BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Instituto de Astrofísica de Andalucía - ECPv6.17.1//NONSGML v1.0//EN CALSCALE:GREGORIAN METHOD:PUBLISH 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: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 BEGIN:DAYLIGHT TZOFFSETFROM:+0100 TZOFFSETTO:+0200 TZNAME:CEST DTSTART:20270328T010000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:+0200 TZOFFSETTO:+0100 TZNAME:CET DTSTART:20271031T010000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260723T123000 DTEND;TZID=Europe/Paris:20260723T133000 DTSTAMP:20260720T124948Z CREATED:20260601T122654Z LAST-MODIFIED:20260720T124948Z UID:33347-1784809800-1784813400@www.iaa.csic.es SUMMARY:SO Colloquium – Degendering Physics: Why So Slow? DESCRIPTION:Among the STEM disciplines\, physics has been long-known to exhibit the most skewed of gender gaps. It has been over a quarter of a century since attention has been drawn to the evidence that the over-representation of men at multiple levels in the physics enterprise is significant and global\, though to varying degrees. The evidence also has pointed to the cause being societal patriarchy leaching into academia and causing gender-based discrimination within\, a trend that is not tempered by the «objectivity» that is attributed to the physics discipline. Progress towards a more equitable and inclusive physics enterprise has been slow\, however. \nWhile the astrophysics sub-discipline could justifiably claim better progress\, I will argue that the slowness is because several mitigative interventions seek to address only the symptoms\, besides also being moulded by patriarchy. Clearly root causes need to be addressed instead\, which requires explicitly stepping away from the all-too-common “Fixing-the-women” approach\, and taking cognisance of the insights from social science scholarship. Interventions need to be interrogated on whether they will bring about long-term cultural transformation\, whether they exclude anyone and whether they could cause harm\, and whether as physicists we have really constructed «merit» in a way that actually promotes understanding our universe. Specific examples from across the globe will be discussed. \nFecha y lugar: 23/07/2026 – 12:30 | Salón de ActosPrajval ShastriThe International Centre for Radio Astronomy Research (ICRAR) URL:https://www.iaa.csic.es/evento/so-colloquium-degendering-physics-why-so-slow/ 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:20260722T123000 DTEND;TZID=Europe/Paris:20260722T133000 DTSTAMP:20260720T124930Z CREATED:20260601T122608Z LAST-MODIFIED:20260720T124930Z UID:33356-1784723400-1784727000@www.iaa.csic.es SUMMARY:Beyond being Cosmic Beacons: Insights on the Role of Accreting Supermassive Black Holes in Galaxy Assembly from the Story at z~0 DESCRIPTION:Supermassive black holes (SMBH) that are found in the centres of most galaxies comply with scaling relationships that imply hand-in-hand growth of the SMBH and its galaxy bulge\, which in turn implies that the SMBHs play a significant role in regulating galaxy assembly. SMBHs grow via coalescence as a consequence of their host galaxies merging or due to accretion. Our current broad understanding is that the SMBHs influence star formation via the consequences of accretion\, which enables them to impact their environments out to spatial scales that are well beyond their gravitational sphere of influence. However\, the exact mechanisms and the circumstances under which positive and negative feedback dominate remain elusive. \nI will describe a multi-frequency investigation of the imprints if any at very nearby redshifts of this feedback between the accretion around the SMBH and star formation in the host galaxy. \nFecha y lugar: 22/07/2026 – 12:30 | Salón de ActosPrajval ShastriThe International Centre for Radio Astronomy Research (ICRAR) \n  URL:https://www.iaa.csic.es/evento/beyond-being-cosmic-beacons-insights-on-the-role-of-accreting-supermassive-black-holes-in-galaxy-assembly-from-the-story-at-z0/ 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:20260717T123000 DTEND;TZID=Europe/Paris:20260717T133000 DTSTAMP:20260714T193346Z CREATED:20260706T121912Z LAST-MODIFIED:20260714T193346Z UID:34538-1784291400-1784295000@www.iaa.csic.es SUMMARY:Southern Hemisphere Asteroid Radar Program (SHARP) DESCRIPTION:Precise knowledge of asteroid orbits and properties such as shape\, rotation state and existence of satellites is essential to assess the extent that they might represent impact hazards to the Earth\, and astronomical radar observations have been used to obtain that. Historically\, Goldstone and Arecibo planetary radar capabilities have made significant contributions to tracking many asteroids. However\, their coverage has been limited to the northern hemisphere sky and consequently have missed a fraction of NEAs during Earth flybys. \nTo fill the gap\, in recent years we have developed and demonstrated the Southern Hemisphere Radar Program (SHARP) capability using the Canberra Deep Space Communication Complex (CDSCC)\, part of the NASA Deep Space Network (DSN)\, as transmitters and the Australia Telescope Compact Array (ATCA) and Murriyang\, the Parkes 64m Radio Telescope\, and more recently University of Tasmania radio telescopes such as Ceduna 30-m dish as receivers. From the start of the project in 2015 to early 2026\, we have detected a total of 43 near-Earth asteroids. \nFecha y lugar: 17/07/2026 – 12:30 | Salón de ActosShinji HoriuchiCSIRO Space & Astronomy/NASA Canberra Deep Space Communication Complex \n  URL:https://www.iaa.csic.es/evento/southern-hemisphere-asteroid-radar-program-sharp/ 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:20260713 DTEND;VALUE=DATE:20260718 DTSTAMP:20260720T122603Z CREATED:20260720T121140Z LAST-MODIFIED:20260720T122603Z UID:34613-1783900800-1784332799@www.iaa.csic.es SUMMARY:XVII Reunión Científica de la SEA 2026 DESCRIPTION:La Sociedad Española de Astronomía se complace en anunciar la celebración de su XVII Reunión Científica\, que tendrá lugar en la ciudad de Tarragona del 13 al 17 de julio de 2026. Este encuentro bienal constituye el foro más importante para el intercambio y la difusión de los avances en la investigación astronómica en nuestro país\, así como una oportunidad única para reforzar la colaboración entre instituciones y profesionales tanto a nivel nacional como internacional. \nEl encuentro está dirigido a profesionales\, estudiantes de máster\, grado y posgrado\, así como a astrónomos aficionados\, cuya contribución resulta esencial para el desarrollo de nuestra disciplina. \nTarragona\, una ciudad con una larga tradición científica y cultural\, ofrecerá un marco excepcional para la discusión\, el debate y la creación de nuevas colaboraciones que impulsarán la astronomía en el siglo XXI. \n  \n  \n \n  URL:https://www.iaa.csic.es/evento/xvii-reunion-cientifica-de-la-sea-2026/ CATEGORIES:Congresos ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/07/Captura-de-pantalla-2026-07-20-a-las-14.06.25.jpg END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20260706 DTEND;VALUE=DATE:20260711 DTSTAMP:20260608T092915Z CREATED:20260608T092747Z LAST-MODIFIED:20260608T092915Z UID:33528-1783296000-1783727999@www.iaa.csic.es SUMMARY:HoRS3S Conference DESCRIPTION:HoRS3S\nHigh-Resolution Exoplanet and Stellar Characterization Today and in the ELT Era\n…\n  \nHoRS3S will take place in the magical city of Granada (Spain) between July 6 and 10\, 2026. \nTwo years after the second HoRSE workshop in Berlin\, experts on all aspects of high-resolution spectroscopy are invited to gallop into southern Spain and discuss the latest developments in the field of exoplanet and stellar characterization. This year’s edition will rein in strongly on next-generation facilities such as the ELT\, synergies with JWST and solar instrumentation\, and the latest on observations\, data analysis and modeling. Expect lively discussions and scientific exchange that’s anything but a one-horse race. \nThe venue\, the School of Architecture of the University\, is located in the beautiful old Jewish quarters («Barrio del Realejo») just immediately below the magnificent Alhambra palace. We know Granada heats up in summer\, but fear not — we’ve planned for plenty of water to keep the whole stable cool and hydrated. \nSOC: Megan Bedell\, Matteo Brogi\, Andrea Chiavassa\,  Elisa Delgado Mena\, Laura Kreidberg\, Karin Lind\, Christophe Lovis\, Rafael Luque (chair)\, Paul Molliere\, Vivien Parmentier\, Julia Seidel\, Yapeng Zhang \nLOC: Rafael Luque (chair)\, Alejandro Sanchez Lopez (co-chair)\, Francisco Pozuelos\, Gabriela Gilli\, Alberto Pelaez\, Cristina Rodriguez Lopez\, Emilo Garcia\, Alicia Pelegrina\, Amanda Lopez\, Celia Navas \n  URL:https://www.iaa.csic.es/evento/hors3s-conference/ LOCATION:Escuela Técnica Superior de Arquitectura de Granada (ETSAG-UGR)\, Campo del Príncipe\, s/n\, Centro\, Granada\, Granada\, 18071\, Spain CATEGORIES:Congresos ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/06/Captura-de-pantalla-2026-06-08-a-las-11.21.14.