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DTSTART;TZID=Europe/Paris:20250306T123000
DTEND;TZID=Europe/Paris:20250306T133000
DTSTAMP:20260416T145726
CREATED:20250224T113433Z
LAST-MODIFIED:20250912T080200Z
UID:25105-1741264200-1741267800@www.iaa.csic.es
SUMMARY:SO Colloquium: Gravitational wave astrometry with the SKAO
DESCRIPTION:Pulsar timing array detection of a gravitational wave background represents a milestone in the field of gravitational wave astronomy. However\, the origin of such a signal is still a matter of intense debate: while supermassive black hole binaries formed as a result of galaxy mergers represent the most obvious candidate for the gravitational wave signal\, many «new Physics» models can potentially explain at least part of the detected background. In this colloquium I will review the current observational and theoretical status of the field\, addressing current issues and future challenges\, Moreover\, I will discuss how radio observations with the SKAO can contribute to this broader context\, and\, in particular\, I will focus on a possible background detection strategy that involves both pulsar timing array and gravitational wave astrometry. \nFecha: 06/03/2025 – 12:30Conferenciante: Dr. Nicola BellomoFiliación: Dipartimento di Fisica “Galileo Galilei”\, Universitá degli Studi di Padova\, Italy \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-gravitational-wave-astrometry-with-the-skao/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250227T190000
DTEND;TZID=Europe/Paris:20250227T200000
DTSTAMP:20260416T145726
CREATED:20250219T095932Z
LAST-MODIFIED:20250219T100037Z
UID:25062-1740682800-1740686400@www.iaa.csic.es
SUMMARY:Ceres como laboratorio natural. Claves orgánicas desde el cinturón de asteroides
DESCRIPTION:En 2017\, la sonda Dawn reveló la presencia de material orgánico en la superficie de Ceres\, un hallazgo que marcó un hito en la exploración del planeta enano más cercano a la Tierra. \nEstudios recientes han identificado nuevas regiones con indicios de compuestos orgánicos adicionales\, ampliando nuestra comprensión de este fascinante mundo. \nDurante la charla\, exploraremos qué hace de Ceres un objeto tan relevante\, profundizando en los hallazgos orgánicos\, su posible importancia para la astrobiología y las perspectivas futuras en su estudio. \nFecha: 27/02/2025 – 19:00Conferenciante: Juan Luis RizosFiliación: Instituto de Astrofísica de Andalucía (IAA-CSIC) \n 
URL:https://www.iaa.csic.es/evento/ceres-como-laboratorio-natural-claves-organicas-desde-el-cinturon-de-asteroides/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250226T123000
DTEND;TZID=Europe/Paris:20250226T133000
DTSTAMP:20260416T145727
CREATED:20250130T075125Z
LAST-MODIFIED:20250130T075128Z
UID:24834-1740573000-1740576600@www.iaa.csic.es
SUMMARY:ORCA-TWIN: Fast & low read noise CMOS camera project for planetary science and astrophysics
DESCRIPTION:The emerging German Center for Astrophyics (DZA) aspires – next to activities for gravitational wave astronomy\, radio astronomy\, and big data – to engage in CMOS sensor development with the local semiconductor industry and international partners. In parallel to establishing a first detector lab that has become operational recently\, two off-the-shelf CMOS cameras were procured to explore hands-on the capabilities for time domain astronomy and solar system research with sub-second time resolution. The cameras are specified to deliver frame rates of up to 125 fpm with read noise below 0.4 e – .The talk will present science cases for a pilot study\, dubbed ORCA-TWIN\, that involves two 1m-class-telescopes on a ~1.500 km baseline (CAHA/Tenerife) to enable direct triangulation of solar system bodies and other objects\, such as space debris and NEOs\, next to other high time resolution applications\, e.g. AGN variability\, M star flares\, exoplanet transits\, etc. The capabilities of the configuration as well as challenges concerning data acquisition\, online data processing\, and synchronization will be discussed. \nFecha: 26/02/2025 – 12:30Conferenciante: Dr. Martin M. RothFiliación: Deutsches Zentrum für Astrophysik (DZA)\, Görlitz Leibniz-Institut für Astrophysik Potsdam (AIP) Universität Potsdam \n 
URL:https://www.iaa.csic.es/evento/orca-twin-fast-low-read-noise-cmos-camera-project-for-planetary-science-and-astrophysics/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250225T123000
DTEND;TZID=Europe/Paris:20250225T133000
DTSTAMP:20260416T145727
CREATED:20250127T091206Z
LAST-MODIFIED:20250127T091208Z
UID:24372-1740486600-1740490200@www.iaa.csic.es
SUMMARY:Chemical Fingerprints of Galaxy Evolution
DESCRIPTION:I will summarise the main projects we are currently working on that use the chemical abundances and pattern as fossil records of galaxy evolution. \nIn particular\, the chemical abundances of the star-forming regions of galaxies contain valuable information about their assembly histories\, as well as about the processes that regulate the history of star formation and the mixing of chemical elements. In particular\, they encode the history of recent mergers and strong gas inflows\, as well as the impact of SN and AGN feedback that could trigger these events. This project was carried out using simulated galaxies from the CIELO and EAGLE projects. I will focus on the studying the impact on the metallicity gradients in the discs and the mass-metallicity relation. \nFecha: 25/02/2025 – 12:30Conferenciante: Dra. Patricia B. TisseraFiliación: Pontificia Universidad Católica de Chile\, Chile \n 
URL:https://www.iaa.csic.es/evento/chemical-fingerprints-of-galaxy-evolution/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250214T180000
DTEND;TZID=Europe/Paris:20250214T200000
DTSTAMP:20260416T145727
CREATED:20250210T150359Z
LAST-MODIFIED:20250210T150401Z
UID:25006-1739556000-1739563200@www.iaa.csic.es
SUMMARY:Mitología e inteligencia artificial\, ejes centrales de la séptima edición del festival multidisciplinar Gravite
DESCRIPTION:El Instituto de Astrofísica de Andalucía (IAA-CSIC) participa\, junto a otras instituciones\, en Gravite 7\, acogiendo la proyección del cortometraje ‘Estela’ y la posterior entrega del premio Viajero en el Tiempo. El evento tendrá lugar en su salón de actos el próximo 14 de febrero a las 18:00 horas. \nEl festival\, patrocinado por CaixaBank\, contará con la presencia de personalidades destacadas del mundo del cine y la ciencia\, como Rosa Montero\, Jorge Volpi\, Margarita Sánchez\, Manuel Sicilia\, Emilio García o Alicia Pelegrina\, entre otras. \nEsta mañana se han presentado en el cementerio de Granada las actividades que se desarrollarán en el marco de la séptima edición del festival multidisciplinar Gravite\, patrocinado por CaixaBank. La jornada ha comenzado en el propio camposanto con un encuentro con el escritor y gestor cultural Alfonso Salazar\, en torno a su libro Los géneros del dolor y el abandono\, publicado por la Editorial Sonámbulos. En esta obra\, Salazar aborda la evolución del tango\, el bolero y la copla a través de las letras de las canciones\, estableciendo una relación entre estos tres géneros y sus posibles conexiones con la música urbana más contemporánea. \nLa presentación de esta nueva edición de Gravite\, ha sido conducida por Juan Ramón Ferreira\, concejal de Cultura del Ayuntamiento de Granada; Javier Rivas\, director de Área de