Calendario de conferencias y eventos
1 - 100 de un total de 1784
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08/04/2025 - 12:30
On radiative transport models in protoplanetary discs TBP Dr. Miguel Jáquez |
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27/03/2025 - 19:00
Ciencia en palabras Peter Brook, uno de los directores más influyentes del teatro contemporáneo, decía que “lo inesperado no tiene límites”. Y así es. Por ejemplo, se puede encontrar la ciencia en lugares inesperados, como los discursos de ingreso de la Real Academia Española (RAE). Estos textos son ensayos muy concretos sobre un tema y, también, son una instantánea de la sociedad, del arte y de la ciencia en diferentes contextos... Sara Cazzoli |
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01/04/2025 - 12:30
A Minion in PANIC arrives to Calar Alto Observatory Calar Alto has a new tenant: PANIC, the PAnoramic Near-Infrared Camera for Calar Alto. PANIC is a project jointly developed by the MPIA in Heidelberg, Germany, and the IAA in Granada, Spain, for the Calar Alto Observatory (CAHA; Almería, Spain). This instrument can work with the 2.2 m and 3.5 m telescopes. Its original detector has been recently replaced by a monolithic HAWAII-4RG, therefore the instrument covers now a field of view of 26×26... Ana Guijarro, Vianak Naranjo, Antonio J. García, José M. Ibáñez and Sara Muñoz |
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29/05/2025 - 12:30
Pevatrons and ultra-high energy cosmic rays as messengers of extreme astrophysical plasma TBP Dra Anabella Araudo |
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31/12/2025 - 12:30
Tolerancia CERO de la teoría a la práctica TBP Ana María Orejas Brasero y Mª Carmen Artuñedo Esteban |
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24/04/2025 - 12:30
SO colloquium: The formation of high-altitude clouds on the terrestrial planets TBP Dr. Anni Määttänen |
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01/01/2025 - 09:15
TBP TBP TBP |
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03/04/2025 - 12:30
Phase curve fitting in the context of large-scale photometric surveys Nowadays, we are experiencing a revolution in astronomical surveys. Thanks to ground-based and orbiting telescopes, millions of observations of asteroids in various photometric filters are available. The main objective of our project is to develop tools for reading, processing, and analyzing large volumes of data. We’ve successfully determined phase curves for thousands of asteroids in orange and cyan filters from the latest ATLAS Solar System... Dr. Milagros Colazo |
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27/03/2025 - 12:30
What Stops Star Formation in Isolated Dwarf Galaxies in the Most Underdense Cosmic Regions? The shallow potential wells of low-mass galaxies, commonly known as dwarf galaxies, make them highly susceptible to environmental effects, often leading to the complete cessation of star formation. But is quenching solely driven by external forces in harsh environments, or can dwarf galaxies also self-quench through mechanisms like strong stellar winds or supernova feedback, independent of external influences? In this contribution, I present our... Dr. Bahar Bidaran |
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27/02/2025 - 19:00
Ceres como laboratorio natural. Claves orgánicas desde el cinturón de asteroides 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. Estudios recientes han identificado nuevas regiones con indicios de compuestos orgánicos adicionales, ampliando nuestra comprensión de este fascinante mundo. Durante la charla, exploraremos qué hace de Ceres un objeto tan relevante, profundizando en los... Juan Luis Rizos |
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11/02/2025
Día Internacional de la Mujer y la Niña en la Ciencia 2025 El Instituto de Astrofísica de Andalucía se suma un año más a la celebración del Día Internacional de la Mujer y la Niña en la Ciencia, que tiene como objetivo visibilizar la labor científica de las mujeres y fomentar las vocaciones en las niñas |
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23/06/2025 - 27/06/2025
International Summer School on Advanced Black Hole Physics 'Tales of Black Holes' Granada |
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27/01/2025
Puentes de Ciencia: La investigación como herramienta de unión cultural «Puentes de Ciencia» es un programa de divulgación científica inclusiva que busca acercar la investigación realizada en los centros del CSIC en Granada y el Instituto DaSCI de la Universidad de Granada a colectivos en riesgo de exclusión social |
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27/01/2025
El IAA se suma a la décima edición de Desgranando Ciencia: un encuentro con historia, ciencia, humor y arte El festival de divulgación granadino conmemora sus diez años bajo el lema “Historia(s) de la Ciencia”, los días 16 y 17 de mayo en el Parque de la Ciencias El evento, de acceso gratuito, también celebrará los aniversarios de algunas de sus entidades colaboradoras: los 30 años del Parque de las Ciencias, los 50 del Instituto de Astrofísica de Andalucía y los 70 de la Estación Experimental del Zaidín |