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260702T123000 DTEND;TZID=Europe/Paris:20260702T133000 DTSTAMP:20260624T185214Z CREATED:20260407T135527Z LAST-MODIFIED:20260624T185214Z UID:30805-1782995400-1782999000@www.iaa.csic.es SUMMARY:SO Colloquium – Filaments: from the large-scale structure to the CGM DESCRIPTION:I will present a characterisation of filamentary structures at different scales\, from the large-scale cosmic filaments forming the skeleton of the cosmic web\, to the smaller-scale filaments playing a crucial role in the circum-galactic medium (CGM). \nUsing the outputs of recent large-scale hydro-dynamical simulations\, I will focus on some fundamental properties of filaments at z=0\, and show how cosmic filaments evolved since z=4. In the second part of my talk\, I will zoom into CGM scales to show how the smaller-scale filaments (or streams) influence the star-formation activity of galaxies\, and present the latest observational detections using a combination of the miniJPAS and DESI datasets. I will conclude on the importance of understanding the multi-scale nature of the cosmic web and discuss prospects for observing filamentary structures with current and future multi-wavelength datasets. \nFecha y lugar: 02/07/2026 – 12:30 | Salón de ActosDaniela Galárraga EspinosaKavli Institute for the Physics and Mathematics of the Universe (IPMU) – Tokyo\, Japan URL:https://www.iaa.csic.es/evento/so-colloquium-filaments-from-the-large-scale-structure-to-the-cgm/ 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:20260630T123000 DTEND;TZID=Europe/Paris:20260630T133000 DTSTAMP:20260615T110504Z CREATED:20260507T072827Z LAST-MODIFIED:20260615T110504Z UID:31204-1782822600-1782826200@www.iaa.csic.es SUMMARY:The Occultation Portal: A Distributed Platform for Stellar Occultations DESCRIPTION:The Occultation Portal (OP) is a scientific infrastructure originally developed within the ERC Lucky Star collaboration to support the coordination\, archiving\, and analysis of stellar occultation campaigns. It now provides the wider community with coordinated access to predictions\, datasets\, and analysis tools\, and supports several international programmes\, including our efforts at IAA–CSIC on trans-Neptunian objects and irregular satellites\, for which occultations are essential to measure sizes\, shapes\, atmospheres\, and ring systems. \nThe Portal has recently been redesigned as a distributed system\, combining centralized campaign coordination and data curation with dedicated analysis capabilities for resource-intensive workflows such as astrometric alignment\, photometry\, light-curve extraction\, and limb fitting. This architecture is designed to scale to additional sites through secure data exchange and automated synchronisation between nodes. \nIn the era of Gaia astrometry\, DR3 and beyond\, and the forthcoming LSST/Rubin survey — both driving a rapid increase in predictable stellar occultations — the OP is becoming an increasingly important data hub for the community. In this talk\, I will introduce the Portal to the IAA community\, present its new distributed architecture\, and highlight the main scientific and technical developments behind it. \nFecha y lugar: 30/06/2026 – 12:30 | Salón de ActosYucel KilicIAA-CSIC \n  \n  URL:https://www.iaa.csic.es/evento/the-occultation-portal-a-distributed-platform-for-stellar-occultations/ 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:20260629 DTEND;VALUE=DATE:20260704 DTSTAMP:20260629T121458Z CREATED:20260629T121104Z LAST-MODIFIED:20260629T121458Z UID:34269-1782691200-1783123199@www.iaa.csic.es SUMMARY:TALES OF BLACK HOLES DESCRIPTION:TALES OF BLACK HOLES\nINTERNATIONAL DOCTORAL SUMMER SCHOOL ON ADVANCED BLACK HOLE PHYSICS\n\nBlack holes are among the most fascinating objects in the universe. From cosmological\, galactic and stellar scales\, where black holes are integral pieces in the formation and evolution of different structures\, to microscopic scales\, where the study of the fabric of spacetime and black hole interiors are interrelated\, black holes are ubiquitous in all research areas in which gravity is a prominent actor. A proper understanding of many aspects of modern physics requires being familiar with the concept of black hole; conversely\, comprehending black holes in all their dimensions requires extensive knowledge in diverse branches of physics\, including geometry\, thermodynamics\, fluid dynamics\, quantum field theory and numerical analysis. \nThis summer school will offer PhD and MSc students the opportunity to gain a solid understanding of the theory\, phenomenology and observations of black holes and acquire a broad perspective of current research tendencies. Lectures covering each of these aspects will be delivered by three leading international experts. \nThe school will take place in the historical Carmen de la Victoria at the heart of the Albayzín\, the old Arab neighborhood of Granada\, where all participants will be hosted on a full board basis. The Carmen de la Victoria faces the famous Alhambra\, the place of inspiration of the popular book by Washington Irving that the name of the school pays homage to. \n\n\n\n\n\n\n\nOrganizers\nRaúl Carballo-Rubio (IAA-CSIC)\nJavier Olmedo (UGR)\nCarlos Barceló (IAA-CSIC)\nJosé Luis Gómez (IAA-CSIC)\nMar Bastero Gil (UGR)\nMiguel Sánchez Portal (IRAM) \n\n\nParticipating institutions\n  \n\n\n\n  \nAcknowledgments: The organisers acknowledge financial support from the University of Granada through the ”Programa de Apoyo a la Organización de International Doctoral Summer Schools en el seno de las Escuelas de Doctorado de la UGR”\, and the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (grant CEX2021-001131-S 10.13039/501100011033). The school is affiliated to the ”Programa de Doctorado en Física y Ciencias del Espacio” of the University of Granada. The school has also received financial support from the Red Española de Física de Ondas Gravitacionales (REDONGRA\, grant RED2024-153735-E) and the Sociedad Española de Gravitación y Relatividad (SEGRE). The organizers acknowledge technical support provided by the Centro de Cálculo at IAA-CSIC. URL:https://www.iaa.csic.es/evento/tales-of-black-holes/ LOCATION:Carmen de la Victoria\, Cuesta del Chapiz 9\, Granada\, 18010\, Spain CATEGORIES:Congresos ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/06/blackhole2.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260625T190000 DTEND;TZID=Europe/Paris:20260625T200000 DTSTAMP:20260616T074051Z CREATED:20260615T102601Z LAST-MODIFIED:20260616T074051Z UID:31032-1782414000-1782417600@www.iaa.csic.es SUMMARY:Subneptunos: los mundos más comunes… ¿y los más habitables? DESCRIPTION:Los subneptunos (planetas de tamaño entre la Tierra y Neptuno) son el tipo de planeta más abundante en la galaxia\, aunque no existen en nuestro Sistema Solar. \nEn esta charla presentaré cómo los detectamos y qué hemos aprendido sobre su formación y diversidad a partir de estudios demográficos y el descubrimiento de sistemas individuales con propiedades únicas. Más allá de su naturaleza aparentemente inhóspita\, discutiré si estos planetas podrían albergar condiciones favorables para la vida\, desde atmósferas templadas hasta interiores ricos en agua. Una pregunta abierta que podría cambiar nuestra idea de habitabilidad en el universo. \nFecha: 25/06/2026 – 19:00Conferenciante:  Rafael LuqueFiliación:  Instituto de Astrofísica de Andalucía (IAA-CSIC) \n  \n  URL:https://www.iaa.csic.es/evento/subneptunos-los-mundos-mas-comunes-y-los-mas-habitables/ 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/2026/06/lucas-lara_junio26.