Negocio de CaixaBank en Granada; Jesús Lens y Gustavo Gómez\, director y gestor cultural del evento respectivamente. Al acto también han asistido representantes de las entidades colaboradoras: Instituto de Astrofísica de Andalucía\, Emucesa\, Fundación CajaGranada\, Consorcio IFMIF-DONES España\, Universidad de Granada\, Parque de las Ciencias y Librerías Picasso. \n \n  \nINTELIGENCIA ARTIFICIAL \nDentro del ciclo de cine sobre inteligencia artificial y robots\, organizado por Gravite y el Cine Club Universitario\, el próximo martes 11 de febrero estará dedicado a esa tecnología que lo está cambiando todo. \nPor la mañana\, a las 11:45\, y con motivo del Día Internacional de la Mujer y la Niña en la Ciencia\, el Parque de las Ciencias y el Festival Gravite han organizado un encuentro con científicas que será retransmitido en directo para alumnado a partir del tercer ciclo de educación primaria de toda Andalucía. Durante el coloquio\, intervendrán tres mujeres con diferentes trayectorias profesionales para compartir su historia personal y profesional desde una perspectiva de igualdad e integración entre ciencias y humanidades. A través de sus experiencias\, el encuentro busca generar referentes femeninos en la ciencia y fomentar el interés por la tecnología y la literatura desde la empatía y la pasión. \nLas participantes serán Ana Guijarro Román\, astrónoma en el Centro Astronómico Hispano en Andalucía (CAHA)\, y María Ángeles Martín Prats\, profesora titular del Departamento de Ingeniería Electrónica y directora de la línea de investigación aeronáutica de Aviónica en la Universidad de Sevilla. Además\, la literatura servirá como vehículo para el desarrollo del coloquio con la participación especial de la escritora y periodista Rosa Montero Gayo. La actividad estará moderada por Lourdes López Pérez\, jefa de Sección de I+D+I en Comunicación Social de la Ciencia del Parque de las Ciencias. \nPor la tarde\, a partir de las 17:00\, en Librería Picasso\, la jornada comenzará con un club de lectura sobre ‘En un abrir y cerrar de ojos’\, de la escritora Jo Callaghan\, una novela que explora la introducción de una inteligencia artificial en el trabajo de campo de la Policía. \nA continuación\, Quico Chirino\, director de IDEAL\, conversará con Francisco Herrera\, catedrático de IA de la UGR\, sobre el impacto de la inteligencia artificial y los algoritmos en los medios de comunicación. Para cerrar la jornada\, Rosa Montero presentará su novela más reciente\, Animales difíciles\, protagonizada por Bruna Husky\, una replicante en un futuro distópico. \nMITOS Y LEYENDAS \nLa arquitecta y guía turística Blanca Espigares Rooney ha diseñado una ruta para desmontar algunos mitos y leyendas que suelen escucharse en las visitas a los lugares más emblemáticos de Granada. \nPor su parte\, la Banda Municipal de Música de Granada\, galardonada con el Memorial Fernando Marías de Gravite 2025\, ofrecerá un concierto titulado Mitos y leyendas en el Teatro CajaGranada. La cita será el miércoles 12 de febrero a las 19:00\, con entrada libre para el público. \nEl viernes 14 de febrero\, el Instituto de Astrofísica de Andalucía (IAA-CSIC) acogerá la proyección del cortometraje Estela\, dirigido por Manuel Sicilia\, reciente ganador de un Premio Carmen. Este trabajo\, realizado en colaboración con el propio IAA-CSIC y IFMIF-DONES\, dará pie a un coloquio en el que se explorarán los vínculos entre cine\, astrofísica e ingeniería. Además\, en el marco de esta jornada\, se entregará el Premio Viajero en el Tiempo al escritor mexicano Jorge Volpi. \nEl sábado 15 de febrero por la tarde\, la catedrática de la UGR y arqueóloga Margarita Sánchez Romero presentará su libro (Pre)historias. Cuentos de mujeres que forjaron el mundo\, publicado por la editorial Destino. Por su parte\, el escritor José Luis Ordóñez hablará sobre su obra El universo de Indiana Jones\, publicada por Notorius Ediciones\, en la que rinde homenaje a uno de los grandes mitos del cine\, encarnado por Harrison Ford a lo largo de cinco películas que abarcan más de 40 años\, todo un viaje en el tiempo. \nEse mismo día\, Gravite ha organizado una visita guiada a la exposición Granada y el romanticismo: los viajes en el siglo XIX\, en el Cuarto Real de Santo Domingo\, así como un recorrido por el Carmen de la Victoria de la UGR y la histórica fábrica de cerámica Fajalauza. \n \nSOBRE GRAVITE \nGravite es un festival multidisciplinar de carácter popular que reivindica esa tercera cultura que fusiona ciencias con artes y letras. Con el viaje en el tiempo como protagonista\, Gravite se puso en marcha en 2018 por Gustavo Gómez y Jesús Lens. Cuenta con el patrocinio de CaixaBank y la colaboración del Ayuntamiento de Granada\, Universidad de Granada-CineClub Universitario UGR\, Emucesa\, Instituto de Astrofísica de Andalucía-CSIC\, Parque de las Ciencias\, CajaGranada Fundación\, Consorcio IFMIF-DONES España y Librerías Picasso. \nUn festival cuyo programa está abierto a todas las ciencias\, las artes y las letras\, defensor de la tercera cultura que permite maridar las disciplinas más diferentes\, posibilitando el contacto y la relación directa entre científicos\, autores\, creadores\, público y aficionados. \n 
URL:https://www.iaa.csic.es/evento/mitologia-e-inteligencia-artificial-ejes-centrales-de-la-septima-edicion-del-festival-multidisciplinar-gravite/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Actividades
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250213T123000
DTEND;TZID=Europe/Paris:20250213T133000
DTSTAMP:20260416T145727
CREATED:20250127T090933Z
LAST-MODIFIED:20250912T080204Z
UID:24366-1739449800-1739453400@www.iaa.csic.es
SUMMARY:SO Colloquium: Present and future of exoplanet research
DESCRIPTION:The search for new worlds in the Galaxy in the past three decades has been highly successful and the prospects for the next decade are even brighter. A succession of space missions and ground-based facilities defines a timeline extending well into the 2030s. Many advances on the planet discovery front will come from the PLATO mission\, which will find long-period planets and even true Earth analogues\, and from the many ongoing and future precise radial velocity instruments from the ground\, such as CARMENES and ESPRESSO. A major leap forward is expected regarding exoplanet detailed characterisation. The goal is to understand the nature of the exoplanetary bodies and their formation and evolutionary histories through remote sensing of their atmospheres. JWST is measuring a select sample of key transiting exoplanets while Ariel will take this methodology to the next level by analysing over 1000 planets. And in the farther future\, extremely large telescopes or interferometers\, both on the ground and in space\, should permit the measurement of temperate rocky planet atmospheres and\, perhaps\, the solid identification of molecules of biological interest\, which will truly be a revolutionary finding. In this talk\, the state of the art of exoplanet research will be described and the main future exoplanet facilities will be presented and put in context. \nFecha: 13/02/2025 – 12:30Conferenciante: Dr. Ignasi RibasFiliación: ICE – CSIC \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-present-and-future-of-exoplanet-research/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250211T123000