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11/02/2025 - 12:30
An Unusual Triple System: CN Lyn 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... Dr. Gökhan Yücel |
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11/03/2025 - 12:30
J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z < 5 In this talk, I will present J-HERTz, the J-PLUS Heritage Exploration of Radio Targets at z... David Fernández Gil |
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10/04/2025 - 12:30
TBP TBP Dr. John Plane |
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26/02/2025 - 12:30
ORCA-TWIN: Fast & low read noise CMOS camera project for planetary science and astrophysics 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... Dr. Martin M. Roth |
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05/05/2025 - 08/05/2025
SO-IAA School on Bayesian Statistics Granada |
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25/02/2025 - 12:30
Chemical Fingerprints of Galaxy Evolution I will summarise the main projects we are currently working on that use the chemical abundances and pattern as fossil records of galaxy evolution. In 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... Dr. Patricia B. Tissera |
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03/02/2025 - 20/02/2025
Element Abundances and the Chemical Evolution of the Cosmos Granada |
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06/03/2025 - 12:30
SO Colloquium: Gravitational wave astrometry with the SKAO 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.... Dr. Nicola Bellomo |
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30/01/2025 - 19:00
La Tierra que acunó la vida: el papel de la sílice 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. Desvelaremos el papel crucial de los minerales, en especial de la sílice, en la autoorganización mineral y en la... Juan Manuel García-Ruiz |
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19/12/2024 - 19:00
¿Qué sabemos de nuestra Galaxia después de Gaia? 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... Emilio J. Alfaro |
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12/12/2024 - 12/12/2024
PySnack 10: PROSE Granada |
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21/01/2025 - 30/10/2025
Academic Spanish Course for Foreigners (2025) Granada |
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19/05/2025 - 23/05/2025
II Advanced School on Galaxy Evolution Granada |
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30/01/2025 - 12:30
SO Colloquium: Modelling of large-scale magnetic field in low-mass stars 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... Dr. Anna Guseva |
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28/01/2025 - 12:30
El crecimiento de la complejidad en el Universo 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... Dr. Eduardo Battaner |
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23/01/2025 - 12:30
Study of the very high energy emission from star-forming regions and young massive star clusters 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... Dr. Gaia Verna |
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31/01/2025 - 12:30
Resolving Stellar Angular Diameters with Asteroid Occultations 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... Joshua Bartkoske |
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28/11/2024 - 19:00
Sobre supernovas, agujeros negros y cinturones de radiación en enanas marrones En 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. Jon Marcaide |
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02/12/2024 - 02/12/2024
PySnack 9: GASTLI Granada |
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31/10/2024 - 31/10/2024
PySnacks 8: PyBDSF Granada |
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03/12/2024 - 12:30
Experimental ice simulations for the interpretation of ice and organics observations in the Solar System 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... Dr. Guillermo Muñoz Caro |
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12/12/2024 - 12:30
Informative Session for Foreign New Hires If you are a foreigner who has recently joined the IAA and haven 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. Lauren C. Smith |
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25/11/2024 - 25/11/2024
Introduction to GitHub Granada |
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16/10/2024 - 20/10/2024
Seventh Workshop on Robotic Autonomous Observatories Torremolinos |
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10/12/2024 - 12:30
ESERO, from space to the classroom 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... Dr. Manuel González |
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31/10/2024 - 19:00
Impacto de los Metales Antropogénicos en la Atmósfera: Desafíos y Estrategias en la Era de las Megaconstelaciones En las próximas décadas se espera un incremento significativo en el número de satélites en la órbita baja terrestre, principalmente impulsado por el crecimiento de las megaconstelaciones de telecomunicaciones de banda ancha. La estrategia de 'cero residuos' de las agencias espaciales busca evitar la generación de grandes cantidades de basura espacial mediante la desintegración programada de vehículos usados y satélites inactivos en la atmósfera... Juan Carlos Gómez Martín |
