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X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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BEGIN:VEVENT
DTSTART;VALUE=DATE:20251104
DTEND;VALUE=DATE:20251106
DTSTAMP:20260407T101812
CREATED:20250822T070829Z
LAST-MODIFIED:20250822T095558Z
UID:26910-1762214400-1762387199@www.iaa.csic.es
SUMMARY:Photonic E-MARCOT: Un nuevo concepto de telescopio de gran apertura. Diseño\, casos científicos e impacto
DESCRIPTION:Photonic E-MARCOT es un nuevo concepto de telescopio astronómico de gran apertura\, escalable y modular\, basado en la combinación de múltiples unidades ópticas comerciales (OTAs\, del inglés Optical Tube Assemblies) mediante linternas fotónicas. El modo operativo combinado de estas OTAS puede lograr el equivalente a un telescopio monolítico de mayor apertura con un coste estimado diez veces inferior al de infraestructuras similares existentes o futuras. \nLa clave de este innovador concepto radica en la integración de tecnología fotónica de última generación\, lo que permite una capacidad sin precedentes para la combinación óptica y la recolección de luz. En particular\, Photonic E-MARCOT utilizará tecnología fotónica para recoger la luz de cada unidad comercial a través de una fibra y combinarla ópticamente mediante una avanzada linterna fotónica multimodo (MM-PL\, del inglés Multi-Mode Photonic Lantern)\, la cual no ha sido aplicada previamente en contextos astronómicos. Este enfoque permitirá acoplar Photonic E-MARCOT con espectrógrafos de alta resolución ya existentes\, como instrumentos similares a CARMENES. \nActualmente\, el proyecto ha desarrollado el prototipo MARCOT-Pathfinder\, que consta de 7 OTAs de 0.40 metros\, equivalentes a una apertura efectiva de 1\,1 metros. La innovación clave reside en el uso de una linterna fotónica multimodo 7-a-1 (MM-PL) para combinar la luz proveniente de estas OTAs. Este telescopio\, equipado con un modo espectroscópico basado en MM-PL\, actuará como demostrador del concepto\, constituyendo el objetivo principal de la Fase 1 del proyecto Photonic E-MARCOT. La Fase 2 ampliará esta base\, apuntando hacia una apertura efectiva de 5 metros. El objetivo final\, en la Fase 3\, es construir un telescopio con una apertura equivalente de 15 metros. Para ello\, ya se ha asegurado financiación mediante una convocatoria de Equipamiento de la Agencia Estatal de Investigación (AEI) para desarrollar el primer módulo espectroscópico basado en tecnología MM-PL\, paso crítico para alcanzar estos objetivos. \nEl caso científico principal del proyecto Photonic E-MARCOT será el estudio de exoplanetas y sistemas planetarios\, ámbito en el que se espera un impacto revolucionario. Photonic E-MARCOT abrirá nuevas vías de investigación en este campo\, desde la búsqueda de planetas similares a la Tierra hasta la caracterización detallada de interiores y atmósferas planetarias. \nA diferencia de otras grandes infraestructuras\, que deben distribuir su tiempo de observación entre múltiples nichos científicos\, Photonic E-MARCOT priorizará grandes campañas de observación en este ámbito\, dedicando una parte significativa de su tiempo a esta área. Esto permitirá un impacto sin precedentes y garantizará un avance considerable en la comprensión de la formación\, evolución y habitabilidad de exoplanetas y sistemas planetarios. Aunque la investigación en exoplanetas será el motor principal de Photonic E-MARCOT\, esta instalación también reservará tiempo abierto para la comunidad científica en general. Así\, otros investigadores podrán abordar diversas áreas de interés\, tales como estudios del Sistema Solar\, investigaciones espectroscópicas de galaxias con alto corrimiento al rojo\, entre otros. Con esta estrategia\, Photonic E-MARCOT busca maximizar su contribución en una amplia variedad de áreas de investigación astronómica. \nConsideramos Photonic E-MARCOT como una nueva infraestructura con claras sinergias con grandes instalaciones como el ELT\, y como un nuevo concepto innovador para la era posterior al ELT. Ante los importantes desafíos económicos\, medioambientales y de sostenibilidad que supone construir telescopios más grandes que el ELT\, Photonic E-MARCOT ofrece una vía transformadora. Su diseño modular y rentable\, junto con la integración de tecnología fotónica avanzada\, lo posiciona como un modelo pionero. Este enfoque permite un rendimiento óptico excepcional\, ofreciendo escalabilidad y