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X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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TZID:Europe/Paris
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250121T090000
DTEND;TZID=Europe/Paris:20251030T170000
DTSTAMP:20260410T012454
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;VALUE=DATE:20250930
DTEND;VALUE=DATE:20251003
DTSTAMP:20260410T012454
CREATED:20250903T075108Z
LAST-MODIFIED:20250912T080504Z
UID:26965-1759190400-1759449599@www.iaa.csic.es
SUMMARY:Programación Controladores Beckhof
DESCRIPTION:Los Controladores Lógicos Programables (PLCs) de la empresa Beckhoff son muy usados en la actualidad en muchos campos de la ingeniería industrial. Entre ellos\, en el área de la instrumentación para astronomía\, ya que el Observatorio Europeo Austral (ESO) los adoptó hace años como estándar para los sistemas de control de la instrumentación desarrollada para sus telescopios. Sus componentes principales son los PLCs basados en PCs\, también conocidos como soft-PLCs\, pero Beckhoff cuenta con un amplio catálogo de productos\, tales como paneles de control táctil\, tarjetas de entradas/salidas digitales y analógicas o fuentes de alimentación\, que permiten desarrollar sistemas de control de subsistemas o instrumentos completos a partir de un diseño modular. \nA día de hoy\, tres de los proyectos de instrumentación en curso en los que la UDIT participa (MOSAIC\, TARSIS\, PACOO) están basados en controladores Beckhoff\, lo que implica la necesidad de formación del personal encargado de su programación\, configuración y desarrollo. En años anteriores ya se celebró un curso de iniciación a la programación en entorno Beckhoff (2019) y otro más específico para el control de motores (2021). El curso que se propone ahora está enfocado en otros aspectos más especializados en el desarrollo de este tipo de sistemas\, tales como el uso de módulos de la familia TwinSafe\, que se centran en la redundancia y seguridad\, o la programación de dispositivos táctiles para la visualización y el control.»
URL:https://www.iaa.csic.es/evento/programacion-controladores-beckhof/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/09/monitor_programming_933392.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251003T123000
DTEND;TZID=Europe/Paris:20251003T133000
DTSTAMP:20260410T012454
CREATED:20250912T084237Z
LAST-MODIFIED:20250930T090827Z
UID:27166-1759494600-1759498200@www.iaa.csic.es
SUMMARY:Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis
DESCRIPTION:Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae\, Baryon Acoustic Oscillations\, Quasars\, and Gamma-Ray Bursts \nCosmological models and their parameters are widely debated\, especially about whether the current discrepancy between the values of the Hubble constant\, H 0\, obtained by Type Ia supernovae (SNe Ia) and the Planck data from the cosmic microwave background radiation could be alleviated when alternative cosmological models are considered. Thus\, combining high-redshift probes\, such as gamma-ray bursts (GRBs) and quasi-stellar objects (QSOs\, or quasars)\, together with baryon acoustic oscillations and SNe Ia is important to assess the viability of these alternative models and whether they can cast further light on the Hubble tension. \nIn this work\, for GRBs\, we use a three-dimensional relation between the peak prompt luminosity\, the rest-frame time at the end of the X-ray plateau\, and its corresponding luminosity in X-rays: the 3D Dainotti fundamental plane relation. Regarding QSOs\, we use the Risaliti-Lusso relation among the UV and X-ray luminosities for a sample of 2421 sources. We correct both the QSO and GRB relations by accounting for selection and evolutionary effects with a reliable statistical method. We here use both the traditional Gaussian likelihoods ( LG ) and the new best-fit likelihoods ( LN ) to infer cosmological parameters of nonflat Lambda cold dark matter (LambdaCDM) and flat wCDM models. We obtain for all the parameters reduced uncertainties\, up to 35% for H0\, when applying the new LN likelihoods in place of the Gaussian ones. \nOur results remain consistent with a flat LambdaCDM model\, although with a shift of the dark energy parameter w toward w < -1 and a curvature density parameter toward Omega k < 0. \nFecha y lugar: 03/10/2025 – 12:30 | Salón de ActosMaria Giovanna DainottiNational Astronomical Observatory of Japan (NAOJ) \n  \n 