DTEND;TZID=Europe/Paris:20250211T133000
DTSTAMP:20260416T145727
CREATED:20250206T081806Z
LAST-MODIFIED:20250206T081824Z
UID:24977-1739277000-1739280600@www.iaa.csic.es
SUMMARY:An Unusual Triple System: CN Lyn
DESCRIPTION:Triple star systems hold significant astrophysical importance\, offering profound insights into stellar evolution\, dynamical interactions\, and mass transfer processes. Due to their complexity compared to single or binary star systems\, triple systems facilitate a more comprehensive understanding of stellar processes from formation to final stages. Thanks to large photometric surveys\, such as Kepler\, researchers were able to detect triple systems with long periods. Also\, the latest studies show that 15% of binaries have a tertiary component. Therefore\, studying such objects will lead to results that benefit every aspect of stellar astrophysics. \nIn this talk\, I will present our latest study of known but not studied in detail triple star system\, CN Lyn\, and our findings by combining spectroscopy\, photometry\, and galactic dynamic techniques. \nFecha: 11/02/2025 – 12:30Conferenciante: Dr. Gökhan YücelFiliación: Istanbul University in Turkey\, Turkey \n  \n 
URL:https://www.iaa.csic.es/evento/an-unusual-triple-system-cn-lyn-2/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250211T080000
DTEND;TZID=Europe/Paris:20250211T220000
DTSTAMP:20260416T145727
CREATED:20250128T083703Z
LAST-MODIFIED:20251204T202104Z
UID:24524-1739260800-1739311200@www.iaa.csic.es
SUMMARY:Día Internacional de la Mujer y la Niña en la Ciencia 2025
DESCRIPTION:En la actualidad\, las mujeres y niñas encuentran barreras de muchos tipos\, a veces muy sutiles\, que dificultan su presencia en la ciencia. Esta desigualdad es observable en la elección de los estudios por parte de las niñas y se va agudizando al avanzar en las carreras científicas y tecnológicas. A fin de lograr el acceso y la participación plena y equitativa en la ciencia para las mujeres y las niñas\, la igualdad de género y el empoderamiento de las mujeres y las niñas\, el 15 de diciembre de 2015 se proclamó el 11 de febrero de cada año como el Día Internacional de la Mujer y la Niña en la Ciencia por la la Asamblea General de las Naciones Unidas. \nEl Instituto de Astrofísica de Andalucía se suma un año a esta iniciativa con una serie de actividades en nuestro centro destinadas a visibilizar el trabajo de las científicas\, y a crear roles femeninos en los ámbitos de la ciencia y la ingeniería que promuevan prácticas que favorezcan la igualdad de género en el ámbito científico. \n \nPregunta a una astrónoma\nPara la actividad ‘Pregunta a una astrónoma’ estudiantes de quinto y sexto de primaria del CEIP Abencerrajes se reunirán con varias investigadoras del IAA-CSIC para hacerles preguntas de astronomía\, sus carreras\, … ¡y lo que se les vaya ocurriendo! Previamente el alumnado ha investigado sobre las ellas\, ya que les hemos dado sus biografías y han trabajado sobre ellas durante los días previos … \n\nMaría Passas Varo – Ingeniera y Doctora en Física y Ciencias del Espacio – Departamento del sistema solar\nYolanda Jiménez Teja – Investigadora postdoctoral – Departamento de astronomía extragaláctica\nJosefa Masegosa Gallego – Investigadora Científica – Departamento de astronomía extragaláctica\nSara Cazzoli – Contratada Doctor Laboral Fijo – Departamento de astronomía extragaláctica\nMaría Álvarez Santiago – Investigadora predoctoral – Departamento de radioastronomía y estructura galáctica\n\n \nMesas astronómicas\nLas «Mesas Astronómicas» consisten en encuentros de pequeños grupos de estudiantes de primero de bachillerato del IES Zaídin-Vergeles con mujeres del IAA-CSIC\, donde les pueden plantear preguntas tanto de carácter científico como sobre su trayectoria personal y profesional. \n\nTeresa Toscano Domingo – Investigadora predoctoral – Departamento de radioastronomía y estructura galáctica\nMirjana Pović – Contratada Doctor Laboral Fijo – Departamento de astronomía extragaláctica\nIsabel Bustamante Díaz – Responsable del taller de mecanizado – Unidad de Desarrollo Instrumental y Tecnológico (UDIT)\nCarolina Kehrig – Científica titular – Departamento de astronomía extragaláctica\nLaura Darriba Pol – Investigadora postdoctoral – Departamento de astronomía extragaláctica\nAmanda López Moreno – Responsable de prensa – Unidad de Cultura Científica y de la Innovación (UCC+I)\n\n \nEl objetivo de esta actividad es ayudar a despertar las vocaciones científicas y tecnológicas de alumnos y alumnas de secundaria\, mostrar modelos a seguir y romper los estereotipos de los roles de género en las ciencias y las tecnologías con el fin último de contribuir a reducir la brecha de género en estos campos. Se trata de que cada uno de los grupos de estudiantes que participan conversen durante unos 10 minutos con cada una de estas mujeres que trabajan en distintas áread del Instituto de Astrofísica de Andalucía-CSIC\, de forma rotativa\, para resaltar el papel de la mujer en la ciencia y la tecnología en el área de Astrofísica y Ciencias del Espacio. Abarca la divulgación de los temas de investigación que se llevan a cabo en el IAA-CSIC y la discusión abierta sobre los roles de género y estereotipos existentes en torno a la ciencia\, la tecnología\, la ingeniería y las matemáticas. \n¿Esa pregunta es para mí?\nCuatro intrépidas astrónomas responderán a preguntas enviadas por escolares de primaria. No sabremos que saldrá\, pero no os lo podéis perder… \n\nGabriella Gilli – Investigadora postdoctoral EMERGIA – Departamento del sistema solar\nClara Cabanillas de la Casa – Investigadora predoctoral – Departamento de astronomía extragaláctica\nMarta Puig Subirà – Investigadora predoctoral – Departamento de astronomía extragaláctica\nLaly Gallego Cano – Investigadora postdoctoral – Departamento de radioastronomía y estructura galáctica\n\n \n \n\n \n \nCAMPAÑA 11F – RED CSIC GRANADA Y AYUNTAMIENTO\nEste año\, con motivo del «Día Internacional de la Mujer y la Niña en la Ciencia» el Ayuntamiento de Granada (Servicio de Igualdad y Servicio de Educación) junto con la Red de Igualdad y Diversidad de los centros CSIC de Granada (el Instituto de Astrofísica de Andalucía\, la Estación Experimental del Zaidín\, la Escuela de Estudios Árabes\, el Instituto de Parasitología y Biomedicina López Neyra\, el Instituto Andaluz de Ciencias de la Tierra y el Centro Nacional Instituto Geológico y Minero de España) hemos querido visibilizar y dar a conocer el trabajo de 18 científicas que trabajan actualmente en estos seis centros del CSIC en Granada. \nhttps://www.granada.org/inet/wmujer8.nsf/ww07igua/8A64DFA71EE4D036C1258B… \nPara ello\, se organizan varias actuaciones: \n\nCampaña de sensibilización a la población general sobre la presencia de las mujeres en la Ciencia\n\nDel 27 de enero al 17 de febrero estarán expuestos distintos MUPIS por toda la ciudad\, presentando fragmentos de la biografía y del trabajo de estas mujeres profesionales de los 6 centros del CSIC en Granada. Estos cuentan con varios QR que se pueden seguir para conocer más a fondo su trabajo y perfiles profesionales. \nLas fichas completas de las investigadoras están disponibles en: https://cloud.iaa.es/index.php/s/WSB9zxnC7AAbaSZ \n\nEsta Campaña es la base de la III EDICIÓN CONCURSO 11-F\n\nEl alumnado de los Centros Educativos de la ciudad podrá participar en el III CONCURSO de DIBUJO\, MURAL y VÍDEO dirigido a diferentes niveles educativos\, presentando trabajos que contribuyan a visibilizar a algunas de estas 18 científicas de los centros del Consejo Superior de Investigaciones Científicas en Granada optando a recibir uno de los 6 premios que se otorgarán. \n \n \n \n \n  \n \n  \n‘Todas hacemos ciencia’: 11F 2025\nEstas actividades se engloban en la campaña ‘Todas hacemos ciencia’\, organizada por el Consejo Superior de De Investigaciones Científicas (CSIC) \n \nReferencia: Comisión de Igualdad\, Diversidad e Inclusión del IAA-CSIC – igualdad.iaa.csic.es – igualdad@iaa.es