versatilidad que podrían redefinir el futuro de los grandes telescopios. Por ello\, Photonic E-MARCOT tiene el potencial de liderar la próxima generación de infraestructuras astronómicas\, en la que la modularidad y la fotónica serán pilares centrales para construir observatorios sostenibles y de bajo coste. \nEsta reunión científica tiene un doble propósito. Por un lado\, sirve como reunión de lanzamiento del proyecto Photonic E-MARCOT\, reuniendo a su equipo central para discutir y coordinar los primeros pasos. Por otro lado\, constituye un foro abierto para la comunidad astronómica en general\, invitando a participar a cualquiera interesado en explorar el potencial del proyecto. En la reunión se presentará el concepto tecnológico del telescopio\, motivando a la comunidad astronómica a proponer nuevos casos científicos para desarrollar con Photonic E-MARCOT-5m y 15m\, explorando el impacto de esta infraestructura de bajo coste en el panorama global de la astronomía a medio y largo plazo. Asimismo\, se busca establecer vínculos colaborativos con grupos científicos y tecnológicos\, tanto de instituciones públicas como privadas. \nPor esta razón\, el workshop incluirá presentaciones sobre desarrollos tecnológicos innovadores y proyectos científicos relevantes para Photonic E-MARCOT\, además de la participación de empresas tecnológicas que expondrán sus experiencias y capacidades en instrumentación astronómica de vanguardia.
URL:https://www.iaa.csic.es/evento/photonic-e-marcot-un-nuevo-concepto-de-telescopio-de-gran-apertura-diseno-casos-cientificos-e-impacto/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Workshops
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/08/e-marcot.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251104T123000
DTEND;TZID=Europe/Paris:20251104T133000
DTSTAMP:20260407T101812
CREATED:20250912T084701Z
LAST-MODIFIED:20251015T105331Z
UID:27172-1762259400-1762263000@www.iaa.csic.es
SUMMARY:The role of groups in galaxy evolution: the importance of the pre-processing effect
DESCRIPTION:We present clear and direct evidence of the pre-processing effect of group galaxies falling into clusters in the local Universe (z ≲ 0.1). We start with a sample of 238 clusters\, from which we select 153 with N200 ≥ 20. We considered 1641 groups within the turnaround radius (~ 5 × R200) of these 153 clusters. \nThere are 6654 individual cluster galaxies and 4133 group galaxies within this radius. We considered two control samples of galaxies\, in isolated groups and in the field. The former comprises 2601 galaxies within 1606 isolated groups\, and the latter has 4273 field objects. The fraction of star-forming galaxies in infalling groups has a distinct clustercentric behaviour in comparison to the remaining cluster galaxies. Even at 5 × R200 the group galaxies already show a reduced fraction of star-forming objects. At this radius\, the results for the individual cluster galaxies are actually compatible with the field. That is strong evidence that the group environment is effective to quench the star formation prior to the cluster arrival. The group star-forming fraction remains roughly constant inwards\, decreasing significantly only within the cluster R200 radius. \nWe have also found that the pre-processing effect depends on the group mass (indicated by the number of members). The effect is larger for more massive groups. However\, it is significant even for pairs and triplets. \nFecha y lugar: 04/11/2025 – 12:30 | Sala de JuntasPaulo Afranio LopesObservatorio do Valongo\, Rio de Janeiro\, Brasil \n 
URL:https://www.iaa.csic.es/evento/the-role-of-groups-in-galaxy-evolution-the-importance-of-the-pre-processing-effect/
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:20251106T123000
DTEND;TZID=Europe/Paris:20251106T133000
DTSTAMP:20260407T101812
CREATED:20250912T085203Z
LAST-MODIFIED:20251104T144003Z
UID:27191-1762432200-1762435800@www.iaa.csic.es
SUMMARY:Mars Atmospheric Isotopes: Insights into Past and Present Fractionation
