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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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TZID:Europe/Paris
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251201T090000
DTEND;TZID=Europe/Paris:20251205T140000
DTSTAMP:20260406T095255
CREATED:20251002T081202Z
LAST-MODIFIED:20251002T081205Z
UID:27556-1764579600-1764943200@www.iaa.csic.es
SUMMARY:Gestión de proyectos con metodologías ágiles y Redmine
DESCRIPTION:Contenidos  \n1. Introducción a las Metodologías Ágiles2. Prácticas Ágiles Fundamentales3. Instalación y Configuración de Redmine4. Gestión Ágil con Redmine y el Plugin Agile5. Caso Práctico: Adopción de Agile con Redmine6. Conclusiones y Mejores Prácticas
URL:https://www.iaa.csic.es/evento/gestion-de-proyectos-con-metodologias-agiles-y-redmine/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Training
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2025/10/pexels-goumbik-669610.jpg
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251202T123000
DTEND;TZID=Europe/Paris:20251202T133000
DTSTAMP:20260406T095255
CREATED:20250930T090312Z
LAST-MODIFIED:20251127T154254Z
UID:27510-1764678600-1764682200@www.iaa.csic.es
SUMMARY:MeerKAT imaging of nearby galaxies
DESCRIPTION:Star formation is one of the dominant internal processes that drive galaxy evolution. We investigate the environmental effects on star formation activity in three nearby galaxy groups: NGC 6221\, NGC 3263 and NGC 2434. These groups were chosen to represent an evolutionary sequence ranging from the early stages to the late stages: from an interacting pair with tidal debris to a loose pre-processing group and finally to a more evolved system dominated by an elliptical galaxy. \nWe use a combination of high-resolution MeerKAT radio continuum data and WISE infrared observations to locate and measure the star formation rate in all group members. We use PAH emission as a tracer of gas heated by young stars to achieve this. In-band spectral index maps constrain the physical mechanisms driving the radio emission\, while SED fitting yields the ages and masses of a subset of the galaxies. \nDepending on the evolutionary stage of their group\, we find that galaxies occupy distinct regions of the WISE colour–colour diagram. All systems except ESO 059–G012 follow the radio–W3PAH correlation; the latter’s deviation may indicate that it has already exhausted its gas reservoir. The data also support the idea that the Vela Cloud originated from an interaction\, likely involving NGC 3263\, NGC 3256B and NGC 3256C. Finally\, our results are consistent with the presence of low-luminosity active galactic nuclei (AGN) in NGC 6221 and NGC 3256\, as previously suggested in the literature. \nFecha y lugar: 02/12/2025 – 12:30 | Sala de JuntasJuliana SaponaraInstituto Argentino de Radioastronomia (IAR) \n 
URL:https://www.iaa.csic.es/evento/meerkat-imaging-of-nearby-galaxies/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251204T123000
DTEND;TZID=Europe/Paris:20251204T133000
DTSTAMP:20260406T095255
CREATED:20251030T103159Z
LAST-MODIFIED:20251204T123759Z
UID:27976-1764851400-1764855000@www.iaa.csic.es
SUMMARY:SO Colloquium: The Earth 2.0 (ET) Space Mission
DESCRIPTION:The Earth 2.0 (ET) mission\, currently in Phase B and scheduled for launch in fall 2028\, aims to discover Earth-like exoplanets using a dedicated space observatory at the Earth-Sun L2 point. It will combine six wide-field transit telescopes and one microlensing telescope\, leveraging large-format CMOS detectors for ultra-precise photometry. Over its four-year primary mission\, ET will monitor ~3 million nearby dwarf stars for transits and ~30 million stars in the Galactic bulge for microlensing events. Simulations suggest the mission will detect ~17 Earth 2.0 analogs\, ~25 free-floating Earth-mass planets\, over 4000 terrestrial-like planets\, and tens of thousands of additional exoplanets. \nThis talk will present an overview of the mission design\, technical innovations\, and its potential for exoplanet\, stellar and time-domain sciences. \nFecha y lugar: 04/12/2025 – 12:30 | Salón de ActosJian GeShanghai Astronomical Observatory \n  \n 