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14/11/2024 - 12:30
Ozone and the Search for Life in the Universe 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... Dr. Thea Kozakis |
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06/02/2025 - 12:30
Equality and harrassment in the CSIC. A case of study: IAA 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. Dr. Josefa Masegosa Gallego |
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04/10/2024
El Universo desde Sevilla III Esta 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. |
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03/10/2024
Un congreso debatirá sobre las implicaciones de la astrofotografía en investigación y divulgación El Congreso Astrofotografía 2024 se celebrará en el Rectorado de la UCO del 4 al 6 de octubre El Instituto de Astrofísica de Andalucía (IAA-CSIC) es patrocinador y forma parte del comité organizador local (LOC) |
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31/10/2024 - 12:30
Using CHEOPS to confirm small transiting exoplanets orbiting bright stars Exoplanets which transit their host stars are unique in allowing detailed characterisation of planetary radius, mass and atmospheric properties. NASA's TESS mission, which has so far observed 97% of the sky with precise photometry, is especially adept at detecting small transiting planets orbiting the brightest... Dr. Hugh Osborn |
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15/05/2025 - 12:30
SO Colloquium: Bursting and cool slowly rotating stellar zombies The large efforts put into studying the transient Universe in the past years allowed the discovery of a variety of new astrophysical classes and events, many of them proposed to be related to the formation of a neutron star or a magnetar, the most magnetic pulsars. Pulsars are unique astronomical laboratories where the most extreme gravity and electromagnetism can be probed. The study of these objects transcends the traditional astrophysical... Dr. Nanda Rea |
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06/11/2024 - 12:30
New UGR proceedings for PhDs 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. Dr. Antonio García Hernández |
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24/10/2024 - 12:30
SO colloquium: Role of Astrophotonics in Astronomy: The MARCOT Pathfinder Dr. Kalaga Venu Madhav, a renowned astrophysicist from the Leibniz Institute for Astrophysics Potsdam, will present a colloquium on the role of astrophotonics in astronomy, focusing on the MARCOT Pathfinder project. The talk will cover advancements in astrophotonic technologies and their applications in modern astronomical instrumentation. Dr. Madhav will discuss the development and implementation of photonic devices in telescopes, their impact... Dr. Kalaga Madhav |
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21/11/2024 - 12:30
Towards the Standardization of the Modeling of Multi-Frequency Observations 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... Dra. Mireia Nievas Rosillo |
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23/09/2024
La Noche Europea de l@s Investigador@s llega con 300 actividades para hacer la ciencia más cercana y social El IAA-CSIC participa con talleres, charlas y una mesa de realidad virtual en un stand propio en el Paseo del Salón |
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13/09/2024
La Noche de l@s Investigador@s 2024 Tenéis cita con la Noche Europea de l@s Investigador@s el 27 de septiembre en Granada, en el Stand del IAA-CSIC en el Paseo del Salón. |
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26/11/2024 - 28/11/2024
3rd edition of the HONEST Workshops: The high energy end of pulsar spectra |
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27/09/2024 - 12:30
Who Is Afraid of the Dark (Energy)? Cosmic acceleration dominates the behavior of the recent universe, with some fundamentally new physics at its heart. Recent data gives a tantalizing suggestion that the dark energy behind it is more complicated than a cosmological constant. Nevertheless, we do know a lot about how to describe dark energy behavior. Data within the next year has great promise to give further insight, and exciting new instruments are being planned. Dr. Eric Linder |
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10/10/2024 - 12:30
Uncovering the magnetized path of massive star formation Both observational and theoretical studies suggest that the magnetic field plays an important role in the process of massive star and cluster formation. However, many open questions still remain, including the exact role of B-field at the different scales (from cloud to disk scales) and its importance compared to turbulence, feedback and self-gravity. Multi-scale studies of the morphology and strength of the magnetic field are thus crucial to... Dr. Chi Yan (Paul) Law |