DESCRIPTION:Present-day Mars is inhospitable for life and cannot sustain liquid water on its surface. Yet\, multiple lines of evidence suggest that in the past\, different climatic conditions allowed liquid water to shape the surface and form minerals we observe today. Isotopic ratios in atmospheric species provide clues that changes in Mars’ climate may have been driven by atmospheric escape. Understanding the planet’s escape history\, however\, requires careful assessment of how heavy and light isotopes are lost to space. \nSince March 2018\, the ExoMars Trace Gas Orbiter has performed high-resolution solar occultation measurements\, enabling\, for the first time\, detailed investigations of the vertical distribution of carbon\, oxygen\, and hydrogen isotopes in the Martian atmosphere. In this seminar\, I will present key results from these studies\, highlighting the atmospheric processes that impact isotope transport to the upper atmosphere and their eventual escape to space. \nFecha y lugar: 06/11/2025 – 12:30 | Salón de ActosJuan AldayInstituto de Astrofísica de Andalucía (IAA-CSIC) \n 
URL:https://www.iaa.csic.es/evento/mars-atmospheric-isotopes-insights-into-past-and-present-fractionation/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20251111
DTEND;VALUE=DATE:20251113
DTSTAMP:20260407T101813
CREATED:20250819T082438Z
LAST-MODIFIED:20250912T080449Z
UID:26904-1762819200-1762991999@www.iaa.csic.es
SUMMARY:XXV Spanish Virtual Observatory School
DESCRIPTION:The Spanish Virtual Observatory (SVO)\, in collaboration with the Instituto de Astrofísica de Andalucía\, is organizing a VO School. The school will take place at IAA premises on November 11–12\, 2025. \nPurpose of the School\nThe main goal of the school is to introduce participants to the capabilities of the Virtual Observatory for accessing and analyzing data from astronomical archives. \nParticipants will become familiar with key Virtual Observatory tools by working through tutorials based on real scientific cases. Expert tutors from the Spanish Virtual Observatory will provide guidance throughout the school. \nThe school will be conducted entirely in English. \n 
URL:https://www.iaa.csic.es/evento/xxv-spanish-virtual-observatory-school/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/08/svo.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251111T123000
DTEND;TZID=Europe/Paris:20251111T133000
DTSTAMP:20260407T101813
CREATED:20250930T090018Z
LAST-MODIFIED:20251103T085232Z
UID:27502-1762864200-1762867800@www.iaa.csic.es
SUMMARY:Extreme gamma-ray pulsars (and what CTAO can say about them)
DESCRIPTION:At the dawn of the century only a handful of pulsars had been found to pulse in gamma-rays\, and certainly none was supposed to emit beyond the GeV scale. \nOver the past two decades\, thanks to the Fermi-LAT\, the situation has dramatically changed: we now know more than 300 such objects\, and the number keeps increasing. Behaving as lepton factories and natural particle accelerators\, the physics of gamma-ray pulsars still lacks a complete\, coherent description. As was first realized in early MAGIC observations of the Crab\, some of these objects elude the strong spectral cutoff imposed by their own gargantuan magnetic field and find a way to emit well beyond the tens of GeV\, into (and beyond!) the TeV scale. This makes these «extreme» pulsars targets for imaging atmospheric Cherenkov telescopes and has prompted a progressive «migration» of the emission scenarios farther away from the neutron star. \nIn this talk I will briefly introduce some basic concepts of pulsar physics\, review current results and discuss present hot topics. Finally\, I will also show how the upcoming CTAO has the potential to spark a second-revolution in gamma pulsars\, its consequences stretching even beyond the usual boundary of astrophysics. \nFecha y lugar: 11/11/2025 – 12:30 | Sala de JuntasGiovanni CeribellaMax Planck for Physics (MPP) \n 
URL:https://www.iaa.csic.es/evento/extreme-gamma-ray-pulsars-and-what-ctao-can-say-about-them/
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:20251113T123000
DTEND;TZID=Europe/Paris:20251113T133000
DTSTAMP:20260407T101813
CREATED:20251001T085011Z
LAST-MODIFIED:20251110T101049Z
UID:27526-1763037000-1763040600@www.iaa.csic.es
SUMMARY:A SITELLE overview of interacting galaxies and supernova remnants
DESCRIPTION:The purpose of this talk\, separated into three « chapters »\, is to present an overview of the capabilities of SITELLE\, a wide-field imaging Fourier transform spectrometer built by our team and attached to the Canada-France-Hawaii telescope. \nAfter a brief technical introduction to this instrument\, I will summarize the collaborative work started a few years ago between IAA\, Universidad de Granada and Université Laval on interacting galaxies (which is the main reason for my two-months sabbatical stay in Granada): Arp82\, Arp 143 and\, more recently\, a sample of Hickson compact groups (a project led by Salvador Duarte Puertas\, from UGR). The last chapter is dedicated to an ongoing work on supernova remnants\, both in the Milky Way (the Crab Nebula and Cassiopeia A)\, and then in nearby galaxies\, using data obtained as part of the SIGNALS survey. \nFecha y lugar: 13/11/2025 – 12:30 | Salón de ActosProf. Laurent DrissenUniversité Laval\, Québec \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/a-sitelle-overview-of-interacting-galaxies-and-supernova-remnants/