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260625T123000 DTEND;TZID=Europe/Paris:20260625T133000 DTSTAMP:20260615T105908Z CREATED:20260416T120143Z LAST-MODIFIED:20260615T105908Z UID:31109-1782390600-1782394200@www.iaa.csic.es SUMMARY:LPAC-Lab: Laboratorio de Astronomía Cuántica La Palma DESCRIPTION:LPAC-Lab is an IAA-CSIC laboratory currently being established at PLOCAN’s BECOMAR center in Tazacorte\, La Palma. It will serve as the technological and operational hub of the La Palma Quantum Interferometer (LPQI)\, connecting cutting-edge quantum astronomy with innovation\, training\, technology transfer\, and sustainable development in La Palma. \nFecha y lugar: 25/06/2026 – 12:30 | Salón de ActosFrancisco PradaIAA-CSIC \n  \n  URL:https://www.iaa.csic.es/evento/lpac-lab-laboratorio-de-astronomia-cuantica-la-palma/ 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:20260618T123000 DTEND;TZID=Europe/Paris:20260618T133000 DTSTAMP:20260615T105754Z CREATED:20260123T100555Z LAST-MODIFIED:20260615T105754Z UID:29319-1781785800-1781789400@www.iaa.csic.es SUMMARY:Particle acceleration and non-thermal radiation in young star clusters DESCRIPTION:Cosmic ray acceleration up to PeV energies has been suggested to take place in massive and young stellar clusters. The formation of a strong termination shock driven by the collective action of stellar winds in a compact cluster offers a promising location where efficient particle acceleration might take place. The subsequent hadronic collisions of these particles result into gamma-ray and neutrino production. \nWithin a scenario of particle acceleration at the cluster wind termination shock\, we compute the expected gamma-ray and neutrino signals from both observed star clusters from the Gaia satellite as well as from the overall Galactic cluster population\, evaluating detection prospects for both source and diffuse emissions from this source population by very-high-energy gamma-ray and neutrino instruments\, as CTA\, KM3NeT\, and IceCube. \nFecha y lugar: 18/06/2026 – 12:30 | Salón de ActosSilvia CelliSapienza University of Rome \n  \n  URL:https://www.iaa.csic.es/evento/particle-acceleration-and-non-thermal-radiation-in-young-star-clusters/ 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:20260616T123000 DTEND;TZID=Europe/Paris:20260616T133000 DTSTAMP:20260615T105232Z CREATED:20260407T140657Z LAST-MODIFIED:20260615T105232Z UID:30821-1781613000-1781616600@www.iaa.csic.es SUMMARY:Decoding the clockwork of repeating nuclear transients: unveiling black hole environments with optical polarimetry DESCRIPTION:Repeating nuclear transients are quasi-periodic outbursts occurring in galactic nuclei\, driven by episodic accretion onto supermassive black holes (SMBHs). These events provide unique laboratories for advancing our understanding of accretion physics\, yet the innermost regions of most galactic nuclei remain inaccessible to direct imaging. More routinely observational approaches are therefore required to uncover the geometry and physical mechanisms governing these extreme environments. \nIn this talk\, I will present optical polarimetry as a powerful tool to probe the hidden structures surrounding SMBHs. I will show how polarimetric observations reveal the geometry of two different classes of repeating nuclear transients: ASASSN-14ko\, the most regularly repeating periodic nuclear transient known to date and a repeating partial tidal disruption event candidate\, and GSN069\, the prototype source of quasi-periodic eruptions. These results are part of POLTerDEIST\, a target-of-opportunity observational program combining data from OSN\, CAHA\, NOT\, and VLT\, which I will also introduce. \nFecha y lugar: 16/06/2026 – 12:30 | Salón de ActosBeatriz Agís GonzálezInstitute of Astrophysics at FORTH \n  \n  URL:https://www.iaa.csic.es/evento/decoding-the-clockwork-of-repeating-nuclear-transients-unveiling-black-hole-environments-with-optical-polarimetry/ 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:20260611T123000 DTEND;TZID=Europe/Paris:20260611T123000 DTSTAMP:20260601T110301Z CREATED:20260407T135831Z LAST-MODIFIED:20260601T110301Z UID:30809-1781181000-1781181000@www.iaa.csic.es SUMMARY:Taking Pictures and Making Movies of Supermassive Black Holes DESCRIPTION:Black holes are cosmic objects so small and dense\, that nothing\, not even light can escape their gravitational pull. Until recently\, no one had ever seen what a black hole actually looked like. Einstein’s theories predict that a distant observer should see a ring of light encircling the black hole\, which forms when radiation emitted by infalling hot gas is lensed by the extreme gravity near the event horizon. \nThe Event Horizon Telescope (EHT) is a global array of radio dishes that has now successfully imaged the 6.5 billion solar mass black hole at the center of galaxy M87\, and the 4 million solar mass black hole at the center of the Milky Way – both exhibiting the predicted strong gravitational lensing. Subsequent observations have revealed ordered magnetic fields on horizon scales with implications on how black holes launch relativistic jets of material. What’s next? The next-generation EHT (ngEHT) is a project to expand the EHT in several ways\, enabling us to make full-color\, high definition movies of black holes in pursuit of the next big questions. \nThis talk will cover the first EHT results\, future directions\, and progress towards realizing the ngEHT. \nFecha y lugar: 11/06/2026 – 12:30 | Salón de ActosShep DoelemanCenter for Astrophysics | Harvard & Smithsonian \n  \n  URL:https://www.iaa.csic.es/evento/taking-pictures-and-making-movies-of-supermassive-black-holes/ 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:20260609T123000 DTEND;TZID=Europe/Paris:20260609T133000 DTSTAMP:20260407T140515Z CREATED:20260407T140511Z LAST-MODIFIED:20260407T140515Z UID:30814-1781008200-1781011800@www.iaa.csic.es SUMMARY:The Index Diagram as a Tool to Disentangle Host Galaxy Contributions in Quasar Spectra DESCRIPTION:We revisit the Quasar Main Sequence (QMS) by investigating the impact of the stellar component from the host galaxy (HG) on the emission-line spectra of active galactic nuclei (AGN). After identifying SDSS-DR19 spectra with broad emission lines\, we constructed the Index diagram\, a novel\, model-independent diagnostic based on redshift-corrected spectra\, designed to efficiently identify sources with significant stellar HG contributions and to classify AGN spectra into three categories: HG-dominated (HGD)\, intermediate (INT)\, and AGN-dominated (AGND) sources. \nOur QMS analysis shows that HGD sources predominantly occupy the Population B region\, typically exhibiting negligible Fe II emission\, while INT and AGND sources display similar distributions in the Population A region. Cross-matching with radio\, infrared\, and X-ray catalogues reveals that the strongest radio emitters are preferentially associated with HGD and INT sources\, whereas strong X-ray emitters are found among INT and AGND objects\, which also populate the AGN region in the WISE colour diagram. The applicability of the Index diagram is also demonstrated by its implementation in large spectroscopic datasets\, including SDSS DR20 and DESI\, enabling systematic studies of AGN-HG decomposition across big data samples. \nFecha y lugar: 09/06/2026 – 12:30 | Salón de ActosAlenka NegreteInstituto de Astronomía – UNAM \n  \n  