URL:https://www.iaa.csic.es/evento/dia-internacional-de-la-mujer-y-la-nina-en-la-ciencia-2025/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Actividades
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/01/imagen_buena_.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250206T120000
DTEND;TZID=Europe/Paris:20250206T130000
DTSTAMP:20260416T145727
CREATED:20250127T090713Z
LAST-MODIFIED:20250127T090747Z
UID:24362-1738843200-1738846800@www.iaa.csic.es
SUMMARY:Equality and harrassment in the CSIC. A case of study: IAA
DESCRIPTION:In this talk I will present the equality plans in the CSIC with a critical look at the particular situation of the IAA. I will focus on the current IAA Equality plan (the first one) and the changes it needs to live in an increasingly friendly environment. Equality will have a positive impact on the quality of the science we produce. \nFecha: 06/02/2025 – 12:30Conferenciante: Dra. Josefa Masegosa GallegoFiliación: IAA – CSIC\, Granada\, España \n 
URL:https://www.iaa.csic.es/evento/equality-and-harrassment-in-the-csic-a-case-of-study-iaa/
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:20250203T093000
DTEND;TZID=Europe/Paris:20250220T230000
DTSTAMP:20260416T145727
CREATED:20250114T173241Z
LAST-MODIFIED:20250912T080528Z
UID:22674-1738575000-1740092400@www.iaa.csic.es
SUMMARY:Element Abundances and the Chemical Evolution of the Cosmos
DESCRIPTION:The course will be taught in seven sessions of 1.5 hours each. \n\n27 Jan 2025: Cosmic elemental abundances. Data sources. Stellar abundances. Nebular abundances.\n29 Jan 2025: Primordial nucleosynthesis and abundances of the light elements.\n3 Feb 2025: Outline of stellar structure and evolution.\n5 Feb 2025: Stellar nucleosynthesis and principles of galactic chemical evolution.\n10 Feb 2025: Specific models of galactic chemical evolution and comparison with availabledata.\n12 Feb 2025: The chemical evolution of external galaxies.\n17 Feb 2025: Element abundances at high redshifts and cosmic chemical evolution.\n\nThis course is taught by Professor Ángeles I. Díaz (Universidad Autónoma de Madrid)
URL:https://www.iaa.csic.es/evento/element-abundances-and-the-chemical-evolution-of-the-cosmos/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/01/shrinath-kc_bxob_a3c-unsplash.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250131T123000
DTEND;TZID=Europe/Paris:20250131T130000
DTSTAMP:20260416T145727
CREATED:20250127T084840Z
LAST-MODIFIED:20250127T084945Z
UID:24345-1738326600-1738328400@www.iaa.csic.es
SUMMARY:Resolving Stellar Angular Diameters with Asteroid Occultations
DESCRIPTION:Occultations have been used for measuring stellar angular diameters since 1936 when French astronomy M. A. Arnulf measured the radius of Regulus during a lunar occultation. Since then\, astronomers have used lunar occultations to measure the angular diameters of hundreds of bright stars m≤5. The technique of measuring an angular diameter using lunar occultations is based on the diffraction of light around the limb of the moon. With this technique\, stars down to 1 milliarcsecond could be resolved. In 2018\, the ground-based gamma-ray observatory VERITAS detected two asteroid occultations. By imaging the diffraction pattern produced during the ingress and egress of the occultation\, VERITAS measured at that time the smallest stellar angular diameter ever recorded of the G IV star TYC 278-748-1 (0.094+0.009 −0.010 mas). Currently\, several other stars have also had angular diameters measured. This presentation details the technique\, current analysis\, and some preliminary results for stellar angular diameters \nFecha: 31/01/2025 – 12:30Conferenciante: Joshua BartkoskeFiliación: University of Utah\, USA \n 
URL:https://www.iaa.csic.es/evento/resolving-stellar-angular-diameters-with-asteroid-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;TZID=Europe/Paris:20250130T190000
DTEND;TZID=Europe/Paris:20250130T200000
DTSTAMP:20260416T145727
CREATED:20250114T075954Z
LAST-MODIFIED:20250125T011041Z
UID:22668-1738263600-1738267200@www.iaa.csic.es
SUMMARY:La Tierra que acunó la vida: el papel de la sílice
DESCRIPTION:En esta conferencia exploraremos los nichos geoquímicos de la Tierra primitiva que pudieron albergar la transición de la geoquímica inorgánica a la geoquímica orgánica\, y de ahí a la química prebiotica y la emergencia de la complejidad que derivaría en las primeras estructuras similares a la vida.  \nDesvelaremos el papel crucial de los minerales\, en especial de la sílice\, en la autoorganización mineral y en la catálisis heterogénea de la química prebiótica. Y discutiremos la relevancia de esos resultados experimentales en el origen de la vida y en la detección de vida primitiva terrestre y extraterrestre. \nEl Dr. Juan Manuel García-Ruiz\, es Profesor Ikerbasque en el Donostia International Physics Center y Profesor de Investigación ad-honorem en el Instituto Andaluz de Ciencias de la Tierra en el CSIC. Lidera actualmente el proyecto ERC-Synergy “El papel del sílice en el amanecer de la vida en nuestro Planeta”. \nFecha: 30/01/2025 – 19:00Conferenciante: Juan Manuel García-RuizFiliación: Donostia International Physics Center e IACT-CSIC \n 
URL:https://www.iaa.csic.es/evento/la-tierra-que-acuno-la-vida-el-papel-de-la-silice/
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/2025/01/lucas_lara.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20250130T120000
DTEND;TZID=Europe/Paris:20250130T130000
DTSTAMP:20260416T145727
CREATED:20250127T084441Z
LAST-MODIFIED:20250912T080210Z
UID:24341-1738238400-1738242000@www.iaa.csic.es
SUMMARY:SO Colloquium: Modelling of large-scale magnetic field in low-mass stars
DESCRIPTION:Recent spectropolarimetric observations of low-mass stars show that large-scale components of their magnetic fields can exhibit cyclic variations or reversals. This magnetic activity affects detection of exoplanets and estimation of their masses\, and so its modelling is particularly important. In convective stellar envelopes\, magnetic fields are created through dynamo action – systematic stretching and twisting of magnetic field lines by helical convective vortices. It is yet however unclear how low-mass stars\, with their strong convective turbulence and relatively slow rotation\, are able to maintain coherent large-scale magnetic activity. In this talk\, I will discuss the physical mechanisms that allow magnetic flux to accumulate at large scales in both turbulent and strongly stratified models of stellar convection. In such models\, a highly turbulent convective layer is formed at the surface while the deep flow interiors remain rotationally constrained. Using direct numerical simulations of such flows\, I will show that small-scale magnetic flux\, generated by small-scale turbulence in the outer flow regions with low density\, is systematically transported into more quiescent inner regions by global magnetic pumping mechanism. Consequently\, the dipolarity of the field at the surface of the domain increases both with enhancement of turbulence and stratification. I will also explore the mechanisms of destabilization of magnetic fields resulting in magnetic reversals\, and their dynamical interactions with zonal flows; finally\, I will discuss the impact of differential rotation on magnetic fields during star formation. Both processes could be responsible for diversity of magnetic topology and activity patterns observed in low-mass stars. \nFecha: 30/01/2025 – 12:00Conferenciante: Dr. Anna GusevaFiliación: Observatoire de Paris\, France. \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-modelling-of-large-scale-magnetic-field-in-low-mass-stars/