URL:https://www.iaa.csic.es/evento/reducing-the-uncertainty-on-the-hubble-constant-up-to-35-with-an-improved-statistical-analysis/
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:20251006
DTEND;VALUE=DATE:20251011
DTSTAMP:20260410T012454
CREATED:20250716T091741Z
LAST-MODIFIED:20251003T095846Z
UID:26168-1759708800-1760140799@www.iaa.csic.es
SUMMARY:Eighth Workshop on Robotic Autonomous Observatories
DESCRIPTION:Sixteen years after the inaugural workshop in Málaga\, robotic and autonomous astronomical observatories have achieved remarkable advancements. The global number of automated facilities has grown substantially\, along with their capabilities in robotization\, autonomy\, and networking. These developments\, driven by the search for electromagnetic counterparts to gravitational waves (such as the groundbreaking detection in 2017)\, have profoundly influenced diverse areas of astrophysics and beyond\, including: \n\nFireball detection\nMinor planet studies\nExoplanet searches\nMonitoring variable stars in the Galaxy\nStudying active galactic nuclei\nSupernova detection and monitoring\nRapid follow-up of high-energy transients like gamma-ray bursts\nElectromagnetic counterparts to neutrino and gravitational waves\n\nThe workshop will also highlight the increasing importance of space debris surveillance and tracking\, the observation of Near-Earth Objects\, the role of robotic observatories in public outreach and education\, and their contributions to open science. \nThe Scientific Organizing Committee aims to deliver a dynamic program addressing scientific\, technical\, educational\, and outreach themes. \nWe encourage researchers\, engineers\, educators\, and enthusiasts working in these fields to join us at AstroRob2025. The success of this workshop series has been largely due to the active participation\, insightful presentations\, and engaging discussions contributed by its attendees. Your involvement is key to making the forthcoming workshop as fruitful and inspiring as previous editions. \n 
URL:https://www.iaa.csic.es/evento/eighth-workshop-on-robotic-autonomous-observatories/
LOCATION:Hotel Cabo de Gata El Toyo\, Almeria\, Urbanización El Toyo\, C. de los Juegos de Casablanca\, 04131\, Almería\, Retamar\, Almería\, 04131\, Spain
CATEGORIES:Congresos,Workshops
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/10/astrorob.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251006T080000
DTEND;TZID=Europe/Paris:20251010T170000
DTSTAMP:20260410T012454
CREATED:20251001T092000Z
LAST-MODIFIED:20251003T100418Z
UID:27544-1759737600-1760115600@www.iaa.csic.es
SUMMARY:IAU Symposium - The Hidden Beauty of the Galactic Outskirts
DESCRIPTION:The IAU Symposium ‘The Hidden Beauty of the Galactic Outskirts’ aims to bring together experts in galaxy formation and evolution to discuss the latest research\, challenges\, and future directions in the field. The symposium will take place in the historic city of Córdoba\, Spain\, from October 6-10\, 2025. \nCórdoba\, a UNESCO World Heritage Site\, offers a rich cultural and historical backdrop for this prestigious event. Participants will have the opportunity to explore the city’s stunning architecture\, including the famous Mosque-Cathedral\, and enjoy its vibrant cultural scene. The symposium will provide a platform for scientists to share their latest findings\, foster new collaborations\, and inspire future research. \nThe event is expected to attract around 150 participants from various countries\, creating a diverse and dynamic environment for knowledge exchange. Sessions will cover a wide range of topics\, from tidal streams and the disruption of satellite galaxies to the role of dark matter in galaxy formation. With a programme designed to encourage in-depth discussions and collaborative opportunities\, this symposium promises to be a milestone event in the field. \n  \n \n  \nAbstract:  \nThe Golden Age for low surface brightness Universe studies has begun. Data from the many ongoing and