URL:https://www.iaa.csic.es/evento/the-index-diagram-as-a-tool-to-disentangle-host-galaxy-contributions-in-quasar-spectra/ 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:20260602T123000 DTEND;TZID=Europe/Paris:20260602T133000 DTSTAMP:20260601T105818Z CREATED:20260407T135242Z LAST-MODIFIED:20260601T105818Z UID:30800-1780403400-1780407000@www.iaa.csic.es SUMMARY:SO Colloquium – Atmospheric Dispersion Correction to detect Exo-Earths: EXOTICA\, ANDES\, and RISTRETTO DESCRIPTION:Astronomical observations with ground-based telescopes are affected by wavelength-dependent atmospheric dispersion\, due to the variation of the refractive index of the atmosphere with wavelength. In high-resolution imagers and spectrographs\, as used in exoplanet searches\, the use of an atmospheric dispersion corrector (ADC) is mandatory. \nState-of-the art ADCs will thus be implemented in EXOTICA\, ANDES and RISTRETTO. EXOTICA\, the recently proposed EXOplanet Tracker Instrument at Calar Alto\, is a high-resolution spectrograph for radial velocity monitoring of exoplanet candidates. ANDES\, the ArmazoNes high Dispersion Echelle Spectrograph\, is the high-resolution optical and near-infrared spectrograph for the ESO Extremely Large Telescope (ELT). RISTRETTO is a visible high-resolution spectrograph fed by an extreme adaptive optics (XAO) system\, to be proposed as a visitor instrument on ESO VLT. \nThe atmospheric dispersion has a strong impact on acquired images even after ADC correction. Fiber-fed seeing-limited spectrographs\, like EXOTICA and ANDES\, have different ADC requirements than diffraction limited instruments\, like RISTRETTO\, that imposes requirements at the level of few milli-arcseconds. On the other hand\, for planet-hunting spectrographs like ESPRESSO\, the ADC were over-engineered to reduce systematics to the cm/s-level. These very stringent requirements are almost impossible to achieve with traditional ADCs\, and as such the field is an area of active research. \nIn this talk\, I will present the three instruments as case studies for how ADC requirements are set and understood\, what is the traditional way to correct atmospheric dispersion\, and present the new concept we will adopt for RISTRETTO. \nFecha y lugar: 02/06/2026 – 12:30 | Salón de ActosBachar WehbeInstitute of Astrophysics and Space Sciences (Portugal) \n  URL:https://www.iaa.csic.es/evento/so-atmospheric-dispersion-correction-to-detect-exo-earths-exotica-andes-and-ristretto/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España CATEGORIES:Seminarios 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:20260528T190000 DTEND;TZID=Europe/Paris:20260528T200000 DTSTAMP:20260529T100002Z CREATED:20260518T115452Z LAST-MODIFIED:20260529T100002Z UID:31033-1779994800-1779998400@www.iaa.csic.es SUMMARY:Los eclipses en el arte DESCRIPTION:Los eclipses solares han sido una de las experiencias naturales más impactantes para la humanidad. La desaparición momentánea del Sol como fuente de vida\, orden y estabilidad\, ha despertado fascinación\, temor y asombro en prácticamente todas las culturas. Por ello\, los eclipses no solo han sido objeto de estudio astronómico\, sino que también se han convertido en poderosos símbolos artísticos\, religiosos y políticos. \nEsta charla propone un recorrido por distintas manifestaciones artísticas inspiradas en los eclipses solares a lo largo de la historia\, desde la Antigüedad hasta el arte contemporáneo. A través de diferentes periodos y culturas\, exploraremos cómo este fenómeno celeste ha sido interpretado\, representado y transformado en imágenes y obras de arte que reflejan la profunda fascinación que el eclipse ha ejercido sobre la humanidad. \nFecha: 28/05/2026 – 19:00Conferenciante:  María Balaguer JiménezFiliación:  Instituto de Astrofísica de Andalucía (IAA-CSIC) \n  \n  URL:https://www.iaa.csic.es/evento/los-eclipses-en-el-arte/ 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/2026/05/lucas-lara.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260528T123000 DTEND;TZID=Europe/Paris:20260528T133000 DTSTAMP:20260407T134157Z CREATED:20260302T161538Z LAST-MODIFIED:20260407T134157Z UID:30058-1779971400-1779975000@www.iaa.csic.es SUMMARY:SO Colloquium – What the Variability of Embedded Protostars Tells Us about Accretion: Past\, Present\, and Future DESCRIPTION:The James Clerk Maxwell Telescope (JCMT) has been monitoring eight nearby low-mass star-forming regions in the Gould Belt at submillimetre wavelengths for more than eight years to search for and quantify the time dependent brightness variability of the resident deeply embedded protostars. \nSecular variability is common among these protostars; greater than 25% of the sample show measurable long-term brightness changes and 10% show burst behaviour lasting months to years. We interpret this secular variability as reflecting changes in the mass accretion rate from the disk to the protostar\, as predicted by theoretical models of (proto)stellar assembly. For a subset of our sample we have contemporaneous mid-IR light-curves which allow additional constraints on the conditions responsible for the brightness variations\, confirming that the submillimetre variability is driven by changes in the dust temperature profile of the envelope. \nFurthermore\, we have combined\, for one source\, single dish and interferometric sub-mm monitoring\, which has allowed us to unambiguously recover a time lag in the variability at larger angular scales and use the results to confirm the envelope structure surrounding the embedded protostar. \nFecha y lugar: 28/05/2026 – 12:30 | Salón de ActosDoug JohnstoneNational Research Council Canada – Herzberg Astronomy and Astrophysics Research Centre \n  \n  URL:https://www.iaa.csic.es/evento/what-the-variability-of-embedded-protostars-tells-us-about-accretion-past-present-and-future/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España CATEGORIES:Seminarios 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:20260526T123000 DTEND;TZID=Europe/Paris:20260526T133000 DTSTAMP:20260512T094244Z CREATED:20260302T161423Z LAST-MODIFIED:20260512T094244Z UID:30054-1779798600-1779802200@www.iaa.csic.es SUMMARY:Round table - Astrophysical Jets in Contrasting Environments and Scales DESCRIPTION:Jets are present on multiple astrophysical scenarios\, from protostars to supermassive black holes. Despite the enormous differences in their energetics\, these jets appear to share several basic properties. Thanks to their proximity and the richness of their detectable multi-wavelength emission (free-free and synchrotron continuum\, as well as atomic\, ionized\, and molecular lines)\, the physical properties of protostellar jets can be studied in great detail\, together with their connection to the associated accretion disk\, the mechanisms responsible for their launching and collimation\, and their interaction with the surrounding environment. \nThe knowledge gained from young stellar objects may therefore offer valuable insights into jets in other astrophysical systems. Three experts will come together to explore this possibility\, discussing the similarities and differences among jets in various contexts. \nFecha y lugar: 26/05/2026 – 12:30 | Salón de ActosSylvie Cabrit (Observatoire de Paris\, France) & Doug Johnstone (National Research Council Canada – Herzberg Astronomy and Astrophysics Research Centre\, Canada) \n  URL:https://www.iaa.csic.es/evento/round-table-astrophysical-jets-in-contrasting-environments-and-scales/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España CATEGORIES:Mesas redondas ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2026/05/mesas-redondas.png END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260521T123000 DTEND;TZID=Europe/Paris:20260521T133000 DTSTAMP:20260518T153625Z CREATED:20260302T161002Z LAST-MODIFIED:20260518T153625Z UID:30049-1779366600-1779370200@www.iaa.csic.es SUMMARY:SO Colloquium - Origin and impact of protostellar outflows: the ALMA and JWST revolution DESCRIPTION:The birth of stars\, and of planets around them\, is universally associated with a spectacular