URL:https://www.iaa.csic.es/evento/the-earth-2-0-et-space-mission/
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
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251209T123000
DTEND;TZID=Europe/Paris:20251209T133000
DTSTAMP:20260406T095255
CREATED:20251015T110641Z
LAST-MODIFIED:20260107T100028Z
UID:27740-1765283400-1765287000@www.iaa.csic.es
SUMMARY:SO Colloquium: Planetesimal vs. Pebble Accretion
DESCRIPTION:A major issue in planet formation theory is whether the terrestrial planets formed mostly by accreting asteroid-sized (~100 km) planetesimals\, or mostly by accreting small (~cm) pebbles. In either theory\, planetesimals are the first steps in formation\, and these may accrete into Mars-sized planets within the ≈2 Myr lifetime of the inner disk. Pebble accretion has been rejected for various reasons\, but those reasons don’t actually discriminate between the theories. One objection is that even mm-sized objects are commonly thought to drift into the Sun in < 2 Myr due to aerodynamic drag. This would prevent terrestrial planets from accreting pebbles with «NC» (inner-disk) isotopic composition. But it would also be a problem for formation of planetesimal parent bodies of chondrites. \nHowever\, I’ll show that the combination of the pebble trap at the dead zone inner edge\, plus turbulent diffusion of chondrules\, is quite favorable for retention of chondrule-sized pebbles\, enabling both pebble accretion and planetesimal accretion. Another objection is the geochemical constraint from Hf-W dating that Earth’s core’s formed over ~10^8 yr\, consistent with planetesimal accretion. However\, nebular H\, He\, and Ne in Earth’s deep mantle demand ingassing into a magma ocean\, and rapid core formation in ~ 10^6 yr. This geochemical constraint demands the Earth’s Hf-W age was reset during the Moon-forming impact and does not discriminate between the scenarios. What might discriminate between the formation scenarios are moderately volatile element (MVE) abundances. Whereas Mars has MVE patterns consistent with planetesimal accretion of chondrites\, Earth is depleted in MVEs. I describe a scenario by which Earth’s embryos mostly grew by accretion of MVE-depleted chondrule-sized pebbles. While Mars might have grown from planetesimals\, growth of larger planets (proto-Earth\, possibly Theia and Venus\, and super-Earth exoplanets) likely is dominated by pebble accretion. \nFecha y lugar: 09/12/2025 – 12:30 | Salón de ActosSteve DeschArizona State University\, USA \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-planetesimal-vs-pebble-accretion/
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
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251211T123000
DTEND;TZID=Europe/Paris:20251211T133000
DTSTAMP:20260406T095255
CREATED:20251002T110437Z
LAST-MODIFIED:20260107T100033Z
UID:27568-1765456200-1765459800@www.iaa.csic.es
SUMMARY:SO Colloquium:  MOSAIC: the multi-object spectrograph for the ELT
DESCRIPTION:MOSAIC will be a multi-object spectrograph for the ELT. It is being designed to work at visible and NIR wavelengths\, and with different observing modes. During the first years of operation of the instrument it will carry out several surveys that will focus on the most relevant key-projects in Astronomy: first galaxies\, mass assembly along the Universe evolution\, exoplanets\, etc… \nThe IAA-CSIC is contributing to the development of the instrument\, as well as to the scientific team that is defining the first observations. The Principal Investigator of the project will update the progress of the project\, both from the technological and scientific points of view. \nFecha y lugar: 11/12/2025 – 12:30 | Salón de ActosRoser PellóLaboratoire d’astrophysique de Marseille (LAM) \n 
URL:https://www.iaa.csic.es/evento/mosaic-the-multi-object-spectrograph-for-the-elt/
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:20251215T130000
DTEND;TZID=Europe/Paris:20251215T133000
DTSTAMP:20260406T095255
CREATED:20251015T110754Z
LAST-MODIFIED:20251203T120633Z
UID:27743-1765803600-1765805400@www.iaa.csic.es
SUMMARY:Simulations to unlock Micro-Arcsecond Astronomy with La Palma Quantum Interferometry (LPQI)