future ground-based surveys like DESI\, LSST\, and the Vera C. Rubin Observatory\, and space missions like Euclid or ARRAKIHS (First Spanish-led ESA mission)\, will open the door to discoveries on the history of formation and evolution of galaxies and\, most probably\, to constrain the nature of Dark Matter. \nThese data allow researchers to test models of galaxy formation that remained theoretical for many years. Studying the formation of galaxies through the analysis of faint structures in local galaxies’ outskirts can shed some light on the process of galaxy assembly and on the nature of the matter that rules the gravitational collapse of early Universe structures\, the dark matter. \nThis symposium will bring together experts on galaxy formation and evolution to identify current challenges in this research field\, report recent results and discoveries\, and define future science avenues. The main objective is to enrich the current ongoing discussions on the interpretation of the new data\, to detect synergies among research groups\, and to trigger the forging of new international collaborations. \n 
URL:https://www.iaa.csic.es/evento/iau-symposium-the-hidden-beauty-of-the-galactic-outskirts/
LOCATION:Rectorado de la Universidad de Córdoba\, Av. de Medina Azahara\, 5\, Poniente Sur\, Córdoba\, 14071\, Spain
CATEGORIES:Congresos
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/10/reducir-fotos.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251009T123000
DTEND;TZID=Europe/Paris:20251009T133000
DTSTAMP:20260410T012454
CREATED:20250925T082843Z
LAST-MODIFIED:20251002T105940Z
UID:27406-1760013000-1760016600@www.iaa.csic.es
SUMMARY:Unveiling Water Vapor Transport in the Martian Atmosphere: Unexpected discoveries by NOMAD/TGO
DESCRIPTION:Water is a key component of planetary atmospheres\, shaping their climate and habitability. On Earth\, Venus or Mars\, water vapor drives their atmospheric chemistry\, and serves as a crucial indicator for potential habitability. Understanding its transport\, condensation/sublimation\, and loss to space is essential for planetary evolution. In this context\, Mars offers a compelling case. Despite its current cold and dry state\, geological evidence suggests a wetter past. Today\, on Mars\, water vapor exists in trace amounts but plays a crucial role in many chemical and radiative processes. \nUntil recently\, knowledge of the vertical distribution of water vapor was limited to models and column density estimates. With the advent of the Trace Gas Orbiter (TGO)\, it has become possible to systematically probe the Martian atmosphere using the solar occultation technique. Already well established on Earth\, solar occultations provide detailed information on both the geographic and vertical distribution of trace species such as water vapor.TBD \nFecha y lugar: 09/10/2025 – 12:30 | Salón de ActosAdrián BrinesInstituto de Astrofísica de Andalucía (IAA-CSIC) \n  \n  \n 
URL:https://www.iaa.csic.es/evento/unveiling-water-vapor-transport-martian-atmosphere/
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:20251014T080000
DTEND;TZID=Europe/Paris:20251015T170000
DTSTAMP:20260410T012455
CREATED:20251117T084320Z
LAST-MODIFIED:20251117T084442Z
UID:28759-1760428800-1760547600@www.iaa.csic.es
SUMMARY:EPIC Technology Meeting on Photonics for Space at IAA
DESCRIPTION:This EPIC Technology Meeting on Photonics for Space will delve into the latest advancements and challenges in applying photonics technology to space and new space\, in harsh environments. Sessions will cover topics from the lastest development of photonic integrated circuits (PICs) for space\, emerging trends and challenges in the new space\, photonics for harsh environments\, and the role and challenges of photonics in earth observation for environmental monitoring. Hosted by Instituto de Astrofísica de Andalucía\, in Granada\, Spain\, it offers a unique opportunity for insightful discussions on the role of photonics in space within an environment rich in observatory\, astrophysics\, and space end-user expertise. The event aims to bring together industry experts to share insights\, explore research and development opportunities\, and facilitate efficient networking among participants.