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:20251117T080000
DTEND;TZID=Europe/Paris:20251121T170000
DTSTAMP:20260407T101813
CREATED:20251119T131419Z
LAST-MODIFIED:20251119T131422Z
UID:28826-1763366400-1763744400@www.iaa.csic.es
SUMMARY:2nd MAGIC + LST F2F Meeting
DESCRIPTION:The second MAGIC + LST F2F Meeting is a conference aimed at strengthening coordination between the MAGIC and LST collaborations. Participants reviewed the status of ongoing and future scientific projects that both collaborations share\, covering key scientific advances as well as technical challenges related to data analysis. Some of the topics discussed were: \n\nExtragalactic astronomy: A review of extragalactic targets and the scientific progress of ongoing programs.\nGalactic astronomy: Discussion of supernova remnants\, pulsars\, and a set of potential Galactic targets.\nStatus of data analysis and background modeling.\nMultimessenger astronomy: Coordinating target selection with previous neutrino and gravitational-wave observations.\nTheoretical perspectives: Including Lorentz Invariance Violation physics and axion-like particle searches.\n\nThe conference is strategically held a couple of months before the next call of observation proposals and will have a direct impact in the criteria for future data taking cycles of both telescopes.
URL:https://www.iaa.csic.es/evento/2nd-magic-lst-f2f-meeting/
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/magic-lst.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251118T130000
DTEND;TZID=Europe/Paris:20251118T143000
DTSTAMP:20260407T101813
CREATED:20250912T085346Z
LAST-MODIFIED:20251118T113748Z
UID:27194-1763470800-1763476200@www.iaa.csic.es
SUMMARY:SO Colloquium: Galactic Centres and their high-energy multimessenger Phenomena
DESCRIPTION:Galactic Nuclei are the densest stellar systems in the Universe\, and they host massive black holes (MBHs). A host of energetic and unique phenomena\, –such as tidal disruption events\, hypervelocity stars and extreme mass ratio inspirals–\, arise from these outstanding features of galactic nuclei. \nIn this talk\, | I will present my group work on state-of-the-art dynamical calculations that link the rate and properties of these different phenomena and show how they can be used to investigate MBH environments at scales hardly accessible (or not yet accessible) by direct observations. \nFecha y lugar: 18/11/2025 – 13:00 | Salón de ActosElena RossiUniversity of Leiden\, The Netherlands \n 
URL:https://www.iaa.csic.es/evento/galactic-centres-and-their-high-energy-multimessenger-phenomena/
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:20251120T130000
DTEND;TZID=Europe/Paris:20251120T143000
DTSTAMP:20260407T101813
CREATED:20251020T133324Z
LAST-MODIFIED:20251118T113833Z
UID:27805-1763643600-1763649000@www.iaa.csic.es
SUMMARY:SO Colloquium: Pre-CTAO Science with LST: Current and Expected Results
DESCRIPTION:The Large-Sized Telescope prototype (LST-1) is the first and the larger of a new generation of instruments that will form the Cherenkov Telescope Array Observatory (CTAO) in the island of La Palma (CTAO-North). CTAO is designed to explore; with unprecedented sensitivity\, angular resolution\, field of view\, and energy coverage; the Universe at very-high-energy gamma rays. Since beginning its observations\, LST-1 has been studying the northern sky in an energy range between about a few tens of GeV up to a few TeV. Thanks to its high sensitivity and its ability to quickly point toward flaring targets\, LST-1 is particularly well suited to detect and follow up on rapidly changing cosmic sources. \nIn this seminar\, I will present the first scientific results obtained with LST-1 as well as the expectations for the full LST northern array (involving an total of 4 LST telescopes in La Palma\, that will become the most sensitive instrument of its class along 2026) regarding new discoveries in the very-high-energy gamma-ray sky. \nFecha y lugar: 20/11/2025 – 13:00 | Salón de ActosProf. Pol BordasIEEC – ICC – Universitat de Barcelona \n 