DESCRIPTION:Stars in the night sky\, even in nearby multi-star systems\, generally appear as unresolved points of light through conventional telescopes. Achieving sub-milliarcsecond resolution at optical wavelengths requires the use of interferometric techniques. While Michelson stellar interferometers now reach baselines of up to 300 m\, extending angular resolution to even finer scales demands a complementary approach: Intensity Interferometry (II). The recent global resurgence of II has opened new possibilities for high-precision studies of massive and evolved stars. \nThe Observatorio del Roque de los Muchachos (ORM) on La Palma\, with its large-aperture telescopes and long baselines\, offers a unique platform for advancing II. In this talk\, I will present simulated results for stellar systems within the framework of the La Palma Quantum Interferometry (LPQI) initiative. These simulations focus on identifying promising stellar targets and assessing achievable signal-to-noise ratios. The results demonstrate the potential to resolve binary systems at micro-arcsecond scales\, enabling precise measurements of stellar radii and orbital parameters in close massive binaries\, modeling Roche-lobe geometries in Wolf–Rayet systems\, and establishing the foundation for exoplanet astrometry in stellar systems\, where traditional detection methods are often limited. \nFecha y lugar: 15/12/2025 – 13:00 | Salón de ActosNitu RaiAryabhatta Research Institute of Observational Sciences (ARIES)\, Nainital \n  \n 
URL:https://www.iaa.csic.es/evento/simulations-to-unlock-micro-arcsecond-astronomy-with-la-palma-quantum-interferometry-lpqi/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20251216T130000
DTEND;TZID=Europe/Paris:20251216T133000
DTSTAMP:20260406T095255
CREATED:20251103T085904Z
LAST-MODIFIED:20251118T091359Z
UID:27989-1765890000-1765891800@www.iaa.csic.es
SUMMARY:KM3-230213A: the ultra-high-energy neutrino detected in KM3NeT
DESCRIPTION:The detection by the KM3NeT neutrino telescope of the ultra-high-energy event KM3-230213A is a milestone in neutrino astrophysics. With an energy estimated of about 220 PeV\, it is the most energetic neutrino observed to date\, challenging the current understanding of the cosmic spectrum. Its observation opens the question of its astrophysical origin. \nIn this talk\, details on the KM3-230213A detection and observed signature will be presented\, describing the detection technique and significance assessment. Possible astrophysical sources\, including extragalactic and cosmogenic origins\, will be discussed. \nFecha y lugar: 16/12/2025 – 13:00 | Salón de ActosSergio Navas ConchaUniversidad de Granada \n 
URL:https://www.iaa.csic.es/evento/km3-230213a-the-ultra-high-energy-neutrino-detected-in-km3net/
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:20251218T190000
DTEND;TZID=Europe/Paris:20251218T200000
DTSTAMP:20260406T095256
CREATED:20251212T151315Z
LAST-MODIFIED:20251215T145839Z
UID:28976-1766084400-1766088000@www.iaa.csic.es
SUMMARY:Darwin y las galaxias
DESCRIPTION:Darwin fue uno de los mayores revolucionarios del pensamiento humano. Su teoría sobre el origen de las especies supuso un auténtico revulsivo intelectual\, culminando la herencia del pensamiento ilustrado y generando consecuencias que aún sentimos hoy. \nVivió 80 años durante el siglo XIX\, siendo testigo privilegiado de la era Victoriana y del notable desarrollo científico que tuvo lugar en Europa\, especialmente en el Reino Unido. Fue contemporáneo de la transformación de la astronomía en astrofísica y admiró a grandes astrónomos de su tiempo. Pero\, ¿qué relación tuvo Darwin con esta ciencia? Y más allá\, ¿puede existir algún paralelismo entre la evolución de las especies y la de los objetos celestes? \nEsta charla propone un fascinante paseo por la “ciencia evolutiva” del universo\, explorando la idea de las especies astronómicas. \nFecha:18/12/2025 – 19:00Conferenciante:  Emilio J. AlfaroFiliación:  Instituto de Astrofísica de Andalucía (IAA-CSIC) \n 
URL:https://www.iaa.csic.es/evento/darwin-y-las-galaxias/
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/2025/12/lucas-lara.jpg
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