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X-WR-CALNAME:Instituto de Astrofísica de Andalucía
X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241010T190000
DTEND;TZID=Europe/Paris:20241121T210000
DTSTAMP:20260423T064338
CREATED:20241004T123407Z
LAST-MODIFIED:20241021T144311Z
UID:22038-1728586800-1732222800@www.iaa.csic.es
SUMMARY:El Universo desde Sevilla III
DESCRIPTION:«El Universo desde Sevilla» llega a su tercera edición como un programa de conferencias para la difusión de la Astrofísica y Ciencias del Espacio de especialistas de Sevilla.  \nEs una contribución del Consejo Superior de Investigaciones Científicas (CSIC) y en particular del Museo Casa de la Ciencia (CSIC) de Sevilla. El fin es destacar el potencial científico-tecnológico-empresarial que tiene Sevilla y Andalucía en el área aeroespacial. \nEsta iniciativa\, que se desarrollará con tres ponencias durante los meses de octubre y noviembre\, está coordinada por el investigador del Instituto de Astrofísica de Andalucía (IAA-CSIC) Emilio J. Alfaro Navarro. \nEl programa es el siguiente:  \n10 de octubre de 2024. «El Sol desde el espacio»  \nJose Carlos del Toro Iniesta (IAA-CSIC) \nEl Sol es nuestra estrella más cercana y\, además de proporcionar la energía necesaria para la vida\, es un laboratorio que nos aporta información sobre el resto de estrellas y otras ramas de la física como la atómica. Se observa desde tiempos inmemoriales\, pero ahora podemos hacerlo desde el espacio abriendo una ventana de conocimiento que no era accesible desde la Tierra. \n \n7 de noviembre de 2024. «Entre lo visible y lo invisible: Materia y energía oscuras»  \nJosé Oñorbe Bernis (US) \nEn el modelo cosmológico estándar actual sólo el 5% del universo está hecho de materia ordinaria\, como los átomos que forman las estrellas\, los planetas\, y nosotros. El resto del universo es oscuro y desconocido\, compuesto de materia y energía oscuras. ¿Qué son estas componentes oscuras? ¿Por qué parecen ser tan relevantes en nuestro Universo? En esta conferencia intentaremos contestar a estas preguntas y hablaremos de las observaciones clave que han dado lugar a este modelo. Además discutiré sobre otras interpretaciones fuera del modelo estándar y por supuesto\, habrá mucho tiempo para contestar vuestras preguntas. \n \n21 de noviembre de 2024. «Los polvos del universo: polvo cósmico y COVID»   \nOlga Muñoz Gómez (IAA-CSIC) \nOlga Muñoz\, directora del Laboratorio de Polvo Cósmico\, Instituto de Astrofísica de Andalucía (IAA)\, nos hablará sobre que el polvo cósmico es lo que conocemos como polvo de estrellas\, el que se forma en la nube de gas en expansión en una estrella y es el polvo a partir del cual se forman todos los cuerpos que conocemos en el universo.
URL:https://www.iaa.csic.es/evento/el-universo-desde-sevilla-iii/
LOCATION:Casa de la Ciencia de Sevilla\, Av. de María Luisa\, s/n\, Sevilla\, Sevilla\, 41013\, Spain
CATEGORIES:Actividades
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2024/10/Sevilla.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20241104
DTEND;VALUE=DATE:20241109
DTSTAMP:20260423T064338
CREATED:20240605T090237Z
LAST-MODIFIED:20250912T080554Z
UID:21517-1730678400-1731110399@www.iaa.csic.es
SUMMARY:Writing and Communicating your Science
DESCRIPTION:There is no science without communication and no successful scientists without good writing and communication skills. You can do the best science that exists\, if you don’t write papers about it – papers that get cited! ­– and if you don’t give presentations that impress people\, your science will likely be ignored. Moreover\, if you do not write convincing proposals that appeal to non-specialists\, you won’t get observing time\, nor the coveted post-doc position and certainly not the very competitive but needed grants to fund your research. Finally\, as a scientist\, it is your duty and privilege to communicate your science to the general public\, policy makers and the media\, and like all the rest\, this is something that needs to be learned.  \nThis course is an introduction about how to get your message across in the various supports you need to use as a scientist. It is aimed are junior scientists who are writing their first papers\, but will also be helpful for colleagues with more experience. The skills learned in this course will be more generally applicable as well\, whether or not you not plan to build a further career as an academic. \nThe course will be split in five sessions combining two hours of lectures and 1.5 hours of exercises. During the course and the exercises\, you will refer to your own writing when we discuss items like title\, abstract\, introduction\, or paragraph and sentence structure\, so bring with you your latest paper\, whether in early draft form or submitted to a journal.
URL:https://www.iaa.csic.es/evento/writing-and-communicating-your-science/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/congresscover-2-e1752660237822.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241106T123000
DTEND;TZID=Europe/Paris:20241106T133000
DTSTAMP:20260423T064338
CREATED:20241023T084843Z
LAST-MODIFIED:20250125T200710Z
UID:22348-1730896200-1730899800@www.iaa.csic.es
SUMMARY:New UGR proceedings for PhDs
DESCRIPTION:Every year we all doubt what needs to be done and uploaded for the university. This is a reminder and updated seminar about the current proceedings that affect the PhD\, especially important since the UGR has modified some things recently. \nFecha: 06/11/2024 – 12:30Conferenciante: Dr. Antonio García HernándezFiliación: UGR\, Granada
URL:https://www.iaa.csic.es/evento/new-ugr-proceedings-for-phds/
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:20241107T123000
DTEND;TZID=Europe/Paris:20241107T133000
DTSTAMP:20260423T064338
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
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241114T123000
DTEND;TZID=Europe/Paris:20241114T133000
DTSTAMP:20260423T064338
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
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:20241121T123000
DTEND;TZID=Europe/Paris:20241121T133000
DTSTAMP:20260423T064338
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
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:20241125T113000
DTEND;TZID=Europe/Paris:20241125T130000
DTSTAMP:20260423T064338
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
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/congresscover-2-e1752660237822.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20241126
DTEND;VALUE=DATE:20241129
DTSTAMP:20260423T064338
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
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20241128T123000
DTEND;TZID=Europe/Paris:20241128T133000
DTSTAMP:20260423T064338
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;TZID=Europe/Paris:20241128T190000
DTEND;TZID=Europe/Paris:20241128T200000
DTSTAMP:20260423T064338
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
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END:VEVENT
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