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17/10/2024 - 12:30
SO Colloquium: Radio eyes for the Sun, Heliosphere and Ionosphere: Status and plans for the SKAO era The Square Kilometre Array Observatory (SKAO) represents a monumental leap in radio astronomy technology, promising to redefine our understanding of the universe through its unprecedented capabilities. As we stand on the brink of the SKAO era, this talk aims to elucidate the transformative potential of SKAO for solar physics, heliospheric, and ionospheric research. The SKAO's advanced radio telescopes, with their superior angular, spectral, and... Dr. Pietro Zucca |
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13/02/2025 - 12:30
SO Colloquium: Present and future of exoplanet research 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... Dr. Ignasi Ribas |
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28/11/2024 - 12:30
SO Colloquium: Cosmic chemical evolution: here, there, and everywhere 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... Profa. Ángeles Díaz |
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26/09/2024 - 11:00
The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collisionless cold dark matter paradigm Unraveling the nature of dark matter (DM) stands as a primary objective in modern physics. I will present evidence suggesting deviations from the collisionless Cold DM (CDM) paradigm. In the standard cosmological model the dark matter (DM) particles are collisionless and, because of this very nature, they develop halos with the characteristic central cusp known as NFW profile. Real galaxies do not show NFW profiles but, rather, have a DM mass... Dr. Jorge Sánchez Almeida |
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15/07/2024 - 19/07/2024
XVI Reunión Científica de la Sociedad Española de Astronomía Granada |
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04/11/2024 - 08/11/2024
Writing and Communicating your Science - an IAA-CSIC Severo Ochoa Workshop Granada |
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17/07/2024
Astronomía “Made in Spain" En el marco de la XVI Reunión Científica de la SEA (15-19 de julio), el IAA-CSIC ha organizado este evento |
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25/06/2024
LGTBIQ+ ROUND TABLE: towards a more diverse and inclusive research Con motivo del Día Internacional del Orgullo LGBT, la Comisión de Igualdad, Diversidad e Inclusión del IAA-CSIC organizó el 25 de junio la mesa redonda "LGTBIQ+ ROUND TABLE: towards a more diverse and inclusive research" |
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24/09/2024 - 12:30
Constraining the Meteoroid Flux in the inner solar system The inner solar system is populated by Interplanetary Dust Particles (IDPs) released from cometary trails and collisions between asteroids. Planetary bodies and satellites therefore encounter a cloud of IDPs along their orbits, giving rise to a permanent bombardment on their respective atmospheres or surfaces. Constraining the magnitude of the mass influx of IDPs onto a solar system body is crucial for understanding the effects in their... Dr. Juan Diego Carrillo Sánchez |
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20/06/2024
Mujer en la Ingeniería: Avances y Retos La Comisión de Igualdad, Diversidad e Inclusión del IAA-CSIC, con motivo del Día Internacional de las Mujeres en la Ingeniería (23 de Junio), ha organizado la conferencia “Mujer en la Ingeniería: Avances y Retos”, a cargo de Laura M. Roa, catedrática de Ingeniería de Sistemas y Automática de la Universidad de Sevilla |
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23/07/2024 - 12:30
The QUIJOTE experiment: status, latest results and future plans I will review the current status and future plans of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a project with the aim of characterising the polarisation of the Cosmic Microwave Background, and other galactic or extragalactic physical processes that emit in microwaves in the frequency range 10-42GHz, and at large angular scales (1 degree resolution). The project has two radio telescopes (2.25m primary aperture) and three instruments, MFI (10... Dr. José Alberto Rubiño Martín |
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27/06/2024 - 19:00
Más allá del sistema solar: el fascinante universo de los exoplanetas La búsqueda de exoplanetas, aquellos planetas que están fuera de nuestro sistema solar, ha revolucionado nuestra comprensión del universo y de nuestro lugar en él. Desde el descubrimiento del primer exoplaneta orbitando una estrella tipo solar en 1995, la astronomía ha experimentado un renacimiento tecnológico y teórico que ha permitido identificar miles de estos mundos alienígenas. En esta charla, exploraremos el fascinante campo de la... Francisco Pozuelos |
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30/09/2024 - 13:00
High-Resolution Study of Blazar TXS 2013+370 and BEAM: A Space Technology and Research Student Team The talk will focus on two key areas. Part one will present the high-resolution imaging of Blazar TXS 2013+370, a study conducted as part of an M.Sc. thesis. This research aims to resolve the inner jet structure of the compact radio source TXS 2013+370 in total intensity and polarization. This analysis utilizes VLBA data combined with Effelsberg observations at frequencies of 22 GHz, 43 GHz, and 86 GHz. Part two will highlight BEAM, a student... Giorgos Michailidis |