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:20250128T123000
DTEND;TZID=Europe/Paris:20250128T133000
DTSTAMP:20260416T145727
CREATED:20241219T110050Z
LAST-MODIFIED:20250125T012544Z
UID:22519-1738067400-1738071000@www.iaa.csic.es
SUMMARY:El crecimiento de la complejidad en el Universo
DESCRIPTION:La existencia de vida es uno de los grandes problemas cosmológicos. Aunque la vida sea un hecho observado en un único planeta\, el proceso de complejización que supone\, debe obedecer a leyes generales universales. Varios autores claman por una “missing law” termodinámica\, a la búsqueda de la cual se incorpora la hipótesis que presentamos aquí. El surgimiento y la evolución de la vida son resultado del mismo principio. Se deduce que la complejidad crea complejidad\, lo que potencia los mecanismos evolutivos. Esta teoría no se presenta como alternativa a la teoría darwiniana\, sino como un necesario complemento.​ \nFecha: 28/01/2025 – 12:30Conferenciante: Dr. Eduardo BattanerFiliación: Universidad de Granada\, Spain
URL:https://www.iaa.csic.es/evento/el-crecimiento-de-la-complejidad-en-el-universo/
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:20250123T123000
DTEND;TZID=Europe/Paris:20250123T133000
DTSTAMP:20260416T145727
CREATED:20241219T105941Z
LAST-MODIFIED:20250125T200413Z
UID:22515-1737635400-1737639000@www.iaa.csic.es
SUMMARY:Study of the very high energy emission from star-forming regions and young massive star clusters
DESCRIPTION:Cosmic rays (CRs) are a fundamental component of the Cosmos. They can penetrate and ionise the dense gas core of molecular clouds\, affecting the dynamics of the cloud itself and triggering chemical reactions that lead to the creation of complex molecular compounds. In star-forming complexes\, CRs can be accelerated by the wind of newly born massive stars\, often found in young massive stellar clusters (YMSC). The amount of freshly injected CRs can be probed by the observations of high-energy and very-high-energy gamma-rays. In this regard\, the future Cherenkov Telescope Array Observatory (CTAO) will play a crucial role. CTAO will be composed of around 100 telescopes deployed on two sites\, one in Northern and one in the Southern Hemisphere. The arrays will cover a wide energy range from tens of GeV to hundreds of TeV employing telescopes of three sizes: the Large\, Medium and Small Sized Telescopes with 23 m\, 14 m and 4.5 m mirror diameters\, respectively. Each telescope is optimized for the detection of photons below 1 TeV (LST)\, between 1-10 TeV (MST) and above 10 TeV (SST). The first LST prototype\, LST-1\, is currently ending its commissioning phase and is starting to collect scientific data. During the present observational cycle\, two observational proposals on YMSC were submitted for the very first time. These observations are challenging due to the extension of the expected gamma-ray emission from YMSC and to the limited Field of View (FoV) of the Cherenkov telescopes (around 2.3° radius for LST-1). In this context is of paramount importance to optimise the reconstruction analysis chain (currently under development) for extended sources and to rank the best targets for the next observational campaigns both of LST-1 and of the upcoming 3 LSTs currently under construction at the CTAO-Northern site. \n​ \nFecha: 23/01/2025 – 12:30Conferenciante: Dr. Gaia VernaFiliación: Università degli Studi di Siena\, Italy
URL:https://www.iaa.csic.es/evento/study-of-the-very-high-energy-emission-from-star-forming-regions-and-young-massive-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:20250121T123000
DTEND;TZID=Europe/Paris:20250121T133000
DTSTAMP:20260416T145727
CREATED:20241219T105200Z
LAST-MODIFIED:20250125T200435Z
UID:22511-1737462600-1737466200@www.iaa.csic.es
SUMMARY:An Unusual Triple System: CN Lyn
DESCRIPTION:Triple star systems hold significant astrophysical importance\, offering profound insights into stellar evolution\, dynamical interactions\, and mass transfer processes. Due to their complexity compared to single or binary star systems\, triple systems facilitate a more comprehensive understanding of stellar processes from formation to final stages. Thanks to large photometric surveys\, such as Kepler\, researchers were able to detect triple systems with long periods. Also\, the latest studies show that 15% of binaries have a tertiary component. Therefore\, studying such objects will lead to results that benefit every aspect of stellar astrophysics. In this talk\, I will present our latest study of known but not studied in detail triple star system\, CN Lyn\, and our findings by combining spectroscopy\, photometry\, and galactic dynamic techniques. \nFecha: 21/01/2025 – 12:30Conferenciante: Dr. Gökhan YücelFiliación: Department of Astronomy and Space Sciences\, Istanbul University\, Turkey
URL:https://www.iaa.csic.es/evento/an-unusual-triple-system-cn-lyn/
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:20250121T090000
DTEND;TZID=Europe/Paris:20251030T170000
DTSTAMP:20260416T145727
CREATED:20241219T121029Z
LAST-MODIFIED:20250912T080532Z
UID:22550-1737450000-1761843600@www.iaa.csic.es
SUMMARY:Academic Spanish Course for Foreigners (2025)
DESCRIPTION:The Academic Spanish course for foreigners is designed to facilitate effective communication in academic and profesional contexts. Through a practical and personalized focus\, the participants will develop essential linguistic abilities to discuss scientific articles\, participate in conferences\, give presentations\, and collaborate in international projects. The program includes technical vocabulary\, beginner and advanced grammar\, and simulations of real-life situations. Moreover\, it will promote the cultural immersion to strengthen the comprehension of the Hispanic world\, and their impact on interdisciplinary investigation and collaboration. \nThis course will be taught throughout in the following blocks: \nJanuary 21st – February 27thApril 22nd – May 29thSeptember 23rd – October 30thThe course is taught by Prof. Nazira Ruíz
URL:https://www.iaa.csic.es/evento/academic-spanish-course-for-foreigners-2025/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/12/academicspanish.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241219T190000
DTEND;TZID=Europe/Paris:20241219T200000
DTSTAMP:20260416T145727
CREATED:20241219T110912Z
LAST-MODIFIED:20250125T010309Z
UID:22529-1734634800-1734638400@www.iaa.csic.es
SUMMARY:¿Qué sabemos de nuestra Galaxia después de Gaia?
