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				SOCJoar BrynnelPedro AmadoJonay GonzálezBruno ChazelasChristine FuessleinManuel AmateMaría Rosa Zapatero Osorio \n			\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				LOCPedro AmadoRocío CalvoRoberto Varas
URL:https://www.iaa.csic.es/evento/andes-technical-meeting/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Workshop
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/congresscover-1-e1752660209538.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20231023T133000
DTEND;TZID=Europe/Paris:20231024T203000
DTSTAMP:20260421T011809
CREATED:20231108T084530Z
LAST-MODIFIED:20250912T080433Z
UID:19422-1698067800-1698179400@www.iaa.csic.es
SUMMARY:100xCiencia.7
DESCRIPTION:El Parque de las Ciencias de Granada acogerá el 23 y 24 de octubre la séptima edición de 100xCiencia\, el encuentro anual de la alianza SOMMa que reúnirá a la comunidad científica de los Centros de Excelencia Severo Ochoa y Unidades de Excelencia María de Maeztu. \n100xCiencia.7 está coorganizado por SOMMa junto a los anfitriones de este año: el Instituto de Astrofísica de Andalucía (IAA-CSIC) y el Instituto de Matemáticas de la Universidad de Granada (IMAG) \nEl Parque de las Ciencias de Granada acogerá el 23 y 24 de octubre la séptima edición de 100xCiencia\, el encuentro anual de la alianza SOMMa que reúnirá a la comunidad científica de los Centros de Excelencia Severo Ochoa y Unidades de Excelencia María de Maeztu. \n100xCiencia.7 está coorganizado por SOMMa junto a los anfitriones de este año: el Instituto de Astrofísica de Andalucía (IAA-CSIC) y el Instituto de Matemáticas de la Universidad de Granada (IMAG) y se desarrollará en dos jornadas: \nLunes 23 de octubre – Asamblea General SOMMa 2023 + Reuniones grupos de trabajo (WG) \n[Restringido a la Comunidad SOMMA] \n\n13:30-15:00h Networking lunch de bienvenida\n15:00-16:30h Asamblea General (restringido a directores/as)\n15:30-16:30h Working groups (Tramo I\, Planteamiento de temas)\n16:30-17:00h Coffee break conjunto (AG+WG)\n17:00-18:00h Working groups (Tramo II\, Conclusiones con asistencia de miembros del EC)\n20:00h Cena de la reunión (Restaurante La Chumbera)\n\nMartes 24 de octubre – Contar la ciencia con excelencia. \n[Restringido a la Comunidad SOMMA \nParque de las Ciencias \nEl objetivo es doble. Por un lado\, un conjunto de talleres dirigidos por expertos no necesariamente del ámbito de la comunicación científica\, en el que se aborden temas y aspectos que estando fuera de este ámbito son utilizados de manera habitual por profesionales de la comunicación.  Por otro lado\, una muestra de casos de éxito de proyectos de comunicación y divulgación liderados por centros SOMMA. \n\n09:30h Bienvenida y presentación\n09:40 – 13:00h Talleres de formación Contar la ciencia con excelencia: un conjunto de master class para profesionales de la comunicación de los centros Severo Ochoa y María de Maeztu.\n13:00 – 14:00h Casos de éxito de proyectos de comunicación y divulgación centros SOMMA\n14:00 – 14:30h Debate y conclusiones\n14:30h Networking Lunch\n\n[Abierto a la ciudadanía] \n\n19:00 – 20:30h Evento “7 preguntas para cambiar el mundo”\n\nAuditorio Parque de las Ciencias. \nGratuito hasta completar aforo.  \nCon el evento “Siete preguntas que cambiarán el mundo” pretendemos echar un vistazo bienintencionado a lo que se nos viene encima. Queremos jugar a imaginar cómo será la ciencia dentro de diez\, de veinte\, de cincuenta años…¿A qué se tendrá que enfrentarse? ¿Qué retos tendrá que asumir? ¿Qué capacidades alcanzaremos?  Vamos a intentar describir de una manera lo más realista posible el futuro. Pero\, ya os lo adelantamos: no lo vamos a conseguir. Si algo nos demuestra la historia de la ciencia y el desarrollo tecnológico es que lo más inteligente es abstenerse de intentar vaticinar nada. Surgirán nuevas tecnologías disruptivas\, cambiarán paradigmas\, caerán fundamentos aparentemente inamovibles\, surgirán ideas que nadie imaginó y se harán descubrimientos inesperados…o quizás nada de esto pase. Lo único cierto es que el horizonte se presenta preocupante. Que hay cosas que deben cambiarse sí o sí\, y que la ciencia y la tecnología deben ayudarnos a hacerlo. Marcar el camino. Aunque para ello\, hay que escuchar a los que saben. Y esto es lo que vamos a hacer.   \nOcho voces expertas hablarán en el presente de la ciencia del futuro. Intentarán responder siete preguntas clave que marcarán el camino de lo que está por venir\, del futuro que nos espera. Y todo ello envuelto de la música que emerge desde el pasado más tradicional y clásico hasta el presente. Arte de siempre para la ciencia y la tecnología del futuro.  \nSiete preguntas que cambiarán el mundo” (El estado del “arte” de la ciencia del futuro)  se enmarca dentro de 100xCiencia.7\, el encuentro anual de la alianza SOMMa que reúne a la comunidad científica de los Centros de Excelencia Severo Ochoa y Unidades de Excelencia María de Maeztu que en esta séptima edición acogerá a representantes de las 65 entidades que actualmente forman parte de la alianza.
URL:https://www.iaa.csic.es/evento/100xciencia-7/
LOCATION:Parque de las Ciencias\, Av. de la Ciencia s/n\, Granada\, 18006\, España
CATEGORIES:Actividades,SO Meeting
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