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10/06/2024
Bajo un mismo cielo Actividad realizada conjuntamente con tres ONG: Acción en red; Granada Acoge y Provivienda |
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20/06/2024 - 12:00
Mujer en la Ingeniería: Avances y Retos En esta conferencia presentaremos, en primer lugar, una panorámica de la situación actual de la mujer en las STEM y en particular en la ingeniería, tratando de analizar qué factores pueden tener una mayor influencia en la situación actual. A continuación trataremos brevemente la educación de la mujer en los dos últimos siglos. Destacaremos el hecho de como las formas de educar a la mujer están directamente relacionadas con el trabajo que... Dr. Laura Roa |
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27/06/2024 - 12:30
Multiple components in the protostellar system HH 212: Infalling envelope, nested shell, MHD disk winds, and free wind gas I will present the Atacama Large Millimeter/submillimeter Array Band 7 observations at ~24 au spatial resolution of the CO (J=3-2) and H13CO molecular lines emission of the protostellar system HH 212 and compare them with the emission of the SiO (J=8-7) and SO (J=8-7) molecular lines. From the large to small scale, previous observations have detected the infalling envelope, CO outflow shell, SO disk wind, SiO expanding shell and jet in the... Dr. Alejandro López-Vázquez |
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25/06/2024 - 11:00
Intersexionality, a key work for diversity? Since we are children we have been taught what we are and we learn how to fit into a set of infinite boxes. Each of these boxes defines us and, at the same time, can be used to discriminate against us, in life and at work. Diversity exists and it could be an advantage for our society. As scientists we should understand how to take care of diversity and use it to improve our work and life quality. One of the main problems in the past has been... Dr. Eleonora Fiorellino |
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23/05/2024 - 19:00
Acerca de la Cosmología La Cosmología como ciencia empírica comenzó en los años 20 del pasado siglo. Desde entonces varios hitos observacionales han inspirado y sostenido el mejor modelo cosmológico que nos hemos podido dar. Sin embargo la materia y la energía oscura, la masa de los neutrinos, y otros nuevos datos observacionales nos obligan a replantearnos algunas preguntas y explorar, quizás, otras aproximaciones a la pregunta de cómo se formó y evoluciona... Mariano Moles |
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06/05/2024
El festival Pint of Science organiza 18 charlas de divulgación científica en los bares de Granada El festival internacional de divulgación científica se celebrará los días 13, 14 y 15 de mayo en toda España, con entrada gratuita En Granada, Pint of Science se celebrará en los bares La Tertulia, Lemon Rock y Sala Premier El programa completo puede consultarse en https://pintofscience.es/events/granada |
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06/06/2024 - 12:30
A complex network perspective on Delta Scuti stars We apply horizontal visibility graphs (HVG) to study the complex network behavior for the delta Sct stars’ light curves observed by TESS. The delta Sct stars are pulsating stars with spectral types A0-F5 and intermediate masses between low-mass stars (≤ 1 Msun) and high-mass stars (≥ 2 Msun). They pulsate in low-order pressure modes and have dominant pulsation frequencies in the 5-80 d−1 range. The high amplitude delta Sct stars (called HADS),... Dr. Elham Ziaali |
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25/04/2024 - 19:00
La Inteligencia artificial ya ha entrado en nuestras vidas La conferencia tratará tres aspectos fundamentales de la multiplicidad prismática de la IA: a) no va a llegar, ya está aquí, con nosotros, desde hace tiempo; b) la IA generativa, ¿ayudante o sustituto?; y c) la eclosión de la IA, riesgos y regulación. Prof. Dr. Francisco Herrera |
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30/09/2024 - 04/10/2024
ERIS 2024 Tenth European Radio Interferometry School Granada |
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23/04/2024 - 18/06/2024
SO Training on Scientific Presentation in Astronomy Granada |
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21/03/2024 - 19:00
Explorando los misterios del Universo a través del viaje de los desconocidos Rayos Cósmicos Los rayos cósmicos -partículas cargadas ultrarrelativistas que bombardean la Tierra desde todas los puntos del cielo- son invisibles al ojo humano pero contienen información sobre los procesos más fundamentales del Universo, tales como su creación y evolución. Estas partículas se producen en los procesos más violentos del Universo y su observación directa no nos da información acerca de... Rubén López-Coto |