URL:https://www.iaa.csic.es/evento/epic-technology-meeting-on-photonics-for-space-at-iaa/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Congresos
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/11/IMAGEN-WEB-NUEVA-2.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251016T090000
DTEND;TZID=Europe/Paris:20251017T170000
DTSTAMP:20260410T012455
CREATED:20250330T085559Z
LAST-MODIFIED:20250912T080500Z
UID:25280-1760605200-1760720400@www.iaa.csic.es
SUMMARY:SO Basics of Neural Networks 2025
DESCRIPTION:Deep learning (DL) is a family of techniques widely used in multiple fields with excellent results. Unfortunately\, DL has a steep  learning curve. Fortunately\, several domain-specific libraries have been developed to facilitate the use of DL models. \nFor 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 applications of DL  in astrophysics and offers a convenient way to learn about neural networks. The de facto standard to tackle this problem is Convolutional Neural Networks (CNN)\, a concrete deep learning architecture.  This course will serve as an introduction to Deep Learning with four  sessions with the following objectives: understanding the basics of neural networks\, getting to know the fundamental libraries and fundamental architectures\, learning how to train a CNN\, gaining confidence in using CNNs for image classification tasks\, and learning how to evaluate their preformance. \n\nSession 1: Deep Learning fundamentals\nSession 2: Convolutional Neural Networks fundamentals\nSession 3: Practical considerations in real-world CNNs\nSession 4: Evaluation\n\nThe tutor of this school is Dr Francisco Eduardo Sanchez Karhunen (Universidad de Sevilla). \nThere will be coffee breaks available to participants. \nContents\n\nSession 1: Deep Learning fundamentals\nSession 2: Convolutional Neural Networks fundamentals\nSession 3: Practical considerations in real-world CNNs\nSession 4: Evaluation \n\nFor more details\, see the agenda below. \nThe repository with contents and materials can be found in Github (TBC) \nOrganizing Committee \n\nRainer Schödel (Chair)\, IAA-CSIC\, Spain \nLaura Darriba\, IAA-CSIC\, Spain  \nJavier Moldón\, IAA-CSIC\, Spain 
URL:https://www.iaa.csic.es/evento/so-basics-of-neural-networks-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/2025/03/artificial-intelligence.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251016T123000
DTEND;TZID=Europe/Paris:20251016T133000
DTSTAMP:20260410T012455
CREATED:20250915T112430Z
LAST-MODIFIED:20251007T154724Z
UID:27208-1760617800-1760621400@www.iaa.csic.es
SUMMARY:The Stellar Halos of Galaxies and Outskirts of Galaxy Clusters: Clues to their Accretion History
DESCRIPTION:Understanding mass assembly at different scales is key to improving our knowledge on galaxy formation and evolution in general. Stellar halos of galaxies\, primarily formed through the accretion and merger of smaller objects\, preserve memory of their assembly history\, offering unique insight into the accretion and mass growth history of galaxies. During the last decade there has been significant progress\, both from the observational and numerical side\, to characterize stellar halos of Milky Way-mass galaxies. And more recently the outskirts of low-mass galaxies have also started to be explored. On the high mass end\, outskirts of galaxy clusters are also important observational probes of how these systems grow in a cosmological context and can provide insights into their accretion history. \nIn this talk\, I will present the main results both from observations and cosmological simulations that allow us to link the observed properties of stellar halos with the accretion history of their host galaxies. Additionally\, I will present the first kinematical measurement of a diffuse stellar halo beyond the Local Group\, the stellar halo of the edge-on galaxy NGC 4945\, using a novel technique. We couple new deep MUSE spectroscopic observations with existing HST imaging data to spectroscopically measure the radial line-of-sight heliocentric velocity and velocity dispersion in a field at 40 kpc (stellar halo field) along NGC 4945 major axis. If time permits\, I will introduce the 4MOST/CHANCES survey\, aimed at observing the outskirts of ~150 galaxy clusters. \nFecha y lugar: 16/10/2025 – 12:30 | Salón de ActosAntonela MonachesiUniversidad de La Serena\, Chile \n  \n 