bipolar ejection phenomenon that extends from stellar to parsec scales. Its manifestations include a narrow and fast axial jet\, surrounded by a broader and slower molecular outflow carrying a large amount of mass. \nThe exact origin of these dual phenomena\, their role in the removal of excess angular momentum\, and their impact on star and planet formation\, have all been a subject of fierce debate and active research over four decades. \nIn this talk\, I will review major progress on these topics obtained from new observational facilities (from the optical to the millimeter range) and from enhanced modeling capabilities. In particular\, I will highlight recent results from ALMA and JWST and how they could revolutionize our understanding of the origin and impact of protostellar outflows. \nFecha y lugar: 21/05/2026 – 12:30 | Salón de ActosSylvie CabritObservatory of Paris\, France \n  \n  URL:https://www.iaa.csic.es/evento/so-colloquium-origin-and-impact-of-protostellar-outflows-the-alma-and-jwst-revolution/ 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:20260518T100000 DTEND;TZID=Europe/Paris:20260519T140000 DTSTAMP:20260521T082528Z CREATED:20260521T082528Z LAST-MODIFIED:20260521T082528Z UID:32992-1779098400-1779199200@www.iaa.csic.es SUMMARY:PhD & JAE-Intro Days DESCRIPTION:Únete a nosotros en las Jornadas de Introducción al Doctorado y al JAE\, una plataforma exclusiva en la que los estudiantes de doctorado y máster presentarán sus proyectos de investigación y sus resultados. Este evento está diseñado para ofrecer a los científicos emergentes de nuestro instituto de investigación un entorno profesional y a la vez acogedor en el que presentar y defender sus trabajos innovadores. Hace hincapié en la difusión del conocimiento y constituye un componente fundamental de su formación como investigadores científicos. \nEste evento tiene como objetivo fomentar un ambiente colaborativo en el que los jóvenes intelectuales puedan recibir comentarios constructivos\, participar en debates estimulantes y mejorar sus habilidades de comunicación. La participación en este evento les ayudará a prepararse para futuros retos académicos y profesionales\, reforzando su confianza y exponiéndolos a procesos de revisión por pares. \nAdemás\, este workshop ofrecerá oportunidades para establecer contactos\, lo que permitirá a los participantes conectar con investigadores experimentados y compañeros\, lo que puede dar lugar a futuras colaboraciones. Este encuentro celebra la vibrante cultura intelectual de nuestro instituto y su compromiso con la excelencia académica. \n \n  URL:https://www.iaa.csic.es/evento/phd-jae-intro-days/ ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/05/Captura-de-pantalla-2026-05-21-a-las-10.12.28.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260514T123000 DTEND;TZID=Europe/Paris:20260514T133000 DTSTAMP:20260512T095420Z CREATED:20260119T144357Z LAST-MODIFIED:20260512T095420Z UID:29183-1778761800-1778765400@www.iaa.csic.es SUMMARY:GCM simulations of ice giants and mini-neptunes: an overview of our understanding of the atmospheric dynamics of these planets DESCRIPTION:Ice giants and Mini-Neptunes have a thick gaseous envelope dominated by hydrogen and helium\, enriched deep within with large amounts of water\, methane or other volatile compounds. Uranus and Neptune are the only known planets of this type in our solar system and can serve as a laboratory for studying this type of atmosphere. \nThe Voyager-2 spacecraft\, followed by numerous studies on large ground-based telescopes and the Hubble Space Telescope\, revealed intense jet streams and meteorological activity on these planets. Indeed\, the fastest zonal tropospheric winds in the solar system are found on Neptune (-400 m/s)\, while storm activity on both planets is no match for the gas giant planets. Despite these scientific motivations and advances in observational techniques\, the atmospheric dynamics of these planets remain very little known. To date\, global climate models (GCM) have never been able to reproduce zonal winds. The simulated winds were a factor of 10 to 100 lower than those observed. \nThe difficulties encountered in modelling atmospheric circulation on ice giants call into question the validity of the atmospheric circulation of mini-neptunes simulated to date by GCMs. The approximations to the primitive atmospheric equations used for the atmospheres of terrestrial planets (Earth\, Mars\, …) may no longer be valid in the case of H2-dominated atmospheres. In this talk\, we will attempt to explain the advances that have been made in understanding the atmospheric dynamics of this type of atmosphere by exploring the validity of various dynamic hypotheses. \nFecha y lugar: 14/05/2026 – 12:30 | Salón de ActosGwenaël Alan MilcareckIAA-CSIC \n  \n  URL:https://www.iaa.csic.es/evento/gcm-simulations-of-ice-giants-and-mini-neptunes-an-overview-of-our-understanding-of-the-atmospheric-dynamics-of-these-planets/ 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:20260513T123000 DTEND;TZID=Europe/Paris:20260513T133000 DTSTAMP:20260202T091226Z CREATED:20260202T090817Z LAST-MODIFIED:20260202T091226Z UID:29399-1778675400-1778679000@www.iaa.csic.es SUMMARY:Semi-analytic Analysis of Galaxy Evolution from the Local Universe to Intermediate Redshifts: The Role of Environment\, Kinematics\, and Feedback DESCRIPTION:Understanding galaxy evolution requires extracting physical information from integrated galaxy spectra\, including the coupled evolution of stars and gas. \nIn this talk\, I present a novel semi-analytic spectral-fitting approach that jointly and self-consistently constrains the chemical evolution of both stars and gas.The model incorporates gas inflow\, outflow\, and star formation processes\, and is fitted directly to galaxy absorption-line spectra\, while emission-line diagnostics are used to constrain the present-day gas-phase metallicity. Applying this framework to galaxies in the local Universe from SDSS-IV/MaNGA and at intermediate redshifts from COSMOS-WALL/LEGA-C\, we reconstruct their star formation and chemical enrichment histories in a self-consistent manner. Such analysis allows us to investigate how the interplay between gas accretion and outflows shapes galaxy evolution\, in particular how galaxies transition away from the star-forming main sequence and become quenched. \nWe further explore the roles of feedback from active galactic nuclei and supernovae\, as well as environmental and kinematic properties\, in regulating these processes. \nFinally\, I will discuss how forthcoming spectroscopic surveys such as WEAVE and 4MOST will provide critical data to further test and extend these scenarios. \nFecha y lugar: 13/05/2026 – 12:30 | Salón de ActosShuang ZhouINAF-OAB \n  URL:https://www.iaa.csic.es/evento/semi-analytic-analysis-of-galaxy-evolution-from-the-local-universe-to-intermediate-redshifts-the-role-of-environment-kinematics-and-feedback/ 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:20260506T190000 DTEND;TZID=Europe/Paris:20260506T210000 DTSTAMP:20260430T112236Z CREATED:20260430T111957Z LAST-MODIFIED:20260430T112236Z UID:31191-1778094000-1778101200@www.iaa.csic.es SUMMARY:Clementina y los planetas DESCRIPTION:  \nClementina y los Planetas es un proyecto de Nauta Teatro y el Instituto de Astrofísica de Andalucía – CSIC que fusiona arte\, ciencia y tecnología para explorar el universo cercano a través del teatro de objetos y la astrofísica. \nMediante la historia de Clementina\, que viaja entre planetas en busca de un mundo sostenible\, se promueve el diálogo entre ciencia y sociedad\, fomentando la conciencia pública sobre la ciencia. \nA pesar de la seriedad de los adultos\, Clementina era una niña pícara y divertida. Conocida como “La escapista” le encantaba inventar mundos imaginarios y mirar a la luna. Su clase favorita era la de astronomía. Acompañándola a todas partes estaba su amigo imaginario\, Mr.Telescopio\, un señor elegante y estirado cuya cabeza era un gran telescopio blanco. \nUna noche y tras una discusión familiar