DESCRIPTION:En los últimos 11 años\, los resultados de la misión Gaia han revolucionado nuestro conocimiento sobre la Vía Láctea\, ofreciendo un nivel de detalle sin precedentes. Este observatorio espacial ha cartografiado con extrema precisión las posiciones\, movimientos y fotometría de más de mil ochocientos millones de estrellas\, proporcionando una visión tridimensional de nuestra galaxia. Gracias a Gaia\, ahora entendemos mejor la estructura espiral de la Vía Láctea\, los procesos de formación estelar y las interacciones gravitatorias con otras galaxias cercanas. \nLos datos han revelado sorprendentes ondulaciones en el disco galáctico\, probablemente causadas por encuentros con galaxias satélite como la Sagitario. También han permitido identificar cúmulos estelares\, corrientes de estrellas y patrones de movimiento que nos cuentan la historia dinámica de la Galaxia. Además\, Gaia ha mejorado significativamente nuestras mediciones de distancias y masas estelares\, lo que impacta directamente  en una  mejor comprensión de la evolución estelar. \nEn esencia\, Gaia no solo ha transformado la astrofísica\, sino que ha permitido a la humanidad explorar con mayor claridad su hogar galáctico\, abriendo nuevas preguntas y desafíos en nuestra búsqueda por comprender el cosmos. \nFecha: 19/12/2024 – 19:00Conferenciante: Emilio J. AlfaroFiliación: Instituto de Astrofísica de Andalucía IAA-CSIC \n 
URL:https://www.iaa.csic.es/evento/que-sabemos-de-nuestra-galaxia-despues-de-gaia/
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/2024/12/alfaro.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241212T123000
DTEND;TZID=Europe/Paris:20241212T133000
DTSTAMP:20260416T145727
CREATED:20241119T085028Z
LAST-MODIFIED:20250125T200500Z
UID:22456-1734006600-1734010200@www.iaa.csic.es
SUMMARY:Informative Session for Foreign New Hires
DESCRIPTION:If you are a foreigner who has recently joined the IAA and have not yet completed all the steps to formalize your residency in Spain\, or if you would like to learn about some of the optional bureaucratic procedures that could make things easier for you living here\, please join us for this informative session led by the Area of Visitor Assistance. \nThe session will be held in English and is open to anyone at the IAA who would like to inform themselves on these procedures. Topics covered will include: \n\nRegistry and Green Card for EU Citizens\nEmpadronamiento • TIE Card\nHealth Card\nDigital Certificate/Signature\nElectoral Registry for EU Citizens\nFinalizing the Doctorate Degree Equivalency with the UGR\n\nFecha: 12/12/2024 – 12:30Conferenciante: Lauren C. SmithFiliación: Severo Ochoa-IAA Research Support Office. Instituto de Astrofísica de Andalucía
URL:https://www.iaa.csic.es/evento/informative-session-for-foreign-new-hires/
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:20241212T103000
DTEND;TZID=Europe/Paris:20241212T163000
DTSTAMP:20260416T145727
CREATED:20241219T114506Z
LAST-MODIFIED:20250912T080537Z
UID:22536-1733999400-1734021000@www.iaa.csic.es
SUMMARY:PySnack 10: PROSE
DESCRIPTION:PySnacks\nWithin the  Severo Ochoa Training Initiative of the IAA-CSIC we are offering short introductory practical courses about Python packages for astrophysical applications (PySnacks). We invite you to participate in the 4h course PySnack 10: PROSE \nAbstract\nApproximately 75% of known exoplanets have been discovered by identifying transit signals in the light curves of their host stars. These discoveries start with the acquisition of raw images of the sky\, followed by the extraction of stellar time-series photometry. In this workshop\, we will process ground-based observations of the star TRAPPIST-1 to replicate the detection of its first exoplanet transit using original data from the TRAPPIST telescope. Participants will learn to calibrate raw images and extract TRAPPIST-1’s light curve using prose\, a Python package designed for modular image processing in astronomy. Finally\, we will apply nuance\, a detection algorithm tailored for identifying transits in noisy datasets. \nOverall\, participants will gain hands-on experience in image calibration\, light curve extraction\, and transit detection\, along with practical skills in using Python tools for astronomical data analysis.
URL:https://www.iaa.csic.es/evento/pysnack-10-prose/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/12/prosetransparent.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241210T123000
DTEND;TZID=Europe/Paris:20241210T133000
DTSTAMP:20260416T145727
CREATED:20241119T084818Z
LAST-MODIFIED:20250125T200517Z
UID:22450-1733833800-1733837400@www.iaa.csic.es
SUMMARY:ESERO\, from space to the classroom
DESCRIPTION:With the slogan ‘from space to the classroom’\, and building on the fascination that students have for space\, the European Space Agency’s (ESA) European Space Education Resource Office in Spain (ESERO Spain) provides resources to primary and secondary school teachers to improve their literacy and STEM (Science\, Technology\, Engineering and Mathematics) skills. Using the theme of space as a context for inspiration and motivation\, ESERO runs a programme of training and continuous professional development\, based on a unique combination of science\, technology and teaching expertise. This combination challenges the traditional way science is taught in schools and involves the application of innovative learning methodologies. \nFecha: 10/12/2024 – 12:30Conferenciante: Dr. Manuel GonzálezFiliación: Oficina ESERO Spain
URL:https://www.iaa.csic.es/evento/esero-from-space-to-the-classroom/
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:20241203T123000
DTEND;TZID=Europe/Paris:20241203T133000
DTSTAMP:20260416T145727
CREATED:20241119T084619Z
LAST-MODIFIED:20250125T200534Z
UID:22444-1733229000-1733232600@www.iaa.csic.es
SUMMARY:Experimental ice simulations for the interpretation of ice and organics observations in the Solar System
DESCRIPTION:The harsh conditions in space (ultra-high vacuum\, cryogenic temperatures\, and radiation) are simulated in laboratory chambers to study ice properties and processes. UV photons/X-rays/ions impact on the ice covering microscopic dust particles in dense interstellar clouds\, comets\, icy moons and planetary surfaces. Radiation produces radicals and reactive species changing the initial composition of the ice (made of simple species like water\, CO\, CO2\, CH3OH\, NH3\, etc) to form complex molecules of prebiotic interest (amino acids\, nucleobases\, sugars\, …) in the laboratory. Many of these molecules were also identified in comets and asteroids. \nThe ice porosity and degree of order in the structure of these ices may also serve to trace their thermal and radiative history. Infrared spectroscopy is a powerful tool to gather detailed information of ices in space\, while mass spectrometry allows to characterize the gas composition. Ice laboratory studies have become essential to prepare new cometary and icy moon missions and to interpret the results delivered by these missions. We will present the application of the ice experiments to the Rosetta mission\, Hayabusa 2\, JUICE and JWST. \nFecha: 03/12/2024 – 12:30Conferenciante: Dr. Guillermo Muñoz CaroFiliación: Centro de AstroBiología – CSIC
URL:https://www.iaa.csic.es/evento/experimental-ice-simulations-for-the-interpretation-of-ice-and-organics-observations-in-the-solar-system/
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:20241202T093000
DTEND;TZID=Europe/Paris:20241202T133000
DTSTAMP:20260416T145727
CREATED:20241121T160454Z
LAST-MODIFIED:20250912T080541Z
UID:22484-1733131800-1733146200@www.iaa.csic.es
SUMMARY:PySnack 9: GASTLI
DESCRIPTION:PySnacks\nWithin the  Severo Ochoa Training Initiative of the IAA-CSIC we are offering short introductory practical courses about Python packages for astrophysical applications (PySnacks). We invite you to participate in the 4h course PySnack 9: GASTLI \nAbstract\nUnderstanding the interior composition of exoplanets is key to uncovering their formation and evolutionary histories\, especially their metal content. By comparing observed mass and radius measurements with interior structure and evolution models\, we can infer a planet’s metal mass fraction. With the advent of JWST\, CHEOPS\, TESS\, and the upcoming PLATO\, we are entering an era of unprecedented precision in exoplanet radius\, age\, and atmospheric metallicity measurements. \nTo harness this growing wealth of data\, we introduce GASTLI (GAS gianT modeL for Interiors) — a user-friendly\, open-source Python package designed to make interior modeling accessible. GASTLI is optimized for rapid computation of mass-radius and radius-luminosity-age relationships and enables interior composition retrievals to fit models to observed mass\, radius\, age\, and\, when available\, atmospheric metallicity. \nSupporting a diverse range of planetary compositions\, masses\, and irradiation conditions\, GASTLI is ideal for modeling planets from warm sub-Neptunes to hot gas giants. It incorporates state-of-the-art thermodynamic data and equations of state for rock\, water\, and hydrogen/helium\, alongside a customizable atmospheric grid feature\, ensuring accurate representation of high-pressure planetary envelopes. \nThis course will be taught by Lorena Acuña (MPIA-Heidelberg). \n 