URL:https://www.iaa.csic.es/evento/the-stellar-halos-of-galaxies-and-outskirts-of-galaxy-clusters-clues-to-their-accretion-history/
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:20251021
DTEND;VALUE=DATE:20251023
DTSTAMP:20260410T012455
CREATED:20251017T085900Z
LAST-MODIFIED:20251017T105903Z
UID:27769-1761004800-1761177599@www.iaa.csic.es
SUMMARY:Presentación final del estudio de viabilidad "Performance and Requirement Consolidation study" de CAIRT
DESCRIPTION:Durante los días 21 y 22 de octubre de 2025\, científicos de varios centros de investigación atmósferica de Europa\, propulsores de la misión CAIRT (The Changing-Atmosphere Infra-Red Tomography Explorer)\, propuesta a la ESA como una de las dos misiones espaciales en fase A como candidatas al programa Earth Explorer 11\, se reúnen en el IAA para exponer y debatir las conclusiones finales del estudio científico de dicha misión. \nEn concreto se trata de la presentación final de uno de los estudios de viabilidad de CAIRT\, el denominado «PerRec»\, «Performance and Requirement Consolidation study» de CAIRT. \n 
URL:https://www.iaa.csic.es/evento/presentacion-final-del-estudio-de-viabilidad-performance-and-requirement-consolidation-study-de-cairt/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Workshops
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/10/Earth_Explorer_11_candidate_mission_Cairt_pillars.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251021T123000
DTEND;TZID=Europe/Paris:20251021T133000
DTSTAMP:20260410T012455
CREATED:20250925T083021Z
LAST-MODIFIED:20251001T091143Z
UID:27410-1761049800-1761053400@www.iaa.csic.es
SUMMARY:Breaks in radial metallicity gradients of spiral galaxies
DESCRIPTION:Radial abundance gradients in spiral galaxy disks provide key constraints on chemical evolution and galaxy formation. While inside-out growth predicts negative gradients\, observations often reveal deviations such as inner drops or outer flattenings. \nI will present recent results from our group on O/H gradients in spiral galaxies using H II region data from the CALIFA survey. We apply an automated fitting procedure to explore correlations between the physical properties of galaxies and bulges and the presence of these inner drops\, seeking possible explanations for the observed variations. We also examine how ionization source classification and diffuse ionized gas (DIG) contamination influence the inner gradient. \nFinally\, I will present new results for the Milky Way based on planetary nebulae with improved distances from a recalibrated Hα surface brightness–radiusrelation and Gaia DR3 parallaxes. These indicate a flatter O/H gradient than previously reported\, with a slope change near 8 kpc\, coinciding with the corotation radius. \nFecha y lugar: 21/10/2025 – 12:30 | Salón de ActosProf. Oscar CavichiaInstituto de Fisíca e Química\, Universidade Federal de Itajubá\, Brasil \n  \n  \n 
URL:https://www.iaa.csic.es/evento/breaks-in-radial-metallicity-gradients-of-spiral-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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251023T123000
DTEND;TZID=Europe/Paris:20251023T133000
DTSTAMP:20260410T012455
CREATED:20250605T082742Z
LAST-MODIFIED:20251001T091417Z
UID:25766-1761222600-1761226200@www.iaa.csic.es
SUMMARY:SO Colloquium: WST - The Wide Field Spectroscopic Telescope
DESCRIPTION:The WST project aims to design and construct an innovative 10-metre class wide-field spectroscopic survey telescope (WST) in the southern hemisphere. It will feature the parallel operation of two cutting-edge instruments: a high-multiplex (30\,000)\, large field-of-view (3 square degrees) multi-object spectrograph (MOS) operating in both low- and high-resolution modes\, and a giant panoramic integral field spectrograph (IFS). \nWST’s ambitious top-level requirements place it well ahead of all existing and planned facilities. In its first five years of operation\, the MOS is expected to observe 300 million galaxies\, 25 million stars at low resolution\, and 2 million stars at high resolution\, while the IFS will deliver 4 billion spectra. These capabilities will enable transformative science across a wide range of astrophysical domains. \nA