se escapó\, se dirigió a su antiguo colegio\, subió al tejado y decidió mirar para arriba: quería ver la luna. En el firmamento todo estaba oscuro\, tanto que ni siquiera encontraba la luna. De repente\, apareció un gran haz de luz que se agrandaba a cada segundo. Quizás sea una estrella fugaz\, se dijo\, y decidió llamarla para pedir un deseo… \nEl haz de luz era un gran cometa\, con una gran masa viviente de rocas de colores blancos naranjas y tintineantes que se acercó ondulando por el firmamento hasta el tejado de la escuela a escuchar a la niña. Los dos con una gran curiosidad por la otra criatura conversaron toda la noche y se hicieron amigos. Cometa le contó sus viajes por el universo y Clementina le habló de sus padres… \nTodos públicos (+8 años) \nCreación y dramaturgia: Nauta Teatro\nDirección y títeres: Rafael Rey\nAsistencia de dirección y dramaturgia: Manuel Mansilla\nElenco: Gabriela Amaro\, Patricio Mango\, Rafael Rey\nBanda sonora: Alba Ermida\nIluminación: Abril Fernández Ferrez\nPintura: Ángela Ríos\nFotografía y vídeo: Lucía García\nEscenografía y utilería: Abril Fernández Ferrez\, Ángela Ríos\, Gabriela Amaro\, Patricio Mango\, Rafael Rey \nUn proyecto coordinado por Sara Cazzoli (IAA-CSIC) \nUna producción del Instituto de Astrofísica de Andalucía (IAA-CSIC) y NAUTA TEATRO\, con la colaboración de la Fundación Española para la Ciencia y la Tecnología (FECYT). \n  \n  \n  URL:https://www.iaa.csic.es/evento/clementina-y-los-planetas/ LOCATION:Teatro Alhambra\, C. Molinos\, 56\, Centro\, Granada\, Granada\, 18009\, Spain CATEGORIES:Actividades ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/04/683584976_1471591738346523_7267830599552324730_n.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260430T190000 DTEND;TZID=Europe/Paris:20260430T200000 DTSTAMP:20260424T082921Z CREATED:20260415T120815Z LAST-MODIFIED:20260424T082921Z UID:31031-1777575600-1777579200@www.iaa.csic.es SUMMARY:En busca de Sagitario A*\, el agujero negro del centro de nuestra galaxia DESCRIPTION:El corazón de la Vía Láctea ha permanecido oculto durante siglos\, escondido tras densas nubes de gas y polvo que bloquean la luz visible. Sin embargo\, gracias al desarrollo de nuevas técnicas de observación\, hoy podemos vislumbrar más allá y descubrir Sagitario A*\, el agujero negro supermasivo que habita en su interior. \nEn esta charla recorreremos el camino que llevó a confirmar la existencia de este objeto extremo: una historia de avances tecnológicos\, ideas teóricas y el trabajo colectivo de la comunidad científica a lo largo de generaciones. También exploraremos los misterios que aún rodean el núcleo de nuestra galaxia. \n\n\n\n\nFecha: 30/04/2026 – 19:00Conferenciante:  Laly Gallego CanoFiliación:  Instituto de Astrofísica de Andalucía (IAA-CSIC) \n  URL:https://www.iaa.csic.es/evento/en-busca-de-sagitario-a-el-agujero-negro-del-centro-de-nuestra-galaxia/ 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/2026/04/lucas-lara-copia.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260430T123000 DTEND;TZID=Europe/Paris:20260430T133000 DTSTAMP:20260407T134843Z CREATED:20260407T134729Z LAST-MODIFIED:20260407T134843Z UID:30792-1777552200-1777555800@www.iaa.csic.es SUMMARY:SO Colloquium – Probing AGN Jet Physics Using Multiwavelength Observations DESCRIPTION:Active Galactic Nuclei (AGN) powered by supermassive black holes launch relativistic jets that emit across the electromagnetic spectrum. Studying this broad emission helps us understand particle acceleration\, jet structure\, and how energy is released in these extreme environments. \nIn this talk\, I will present recent multiwavelength studies that combine radio\, X-ray\, and gamma-ray observations of different AGN systems. This includes low-frequency uGMRT results from the Palomar-Green (PG) quasar sample\, which provide new insights into extended radio emission and its connection to accretion and jet power; broadband modeling of sources such as NGC 1275 and Pictor A\, revealing complex jet components and high-energy behavior; and constraints on the gamma-ray emission region in the quasar 3C 380 using radio-gamma correlations and SED modeling. Together\, these results show how observations from MHz radio to GeV gamma-rays can uncover the physical conditions within AGN jets and improve our understanding of their emission processes and unification. \nFecha y lugar: 30/04/2026 – 12:30 | Salón de ActosSanna GulatiNational Centre for Radio Astrophysics (NCRA-TIFR)\, Pune\, India \n  URL:https://www.iaa.csic.es/evento/probing-agn-jet-physics-using-multiwavelength-observations/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España CATEGORIES:Seminarios 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:20260423T123000 DTEND;TZID=Europe/Paris:20260423T133000 DTSTAMP:20260416T115947Z CREATED:20260416T115454Z LAST-MODIFIED:20260416T115947Z UID:31098-1776947400-1776951000@www.iaa.csic.es SUMMARY:SO Colloquium – Metasurface enabled astronomical polarimetry DESCRIPTION:The nanotechnology of metasurfaces is rapidly changing the landscape of applied optics. While traditional lensing systems may not benefit significantly from the new technology\, the ability of metasurfaces to manipulate light and its polarization state offers great advantages in applied polarimetry\, as in the case of the magnetic diagnostics of astrophysical plasmas. The Solar Imaging Metasurface Polarimeter (SIMPol) was a NASA funded project to demonstrate such a capability and advance the TRL of metasurfaces for application to polarimetrice observations from space. \nWe present the general concept of metasurface-enabled spectro-polarimetry\, as well as preliminary results from the test campaign of SIMPol at a major solar research facility. \nFecha y lugar: 23/04/2026 – 12:30 | Salón de ActosRoberto CasiniNSF NCAR \n\n  URL:https://www.iaa.csic.es/evento/so-colloquium-tbd-metasurface-enabled-astronomical-polarimetry/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España CATEGORIES:Seminarios 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:20260423T103000 DTEND;TZID=Europe/Paris:20260502T140000 DTSTAMP:20260512T080739Z CREATED:20260401T105730Z LAST-MODIFIED:20260512T080739Z UID:30531-1776940200-1777730400@www.iaa.csic.es SUMMARY:Área de la Ciencia - Feria del Libro de Granada 2026 DESCRIPTION:Un año más\, el Instituto de Astrofísica de Andalucía (IAA-CSIC) y la Estación Experimental del Zaidín (EEZ-CSIC) se unen para coordinar el “Área de la Ciencia” en la Feria del Libro de Granada\, un espacio dedicado a la divulgación científica para todos los públicos. \nDel 23 de abril al 2 de mayo\, el Área de Ciencia albergará más de cuarenta actividades totalmente gratuitas en pleno centro de la ciudad: talleres\, charlas\, presentaciones de libros\, pódcast en directo\, … Se trata de la novena edición de una iniciativa pionera en la que ciencia y literatura comparten espacio\, tiempo y público\, una fórmula que ha empezado a implantarse ya en otras ferias del libro. Cuenta con el apoyo del CSIC a través de la Vicepresidencia Adjunta de Cultura Científica y Ciencia Ciudadana y de la Delegación en Andalucía\, y la colaboración de ESERO-Spain\, proyecto educativo de la Agencia Espacial Europea liderado en España por el Parque de las Ciencias de Granada. \nLas actividades del Área de la Ciencia de la Feria del Libro de Granada se entroncan dentro de la programación del Desgranando Fest\, un festival de divulgación científica del 18 al 26 de abril \nPROGRAMACIÓN ÁREA DE LA CIENCIA FERIA DEL LIBRO DE GRANADA \nDel 23 de abril al 2 de mayo de 2026 \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n JUEVES 23 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 10:30 h \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n  \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:30 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n  ¿Quién quiere ser… de Graná?Montserrat Benítez & Estefanía ValenzuelaEscuela de Estudios Árabes (EEA-CSIC)Concurso divulgativo \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n Recetas del