URL:https://www.iaa.csic.es/evento/pysnacks-8-pybdsf-2/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2024/11/gastly.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241128T190000
DTEND;TZID=Europe/Paris:20241128T200000
DTSTAMP:20260416T145727
CREATED:20241219T110541Z
LAST-MODIFIED:20250125T010331Z
UID:22523-1732820400-1732824000@www.iaa.csic.es
SUMMARY:Sobre supernovas\, agujeros negros y cinturones de radiación en enanas marrones
DESCRIPTION:Muchas veces imágenes obtenidas con técnicas novedosas\, y al límite técnico\, son cruciales para hacer descubrimientos. \nAsí fue entre otros casos\, y como es bien sabido\, para el descubrimiento de la estructura de doble hélice del ADN. También aspectos esenciales de las radioemisiones de las supernovas\, los agujeros negros masivos y las enanas marrones se han descubierto a través de imágenes obtenidas con una misma técnica de muy alta resolución angular utilizada cada vez de modo muy distinto y en el límite técnico. \nEn la charla se abordará de modo conciso lo que es esencial a cada uno de esos descubrimientos que nos han permitido conocer los detalles de la expansión de las supernovas\, del entorno de los agujeros negros masivos y de los cinturones de radiación que rodean a las enanas marrones como lo hacen a Júpiter o la Tierra.   \nFecha: 28/11/2024 – 19:00Conferenciante: Jon MarcaideFiliación: Real Academia de Ciencias Exactas\, Físicas y Naturales de España \n 
URL:https://www.iaa.csic.es/evento/sobre-supernovas-agujeros-negros-y-cinturones-de-radiacion-en-enanas-marrones/
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/2024/12/marcaide.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241128T123000
DTEND;TZID=Europe/Paris:20241128T133000
DTSTAMP:20260416T145727
CREATED:20241119T084404Z
LAST-MODIFIED:20250912T080215Z
UID:22440-1732797000-1732800600@www.iaa.csic.es
SUMMARY:SO Colloquium: Cosmic chemical evolution: here\, there\, and everywhere
DESCRIPTION:Metals play a very important role in star formation and stellar evolution. Amongst other things they control the cooling of the interstellar gas\, thus allowing the formation of stars; they affect the radiation transport\, through the opacities involved in the different microscopic processes; and they have the most important role in the dust formation and in the mass loss from stars. Metals are formed inside stars. Therefore\, it is expected that metal enrichment in the universe should start soon after the formation of the first massive stars that\, after a very short life\, would return to the interstellar medium (ISM) in explosive events newly synthesised chemical elements\, heavier than the primordial hydrogen and helium. It is thought that this ejecta\, at some point mixed with the surrounding gas\, would help to its cooling and propitiate the appearance of a new generation of stars\, hence giving rise to the cycle of cosmic chemical evolution. All this wealth of detail is somehow imprinted in the distribution of abundances in galaxies. The absolute quantities of metals a galaxy (or a region of a galaxy) possesses\, the relative abundances of the different elements\, and their spatial distribution in a given galaxy are important constraints for the verification of our models and scenarios of the formation and evolution of galaxies. \nThere are two ways of handling and exploiting this information. One is to derive abundances in galaxies “in situ”\, i. e. in galaxies at their different redshifts. In that way\, we can observe the gas abundances at the time of the emission of radiation and thus obtain the value of the mean abundances of the gas at a given epoch. The other one is to derive the gas abundances at the present epoc \, that is\, observing galaxies at redshift zero and then use chemical evolution models to infer their abundances at previous epochs. \nEventually both approaches must converge in a single galaxy formation and evolution scenario. Once that convergence is achieved\, the models can be extrapolated back to even earlier times and predictions can be made which can be contrasted with planned observations. \nFecha: 28/11/2024 – 12:30Conferenciante: Profesora Ángeles DíazFiliación: Universidad Autónoma de Madrid\, Madrid\, España
URL:https://www.iaa.csic.es/evento/so-colloquium-cosmic-chemical-evolution-here-there-and-everywhere/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20241126
DTEND;VALUE=DATE:20241129
DTSTAMP:20260416T145727
CREATED:20240906T091217Z
LAST-MODIFIED:20250124T165929Z
UID:21886-1732579200-1732838399@www.iaa.csic.es
SUMMARY:Hot Topics High Energy Astrophysics HONEST 3
DESCRIPTION:The high energy end of  pulsar spectra. \nPulsars as rapidly spinning neutron stars have always been excellent laboratories for the study of plasma physics\, particle acceleration and cosmic rays. Comprehending how and where particles are accelerated to produce the broadband shape that the pulsed spectra present is subject of enthusiastic discussions and constitute one of the hot topics in high energy astrophysics nowadays.  \nResults from the recent years extending pulsar spectra to TeV energies and beyond motivate debates that can only be elucidated through a deep understanding of the high energy end of their spectrum. In this Workshop\, we aim to discuss the latest results on pulsars from high energy instruments\, their implications for the current theories\, and prospects for future observatories. \n 
URL:https://www.iaa.csic.es/evento/hot-topics-in-high-energy-astrophysics-honest-3/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Workshops
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/congresscover-2-e1752660237822.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241125T113000
DTEND;TZID=Europe/Paris:20241125T130000
DTSTAMP:20260416T145727
CREATED:20241113T155256Z
LAST-MODIFIED:20250912T080546Z
UID:22408-1732534200-1732539600@www.iaa.csic.es
SUMMARY:Introduction to GitHub
DESCRIPTION:This session is a hands-on introduction to using GitHub for scientific research collaboration within the  Severo Ochoa Training Initiative of the IAA-CSIC. We’ll explore software repositories and their role in managing and sharing research work within a group. Key concepts—such as commits\, forks\, pushes\, pulls\, and pull requests—will be clarified with practical examples of their use. Participants will also receive practical guidance on repository management and effective collaboration techniques. The session includes a hands-on component where attendees will create repositories and work together to build and populate a shared repository using GitHub’s tools. \n(Note: This tutorial will focus on GitHub’s interface and functionality\, not on Git. A follow-up session will address Git fundamentals in depth.) \nInformation\n– This event is a hands-on session on how to use GitHub. It will be given by Manuel Parra and Javier Moldón\, from the IAA-CSIC.– This training event will be primarily held in-person at the IAA. While remote participation is available\, in-person attendees will be prioritized given the interactive and hands-on nature of the session.– Registration is required (see below). \nContent\nLecture: Introduction to Github \nPractical exercises:– Exercise 1 – Create an initial repository for this session– Exercise 2 – Managing forks to collaborate– Exercise 3 – Managing branches– Exercise 4 – Common project. Interacting with repositories and users. Parallel merge requests \nDate and location\nPlace: Sala Polivalente\, Building A\, IAA-CSICDate and time: Monday\, November 25th\, 11:30 to 13:00h \nRegistration\nPlease register at https://forms.gle/BUHDGhEFxRV5J4YS8 before the 19 November 2024. The number of participants will be limited to 15. First come\, first serve.