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17/06/2024 - 18/06/2024
PySnacks 7: sedcreator: the python package to build and fit spectral energy distributions Granada |
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12/03/2024 - 15/03/2024
ESA's Vigil PMI instrument kick-off consortium meeting Granada |
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12/03/2024
Espacio 3 organiza el primer “Micro Abierto” de Ciencia de Granada en la Sala Aliatar “Abierto por defecto, y ven a contar tus movidas” tendrá la idea de “Libertad” como hilo conductor del proyecto de Ciencias y Artes Escénicas que incorpora nuevos formatos en su cita de marzo |
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04/03/2024
8M: Día Internacional de la Mujer 2024 El Instituto de Astrofísica de Andalucía participa en la celebración del Día Internacional de la Mujer celebrando la mesa redonda "Vocaciones en áreas STEM: El caso de la Física" y participando en la organización del II Encuentro Científicas y Empresarias de Granada |
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11/07/2024 - 12:30
Dust in protoplanetary disks, (still) that great unknown Planetary systems are a side effect in the formation of a star. Planets are believed to be just simply the last remaining of dusty circumstellar disks which is formed around the protostar at very early stages. Thus, understanding how planets are formed requires to understand how dust evolve in these disks. It is less than ten years that we have the possibility of mapping the dust distribution in protoplanetary disks with great detail with... Carlos Carrasco González |
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14/05/2024 - 12:30
New possibilities for atmospheric analysis with Monte Carlo In recent years, significant advancements have been made in scientific computing utilizing the Monte Carlo method, particularly at the intersection of two key communities: the heat transfer community and the computer graphics community. The first breakthrough is that the computation time required to solve radiative transfer becomes invariant, whether the ground is described by a single building or thousands of them, whether the 3D clouds are... Dr. Yannis Inouk Nyffenegger Péré |
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30/04/2024 - 12:30
The art of astrophysical measurements: An elementary lecture on photon counting and S/N Have you ever dared to understand how many photons are detected by your camera when you are pointing the telescope to the sky? Is the action of the spectrograph fully understood when analyzing those photons? Do typical image formation rules hold when studying the polarization of light? All these are a few examples of questions addressed by researchers when designing instruments, which are later constrained by technological capabilities. This... Dr. José Carlos del Toro Iniesta |
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11/04/2024 - 12:30
LP791-18d as a case study for outgassing rocky exoplanets Over the past three decades, the discovery of over five thousand exoplanets has opened avenues for atmospheric characterization, now feasible for a select subset through spectroscopic observations paired with Bayesian inference techniques. These exoplanetary atmospheres serve as crucial windows into planetary formation and evolutionary histories. Achieving accurate interpretations demands a comprehensive approach, advancing theory and modeling... Dr. Leonardos Gkouvelis |
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04/04/2024 - 12:30
The Earthbound Fate of Meteor Phenomena Understanding meteor phenomena is essential for promptly and effectively recovering meteorites, predicting meteor showers, studying atmospheric properties, and assessing the threat posed by space objects to both in-orbit and ground-based infrastructure. By observing and interpreting meteor phenomena, we can predict impact consequences and efficiently locate and identify surviving meteorite fragments on the ground. Through dimensional analysis,... Dr. Maria Gritsevich |
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22/02/2024 - 19:00
Ciencia abierta y la crisis de la reproducibilidad La ciencia es una fantástica y gigantesca empresa humana en la que se estima que están implicadas mas de nueve millones de personas y en la que actualmente se invierte en el mundo más de un billón y medio de euros anualmente. El método científico es el instrumento que ha caracterizado a la ciencia para alcanzar su objetivo de conocer y comprender el mundo natural que nos rodea. Emilio Sánchez-Cantalejo |
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04/03/2024 - 05/03/2024
PySnacks 6: pyFIT3D/pyPipe3D: Resolved Properties of Stellar Populations and Ionized Gas with Galaxy IFS Data Granada |
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25/04/2024 - 12:30
Artificial Intelligence in Service of Galaxy Evolution Research: A Personal Journey In this seminar, I will present my personal exploration of the application of artificial intelligence in the study of galaxy evolution. Since the early 2010s, the fields of machine learning and deep learning have undergone unprecedented development, marked by enhancements in algorithms and hardware advancements. This progress has significantly influenced various scientific domains. Concurrently, the increasing volume and complexity of data... Dr. Ginés Martínez Solaeche |