URL:https://www.iaa.csic.es/evento/pre-ctao-science-with-lst-current-and-expected-results/
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:20251125T123000
DTEND;TZID=Europe/Paris:20251125T133000
DTSTAMP:20260407T101813
CREATED:20250930T090140Z
LAST-MODIFIED:20251118T113754Z
UID:27506-1764073800-1764077400@www.iaa.csic.es
SUMMARY:SO Colloquium: The future science of CTAO
DESCRIPTION:In this talk\, I will review the plans for construction\, and the current status of the Cherenkov Telescope Array Observatory\, CTAO\, as well as the current plans for its scientific exploitation through the Key Science Program as described in the latest CTA Science Book. Moreover\, I will also present the opportunities that the future CTAO imply for the entire scientific community in general. \nFecha y lugar: 25/11/2025 – 12:30 | Sala de JuntasGiacomo BonnoliINAF – Istituto Nazionale di Astrofisica\, Osservatorio Astronomico di Brera – Sede di Merate \n 
URL:https://www.iaa.csic.es/evento/the-future-science-of-ctao/
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:20251127T123000
DTEND;TZID=Europe/Paris:20251127T133000
DTSTAMP:20260407T101814
CREATED:20250912T085614Z
LAST-MODIFIED:20251127T111959Z
UID:27198-1764246600-1764250200@www.iaa.csic.es
SUMMARY:First Glimpses of the Extragalactic Gamma-ray Sky with LST-1: Paving the Way to CTAO
DESCRIPTION:The gamma-ray extragalactic sky is dominated by blazars\, radio-loud active galactic nuclei (AGN) with relativistic jets that are closely aligned with our line of sight. In the MeV range\, the Fermi-LAT satellite has led the efforts in studying this violent type of sources\, with more than 3000 known blazars discovered so far in the MeV range. In the GeV-TeV range\, the Cherenkov experiments MAGIC\, HESS and VERITAS have made significant advances in the field. However\, their sensitivity has only allowed us to discover ~300 sources in the most extreme Universe after two decades of operations\, with only ~90 being AGN and blazars. \nThe Cherenkov Telescope Array Observatory (CTAO) stems as the future of ground-based gamma-ray astronomy. Its improved capabilities promise to revolutionize the field in the near future. Its first telescope\, the Large-Sized Telescope prototype (LST-1)\, is already operating in La Palma (Spain) since 2018\, therefore being not only the future but also the present in the field. In this talk I will give an overview of some of the first scientific results on AGN and blazars obtained during LST-1’s first years of operation. The seminar will conclude with a discussion of future perspectives with the fully operating CTAO. \nFecha y lugar: 27/11/2025 – 12:30 | Salón de ActosJorge Otero-SantosINFN Sezione di Padova \n 
URL:https://www.iaa.csic.es/evento/first-glimpses-of-the-extragalactic-gamma-ray-sky-with-lst-1-paving-the-way-to-ctao/
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:20251127T190000
DTEND;TZID=Europe/Paris:20251127T200000
DTSTAMP:20260407T101814
CREATED:20251111T101816Z
LAST-MODIFIED:20251111T101944Z
UID:28731-1764270000-1764273600@www.iaa.csic.es
SUMMARY:Mirar los cielos: el misterio de la Luna
DESCRIPTION:Desde hace milenios nuestra interpretación del universo ha estado moldeada por la superstición\, las creencias religiosas\, los intereses políticos\, económicos y sociales\, la filosofía y la ciencia. La investigación astronómica actual es herencia de ese crisol de maneras de pensar. En este sentido\, la luna ha jugado un papel protagonista. Por su cercanía\, su estudio sirvió para definir y cuestionar los principios de la naturaleza y del propio universo. \nEn esta conferencia veremos cómo sus múltiples facetas inspiraron algunas de las preguntas más profundas que nos hemos hecho relacionadas con la esencia misma del cosmos\, el lugar que el ser humano ocupa en él y hasta la existencia de vida extraterrestre. Veremos también cómo el arte dejó constancia de todo ello. \nEsta conferencia se hace dentro de una colaboración con el Ateneo de Granada. \nFecha:27/11/2025 – 19:00Conferenciante:  Monserrat Villar MartínFiliación: Centro de Astrobiología (INTA-CSIC) \n 
URL:https://www.iaa.csic.es/evento/mirar-los-cielos-el-misterio-de-la-luna/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
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END:VEVENT
END:VCALENDAR