talento científico:¿genios o cabezotas?Elena González ReyInstituto de Parasitología y BiomedicinaLópez Neyra (IPBLN-CSIC)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n VIERNES 24 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 10:30 h \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n  \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:30 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n Otra historia de la música ¿Qué pensaría Bach de la música actual?Somos BMiguel Ángel CajigalEl BarroquistaPresentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n Los insectos comestibles Editorial CSIC y CatarataLigia DíazInstituto de Ciencia y Tecnología de Alimentos y Nutrición (ICTAN-CSIC)Presentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 21:00 h \n \n \n \n \n \n \n \n \n \n \n \n Lo que vale la cienciaEspecial Noche en blancoColectivo del Sainete TrágicoPequeña obra de teatro científico \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n SÁBADO 25 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 11:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 12:30 h \n \n \n \n \n \n \n \n \n \n \n \n La delgada línea entre la locura y la creatividadBinomioClara Peñalver & Javier S. BurgosPresentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:00 h  \n \n \n \n \n \n \n \n \n \n \n \n Viaja al radiotelescopio que leerá todo el cieloPlazas de CienciaEquipo SKAO-EspañaInstituto de Astrofísica de Andalucía (IAA-CSIC)Mesa de Realidad Virtual \n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:30 h \n \n \n \n \n \n \n \n \n \n \n \n Le seré sincero\, no pinta bienUn viaje a través del arte y la enfermedadCríticaÁlvaro CarmonaUniversidad Loyola AndalucíaPresentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:30 h \n \n \n \n \n \n \n \n \n \n \n \n ¿El universo se está vaciando? La Tensión de HubbleRaúl González DíazInstituto de Astrofísica de Andalucía (IAA-CSIC)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n DOMINGO 26 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 11:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n  \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 12:30 h \n \n \n \n \n \n \n \n \n \n \n \n TiburonesEditorial CSIC y CatarataAnabel ColmeneroInstitut de Ciències del Mar (ICM-CSIC)Presentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:30 h \n \n \n \n \n \n \n \n \n \n \n \n Explorando el universo más extremoPlazas de CienciaGrupo VHEGA-CTAOInstituto de Astrofísica de Andalucía (IAA-CSIC)Mesa de Realidad Virtual \n\n  \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:30 h \n \n \n \n \n \n \n \n \n \n \n \n Historias de ballenas y otros cetáceosGuadalmazánAna J. CáceresMylestringPresentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:30 h \n \n \n \n \n \n \n \n \n \n \n \n Minerales críticos: los recursos invisibles de nuestro futuroConcepción Fernández LeyvaInstituto Geológico y Minero de España (IGME-CSIC)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n LUNES 27 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil/inclusivo \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n Violencia de género\, cerebro y emoción: comprender para reparar María Pérez\, Julia Arnal\,Inma Garrido & Andrea BenítezUniversidad de Granada (UGR)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n El suelo: clave para una agricultura sostenible y circularBeatriz Gómez MuñozEstación Experimental del Zaidín (EEZ-CSIC)​Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n MARTES 28 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 10:30 h \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:30 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n Leche materna y fórmulas de nueva generación:la importancia de la nutrición en los primeros meses de vidaLeticia BenavidesEstación Experimental del Zaidín (EEZ-CSIC)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n Homo Imperfectus: el manual de quejas del cuerpo humanoEspasaInés Moreno SanchezLa Traumatóloga GeekPresentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n MIÉRCOLES 29 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n Carlos V y su legado universitario en GranadaMiriam TejeroUniversidad de Granada (UGR)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n Ingeniería tisular en Granada: del laboratorio de Histología a losprimeros medicamentos vivos en la clínicaJesús Chato-Astrain y Fernando CamposUniversidad de Granada (UGR)Conferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n JUEVES 30 DE ABRIL\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 10:30 h \n \n \n \n \n \n \n \n \n \n \n \n Talleres escolares \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:30 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n EclipsesCiencia para leerDirige y presenta Carmen Guerrero (CSIC)Con la ilustradora Noemí Fabra& Alejandro Sánchez de Miguel (IAA-CSIC)Podcast en directo \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n Las FuriasClara Peñalver\, Marga SánchezRomero & Susana EscuderoCon Rocío Benavente (periodista y verificadora)Podcast en directo \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n VIERNES 1 DE MAYO\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 11:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 12:30 h \n \n \n \n \n \n \n \n \n \n \n \n El dios incomprendido: el desafío del Clima en la historia de la humanidadDesperta Ferro EdicionesFrancisco JiménezInstituto Andaluz de Ciencias de la Tierra (IACT-CSIC)Presentación de libro \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n Tarde \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 17:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil/inclusivo \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 19:00 h \n \n \n \n \n \n \n \n \n \n \n \n Ni frío ni calorÓscar HuertasDesgranando FestConferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 20:00 h \n \n \n \n \n \n \n \n \n \n \n \n El Espacio de nuestras vidasManuel GonzálezESERO-EspañaConferencia de divulgación \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n SÁBADO 2 DE MAYO\n \n \n \n \n \n Mañana \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 11:00 h \n \n \n \n \n \n \n \n \n \n \n \n Taller infantil \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n 12:30 h \n \n \n \n \n \n \n \n \n \n \n \n Ciencia ciudadana para reciclar residuosGermán Tortosa Estación Experimental del Zaidín (EEZ-CSIC) Conferencia de divulgación URL:https://www.iaa.csic.es/evento/area-de-la-ciencia-feria-del-libro-de-granada-2026/ LOCATION:Fuente de las Granadas\, Pl. del Humilladero\, Granada\, Granada\, 18009\, España CATEGORIES:Actividades ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2026/04/IMAGEN-WEB-NUEVA-1.png END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260420T080000 DTEND;TZID=Europe/Paris:20260422T170000 DTSTAMP:20260422T081506Z CREATED:20260422T080642Z LAST-MODIFIED:20260422T081506Z UID:31168-1776672000-1776877200@www.iaa.csic.es SUMMARY:ACS & NOMAD SWT meeting DESCRIPTION:Esta semana ha tenido lugar en el Instituto de Astrofísica de Andalucía la reunión de los equipos científicos de los instrumentos ACS (Atmospheric Chemistry Suite) y NOMAD (Nadir and Occultation for MArs Discovery) a bordo del satélite ExoMars Trace Gas Orbiter\, que opera alrededor de Marte desde marzo de 2018. \nEstos espectrómetros infrarrojos\, mediante observaciones de ocultaciones solares\, están permitiendo monitorizar con una sensibilidad sin precedentes la composición química de la atmósfera marciana. Algunos de los descubrimientos más relevantes de esta misión incluyen la detección de especies cloradas\, el estudio del efecto de las tormentas de polvo en el escape atmosférico y la caracterización de la composición isotópica de la atmósfera. \nDurante la reunión se han discutido los últimos avances científicos obtenidos a partir de los datos de estos instrumentos\, así como el desarrollo de modelos climáticos para interpretar las observaciones. Además\, se han definido los objetivos y las operaciones