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31/01/2024
Día Internacional de la Mujer y la Niña en la Ciencia 2024 El Instituto de Astrofísica de Andalucía se suma un año más a la celebración del Día Internacional de la Mujer y la Niña en la Ciencia, que tiene como objetivo visibilizar la labor científica de las mujeres y fomentar las vocaciones en las niñas |
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27/02/2024 - 12:30
Unraveling the Gamma-ray emission in radiogalaxies and their jets Radio-galaxies are a minority among all extragalactic sources detected in gamma-rays, yet they have excellent potential to study particle acceleration and non-thermal emission in AGN jets. In contrast with blazars, which have jets aligned with the line-of-sight, radio-galaxies have a smaller Doppler boosting factors. The implications are important: First, the distance at which they are detectable in gamma-rays is smaller. Second, the thermal... Mireia Nievas Rosillo |
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24/01/2024 - 24/01/2024
Cosmic Dust Workshop Granada |
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21/05/2024 - 12:30
Coloquio SO: Spectroscopy's Role in Stellar Astrophysics To characterize a star, the stellar fundamental parameters such as mass, radius, metal abundance, and effective temperature should be known. Direct measurements of these parameters, especially for single stars, are quite challenging, and indirect methods are often employed to obtain these characteristics. The most effective method for determining these parameters is spectroscopy, which is an analysis technique of spectra. It allows us to... Dr. Filiz Kahraman Aliçavuş |
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09/04/2024 - 12:30
Laboratory Research on the Atmospheric Impact of Spacecraft Re-entry Debris: Perspectives and Future Challenges The rapid growth of space debris, especially in Low Earth Orbit (LEO), poses a rising risk to both space operations and Earth's atmosphere. Debris fragments, even minuscule in size, can cause significant damage due to their high orbital speeds. To mitigate risks, controlled re-entry of debris is common practice, but this introduces a new concern: the increasing mass of human-made materials injected into the atmosphere. As satellites and rocket... Dr. Antonio Ocaña |
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07/03/2024 - 12:30
SO colloquium: Stars and their close-by planets: clues of magnetic interactions Stars interact with their close-in planets through the gravitational and magnetic fields and with their radiation. After a general introduction to those interactions, I shall review some observational clues of magnetic star-planet interactions considering data obtained in the optical, X-ray, and radio domains. Based on a stellar force-free coronal field or the excitation of Alfven waves by an orbiting planet, some analytical models will be... Dr. Antonino Francesco Lanza |
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21/03/2024 - 12:30
The Local Volume Mapper, state of the art The LVM, one of the three surveys that conform the SDSS-V project, is the first Integral Field Spectroscopy survey of the Local Group, including and unique mapping of the Milky Way. It started survey operations in October 2023, with some early science observations on cheery-peaked targets, and the first observations on the foreseen survey itself. I present here the status of the survey, including the state of the major contributions from the IA... Dr. Sebastián Sánchez |
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14/03/2024 - 12:30
SO Colloquium: Spatially resolved spectroscopy properties of low-redshift galaxies We summarize here some of the results reviewed recently by Sanchez (2020) and Sanchez et al. (2021) comprising the advances in the comprehension of galaxies in the nearby universe based on integral field spectroscopic galaxy surveys. We review our current knowledge of the spatially resolved spectroscopic properties of low-redshift star-forming galaxies (and their retired counterparts) using results from the most recent optical integral field... Dr. Sebastián Sánchez |
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19/02/2024 - 23/02/2024
English for Academic Purposes Granada |
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19/03/2024 - 16:30
Recent Progress in Understanding Solar Flare Magnetism using Data-Driven Simulations and Statistical Analysis of Vector Magnetic Fields Continuous vector magnetic-field measurements by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) allowed us to run data-driven simulations of solar eruptions and perform statistical studies of magnetic-fields for many flares. In this talk I will review new aspects of flare magnetism discovered using SDO data, including progress in data-driven simulations and statistical studies of magnetic-reconnection... Dr. María Kazachenko |