URL:https://www.iaa.csic.es/evento/introduction-to-github/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241121T123000
DTEND;TZID=Europe/Paris:20241121T133000
DTSTAMP:20260416T145727
CREATED:20241119T084019Z
LAST-MODIFIED:20250125T200612Z
UID:22436-1732192200-1732195800@www.iaa.csic.es
SUMMARY:Towards the Standardization of the Modeling of Multi-Frequency Observations
DESCRIPTION:Blazars\, a class of Active Galactic Nuclei (AGN) with relativistic jets oriented toward Earth\, are powerful and highly variable emitters across the electromagnetic spectrum. Time-domain multi-messenger and multi-wavelength (MWL) studies are essential for understanding the physical processes at work on these systems\, yet they often rely on proprietary tools specific to each instrument for reconstructing and modeling the collected data. In this talk\, the current state of blazar studies is briefly outlined within the context of astroparticle physics and gamma-ray astrophysics\, with a focus on the importance of MWL observations. \nIn the second part\, we explore the use of the open-source Python package Gammapy\, originally developed for gamma-ray data analysis\, to design a unified framework for MWL analyses\, spanning a broad energy range from optical to gamma-rays. Recent data from the flaring blazars OP 313 and 4C+27.50 are used to illustrate how a consistent analysis and modeling of the data can be performed by integrating observations from instruments such as the Liverpool Telescope\, Swift\, NuSTAR\, and Fermi-LAT. A forward-folding approach is employed\, providing a more rigorous treatment of observational data\, instrument responses and astrophysical and instrumental backgrounds. With this\, we demonstrate the potential of open-source tools and standardized data formats to unify traditionally isolated datasets\, setting the path for more accessible and reproducible MWL studies. The seminar concludes with a discussion of two immediate applications of this methodology in AGN research. \nFecha: 21/11/2024 – 12:30Conferenciante: Dra. Mireia Nievas RosilloFiliación: IAC\, Canarias\, Spain
URL:https://www.iaa.csic.es/evento/towards-the-standardization-of-the-modeling-of-multi-frequency-observations/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241114T123000
DTEND;TZID=Europe/Paris:20241114T133000
DTSTAMP:20260416T145727
CREATED:20241113T104538Z
LAST-MODIFIED:20250125T200631Z
UID:22382-1731587400-1731591000@www.iaa.csic.es
SUMMARY:Ozone and the Search for Life in the Universe
DESCRIPTION:As we approach the era where we will be able to characterize the atmospheres of terrestrial exoplanets\, we are put on a path to answer one of humanity’s most compelling questions: are we alone in the universe? Molecular oxygen (O2) with a reducing gas (i.e.\, methane) is widely regarded as a promising biosignature – a sign of life in the atmospheres of terrestrial exoplanets. However\, there are circumstances in which O2 will be very difficult or impossible to detect\, such as in atmospheres with small amounts of O2 (as was the case for much of Earth’s history)\, or for missions looking in the mid-IR. For these scenarios\, it has been suggested that ozone (O3)\, the photochemical product of O2\, could be used as a proxy to infer the presence of O2. While O3 is not directly produced by life\, it plays an important role in habitability as the ozone layer is the primary source of UV shielding for surface life on Earth. However O3 production is known to have a nonlinear dependence on O2\, along with being strongly influenced by the UV spectrum of the planet’s host star. In this talk I will discuss planetary habitability in general as well as the climate and photochemistry modeling I have done to assess the reliability of O3 as a proxy for O2. Overall I find that the O2-O3 relationship varies significantly around different stellar hosts\, with distinct trends between planets orbiting hotter stars (G0V-K2V) versus cooler stars (K5V-M5V). Understanding the full context of the planetary atmosphere will be key for interpreting emission spectral features of biosignature gases. \nFecha: 14/11/2024 – 12:30Conferenciante: Dr. Thea KozakisFiliación: IAA-CSIC\, Granada\, Spain
URL:https://www.iaa.csic.es/evento/ozone-and-the-search-for-life-in-the-universe/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241107T123000
DTEND;TZID=Europe/Paris:20241107T133000
DTSTAMP:20260416T145727
CREATED:20241023T085356Z
LAST-MODIFIED:20250912T080219Z
UID:22352-1730982600-1730986200@www.iaa.csic.es
SUMMARY:SO Colloquium: The tidal arms of open star clusters are much longer than thought\, but more difficult to find
DESCRIPTION:The tidal arms of stellar clusters are an important tool for studying the clusters’ birth conditions\, their evolution\, coupling\, and interaction with the Galactic potential. They also help understand how field stars populate the Milky Way. Thanks to Gaia\, much progress has been accomplished in finding the tidal arms of open clusters. I will show here that such arms are much longer than previously observed\, and that their identification requires not only a sophisticated analysis of the Gaia catalogue\, using the convergent point method and clustering algorithms\, but ideally\, the use of N-body simulations and the new compact convergent point method. I will highlight recent results about the arms of several open clusters\, which extend over several hundreds of parsecs. \nFecha: 07/11/2024 – 12:30Conferenciante: Dr. Henri BoffinFiliación: European Southern Observatory
URL:https://www.iaa.csic.es/evento/so-colloquium-the-tidal-arms-of-open-star-clusters-are-much-longer-than-thought-but-more-difficult-to-find/
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