key strength of WST lies in the synergy between its MOS and IFS instruments\, offering highly complementary spectroscopic survey modes. This dual approach is central to the project’s scientific ambition. \nWST is envisioned as the next major facility for ESO following the ELT\, and a proposal will be submitted in response to the upcoming ESO Call for Ideas in 2027. The project is backed by a large consortium of leading institutes from nine European countries and Australia\, with deep expertise in astronomical instrumentation and survey science. \nFecha y lugar: 23/10/2025 – 12:30 | Salón de ActosProf. Roland BaconCRAL – Observatoire de Lyon\, France \n 
URL:https://www.iaa.csic.es/evento/wst-the-wide-field-spectroscopic-telescope/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251030T190000
DTEND;TZID=Europe/Paris:20251030T200000
DTSTAMP:20260410T012455
CREATED:20250924T112936Z
LAST-MODIFIED:20251007T160452Z
UID:27372-1761850800-1761854400@www.iaa.csic.es
SUMMARY:Estrellas con voz propia. PLATO y las últimas misiones espaciales en astrosismología
DESCRIPTION:Las estrellas\, además de luz propia\, tienen «voz» propia. Así como la luz de las estrellas nos ha dado desde hace tiempo valiosas informaciones sobre su atmósfera y composición\, las oscilaciones acústicas de las estrellas pulsantes\, esa «voz propia» que se viene observando desde hace pocas décadas a través de variaciones de brillo\, nos está revelando muchas de sus propiedades físicas y hasta su estructura interna. Además\, el descubrimiento de otros tipos de oscilaciones\, por ahora investigadas solo en modelos teóricos\, podrá potencialmente revolucionar la física estelar. \nDesde los hallazgos de las primeras variables por parte de Henrietta Leavitt hasta la próxima inminente misión espacial PLATO de la ESA\, pasando por las predecesoras Corot\, Kepler y TESS\, en esta charla veremos cómo el fascinante campo de la astrosismología desvela los secretos más íntimos de las estrellas a través de esa «voz propia» y cuál es el emocionante futuro que nos espera en la comprensión de la evolución y de las dinámicas estelares. \nFecha: 30/10/2025 – 19:00Conferenciante: Javier PascualFiliación: Instituto de Astrofísica de Andalucía (IAA-CSIC) \n 
URL:https://www.iaa.csic.es/evento/estrellas-con-voz-propia-plato-y-las-ultimas-misiones-espaciales-en-astrosismologia/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251031T090000
DTEND;TZID=Europe/Paris:20251031T140000
DTSTAMP:20260410T012455
CREATED:20250828T091037Z
LAST-MODIFIED:20250912T080455Z
UID:26919-1761901200-1761919200@www.iaa.csic.es
SUMMARY:Intellectual Property for Researchers
DESCRIPTION:IAA-CSIC\, Salón de Actos31 Oct 2025\, 9-11h and 12-14h \n\n Objectives\n\nAfter this seminar\, you will know how to: \n\nProtect your research results with legal instruments (patents\, copyright\, etc.)\nNot to infringe the intellectual property rights of others\nDisseminate your research results following the principles of open science\n\n\n Contents\n\n\nIntroduction\nBasic notions on Intellectual Property Rights\nIndustrial property\n\n(coffee break) \n\nCopyright\nSoftware licenses\nOpen data\, open science\n\n Instructor \nVíctor Rodríguez Doncel (1978)\, Profesor Titular de Universidad at the Department of Artificial Intelligence\, Universidad Politécnica de Madrid. Víctor regularly teaches intellectual property rights (IPR) for scientists\, and his research focuses on artificial intelligence and law. He is editor of several ISO/IEC standards on the representation of IPR and a W3C Recommendation. He is coordinating now a EU-funded project on the AI Regulation\, and this year he will give a talk at the Congreso de la Lengua Española on «Lengua\, IA y propiedad intelectual» in Arequipa\, invited by Real Academia Española de la lengua (RAE). \nThis event is supported by the «Center of Excellence Severo Ochoa» award to the Instituto de Astrofísica de Andalucía. We acknowledge financial support from the Severo Ochoa grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/501100011033 from the Instituto de Astrofísica de Andalucía.
URL:https://www.iaa.csic.es/evento/intellectual-property-for-researchers/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/08/Writing.jpg
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