previstas para los próximos meses con el fin de maximizar el retorno científico de la misión. \n  URL:https://www.iaa.csic.es/evento/acs-nomad-swt-meeting/ LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/04/Schiaparelli_separating_from_Trace_Gas_Orbiter_pillars.jpg END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20260418 DTEND;VALUE=DATE:20260504 DTSTAMP:20260420T080043Z CREATED:20260417T101048Z LAST-MODIFIED:20260420T080043Z UID:31070-1776470400-1777852799@www.iaa.csic.es SUMMARY:Exposición ‘La ciencia de Mortadelo y Filemón’ DESCRIPTION:Francisco Ibáñez (1936-2023) fue\, a su modo\, un gran aliado de la ciencia. El creador de los inolvidables Mortadelo y Filemón combinó en sus historietas el humor y la investigación científica con un ingenio mordaz\, mostrando la ciencia como un fenómeno cotidiano\, torpe\, exagerado y\, a veces\, absurdo. Pero siempre humano. A través de una selección de 39 portadas protagonizadas por estos míticos personajes\, el Consejo Superior de Investigaciones Científicas (CSIC) ha querido rendir homenaje a Ibáñez y a la comunidad científica a través de la exposición La ciencia de Mortadelo y Filemón. Crónicas disparatadas de la investigación en España. La muestra\, que ha sido producida por la Vicepresidencia de Cultura Científica y Ciencia Ciudadana del CSIC y cuenta con la colaboración de Penguin Random House Grupo Editorial\, se ha inaugurado este viernes 17 de abril en el patio del Ayuntamiento de Granada con la presencia de diversas autoridades. La exposición\, que se enmarca como una de las actividades estrella del Desgranando Fest –festival de ciencia en la provincia de Granada– y coincide con la Feria del Libro de Granada\, – donde el CSIC instala el Área de Ciencia–\, permanecerá en esta sede hasta el 3 de mayo de 2026. \nTres expertos del CSIC han colaborado en La ciencia de Mortadelo y Filemón: Fernando del Blanco\, del Centro de Investigación y Desarrollo (CID-CSIC)\, y Jon Arrizabalaga y Alfons Zarzoso\, de la Institución Mila y Fontanals (IMF-CSIC). \nLa muestra se estrenó en el Museo Casa de la Ciencia de Sevilla\, del CSIC\, el pasado 28 de noviembre de 2025\, con la presencia de varias autoridades y la hija del autor. Granada es la segunda sede\, tras Bruselas\, de una itinerancia que durará dos años. Tras su paso por Granada recorrerá otras ciudades españolas\, entre ellas Oviedo y Zaragoza. \n  \nObjetivo eliminar al “Rana” (1993) \n  \nUna exposición\, cinco secciones \nLa ciencia de Mortadelo y Filemón propone un recorrido visual y temático a través de portadas publicadas entre 1975 y 2018 que se dividen en cinco secciones. La primera es Un mundo en movimiento bajo la lupa de la ciencia\, un repaso por portadas en las que Ibáñez emplea su peculiar humor para explorar y retratar la relación entre ciencia\, naturaleza y sociedad\, con referencias que van desde el deshielo de glaciares hasta las epidemias\, pasando por los últimos descubrimientos en producción agrícola. \nEn Innovaciones tecnológicas incorporadas por la T.I.A. se recogen algunos de los inventos desarrollados o utilizados por esta agencia de espionaje\, que en no pocas ocasiones llevaban al caos. Pero la sátira del dibujante recuerda que la innovación solo tiene sentido si resuelve un problema real. Por su parte\, el Profesor Bacterio encarna lo mejor y lo peor del arquetipo del científico loco. \nLa sección El laboratorio de Bacterio\, aciertos y accidentes caricaturiza\, a través del humor\, los límites de la ciencia y recuerda los riesgos de separarla del sentido común porque\, cuando se trata de hacer investigación\, la ética y la seguridad no son opcionales. \nEn La ciencia en el espejo social de Mortadelo y Filemón los personajes son testigos de cómo la ciencia se negocia\, se distorsiona y\, a veces\, se malinterpreta. De ahí la importancia de difundir las investigaciones e innovaciones con rigor\, evidencia y responsabilidad. En las portadas seleccionadas hay sitio para la pseudociencia\, la vida en la prehistoria o la que existe más allá de nuestra galaxia. \nCierra la muestra la sección Ciencia de emergencia para tiempos revueltos. Ibáñez quiso arrancar una carcajada en medio del desastre. El cambio climático\, la contaminación\, los mosquitos invasores o las nubes de polvo sahariano son algunas de las amenazas a las que se enfrentan Mortadelo y Filemón con más o menos éxito en el último tramo de la exposición. \n  \nNuestro antepasado\, el mico (2010) \n  \nWeb\, catálogo e itinerancia \nUna web\, lacienciademortadeloyfilemon.csic.es\, amplía los contenidos de la exposición. En cada sección el visitante puede conocer a través de códigos QR las investigaciones reales desarrolladas por el CSIC en las áreas científicas que reflejan las portadas de Ibañez\, y relacionar así el imaginario humorístico del autor con la ciencia puntera que se desarrolla en la primera institución pública de investigación de España. \nAdemás\, la muestra va acompañada de un catálogo que recoge todas las portadas y los textos de la exposición. La ciencia de Mortadelo y Filemón itinerará durante 2026 y 2027 por las delegaciones y centros de divulgación del CSIC en toda España\, así como por otros museos de ciencia. \n  \nEl coche eléctrico (2013) \n  \nUn estilo propio \nFrancisco Ibáñez fue un prolífico autor que trabajó durante décadas en la editorial Bruguera. Allí creó numerosos personajes\, pero fue con Mortadelo y Filemón\, nacidos en enero de 1958\, con quienes alcanzó un éxito masivo. Su estilo se caracterizó por el humor visual\, los juegos de palabras\, la crítica social y una capacidad inigualable para reflejar la actualidad a través de la sátira. \nLas aventuras de sus famosos personajes (marcadas por el caos del profesor Bacterio y los inventos imposibles de la T.I.A.) se hacen eco de asuntos científicos del momento: las consecuencias ambientales de nuestra huella en el planeta\, los primeros trasplantes de órganos\, las propagaciones de enfermedades\, la ingeniería genética\, la deforestación e incluso los avances en el estudio de la evolución humana. \n  \nMortadelo y Filemón\, creados por Francisco Ibáñez\, protagonizan la nueva exposición del CSIC. \n  \nLa presentación de la exposición en Granada\, en fotos \n \n  \n  URL:https://www.iaa.csic.es/evento/exposicion-la-ciencia-de-mortadelo-y-filemon/ LOCATION:Ayuntamiento de Granada\, Plaza del Carmen\, 3\, Centro\, Granada\, Granada\, 18009\, Spain CATEGORIES:Actividades ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/04/Mortadelo-y-Filemon-creados-por-Francisco-Ibanez-protagonizan-la-nueva-exposicion-del-CSIC.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=Europe/Paris:20260416T123000 DTEND;TZID=Europe/Paris:20260416T133000 DTSTAMP:20260306T124941Z CREATED:20260306T124703Z LAST-MODIFIED:20260306T124941Z UID:30209-1776342600-1776346200@www.iaa.csic.es SUMMARY:SO Colloquium - Bursting and cool slowly rotating stellar zombies DESCRIPTION:The large efforts put into studying the transient Universe in the past years allowed the discovery of a variety of new astrophysical classes and events\, many of them proposed to be related to the formation of a neutron star or a magnetar\, the most magnetic pulsars. Pulsars are unique astronomical laboratories where the most extreme gravity and electromagnetism can be probed. The study of these objects transcends the traditional astrophysical approach and requires a multidisciplinary effort that spans from particle and nuclear physics to astrophysics\, from experiment to theory\, from gravitational waves to the electromagnetic spectrum. \nI will review in this seminar what pulsars and magnetars are\, their observational characteristics\, their expected population\, as well as their connection with the most extreme extra Galactic events such as Gamma-Ray Bursts and Fast Radio Bursts. \nFecha y lugar: 0/04/2026 – 12:30 | Salón de ActosNanda ReaICE-CSIC \n  \n  URL:https://www.iaa.csic.es/evento/so-colloquium-bursting-and-cool-slowly-rotating-stellar-zombies/ 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 END:VCALENDAR