Calendario de conferencias y eventos
1 - 100 de un total de 1642
Pages
|
28/06/2023 - 12:30
Seminario día orgullo TBP TBP |
|
28/09/2023 - 12:30
Revealing Massive Star Formation through NIR Interferometry TBP Dr. Maria Koutoulaki |
|
02/11/2023 - 12:30
SO colloquium: A new digitized age of SETI – interferometric commensal observations and machine learning The search for technosignatures - remotely observable indicators of advanced extraterrestrial life - addresses one of the most profound questions in science: are we alone in the universe as intelligent life? The Breakthrough Listen program is leading the most concerted search for extraterrestrial intelligence (SETI) effort to-date through radio and optical surveys of nearby stars, nearby galaxies and the Milky Way galactic plane, thus... Dr. Cherry Ng |
|
20/07/2023 - 12:30
Near-Infrared Observations of Massive Protostellar Outflows TBP Sam Crowe |
|
06/06/2023 - 12:30
Aperture Masking Interferometry with the JWST In this talk, I will present how the aperture masking interferometric (AMI) mode of the JWST works. I will describe the main characteristics of this mode. In particular, I will show some of the advantages of the mode complementary to standard imaging and coronagraphic observations. I will also introduce the basic principles of the AMI data analysis, including the extraction of the interferometric observables and their interpretation with... Dr. Joel Sanchez Bermudez |
|
13/07/2023 - 10:45
Seminario física solar TBP Dr. Teresa Nieves Chinchilla |
|
22/05/2023
Exploración espacial de Marte y Venus - Gabriella Gilli y Francisco González Galindo El día 22 de Mayo a las 20:00h, Gabriella Gilli y Francisco González Galindo, ambos del Instituto de Astrofísica de Andalucía (IAA-CSIC), dieron una conferencia de divulgación en el Palacio de La Madraza titulada "Exploración espacial de Marte y Venus". |
|
24/05/2023 - 26/05/2023
https://sites.google.com/view/qftcsworkshop2023/home Granada |
|
25/05/2023 - 19:00
¿Agujeros negros o estrellas negras? Un diálogo galileano Los agujeros negros parecen ser el resultado ineludible del colapso gravitatorio, el estadio final de la evolución estelar Julio Arrechea y Carlos Barceló |
|
15/05/2023 - 19/05/2023
https://www.granadacongresos.com/els2023 Almuñecar |
|
09/11/2023 - 12:30
NO IN-PERSON SEMINAR/COLLOQUIUM Salón de actos ocupado N/A |
|
21/06/2023 - 21/06/2023
https://docs.google.com/forms/d/e/1FAIpQLSf3LCWdpRFmz0JVl9GtG52KDRaGLKNEEw674XWk… Granada |
|
21/12/2023 - 12:30
Confirmation of the standard cosmological model from red massive galaxies ∼ 600 Myr after the Big Bang In their recent study, Labbe ́ et al. used multi-band infrared images captured by the James Webb Space Telescope (JWST) to discover a population of red massive galaxies that formed approximately 600 million years after the Big Bang. The authors reported an extraordinarily large density of these galaxies, with stellar masses exceeding 1e10 solar masses, which, if confirmed, challenges the standard cosmological model as suggested by recent studies... Dr. Francisco Prada |
|
16/05/2023 - 12:00
Seminario Centro de Cálculo Nueva infraestructura de cálculo del IAA Centro de Cálculo |
|
24/04/2023 - 28/04/2023
https://www.granadacongresos.com/ctac-ctao Granada |
|
24/04/2023 - 28/04/2023
https://www.granadacongresos.com/gcw2023 Granada |
|
20/04/2023
El premio Nobel Reinhard Genzel repasa en Granada los principales hallazgos sobre agujeros negros El Instituto de Astrofísica de Andalucía (IAA-CSIC) organiza una conferencia de Reinhard Genzel, que obtuvo el premio Nobel de Física en 2020 por el descubrimiento del agujero negro del centro de la Vía Láctea. La sesión, con entrada libre hasta completar aforo, tendrá lugar en el auditorio del Parque de las Ciencias el lunes 24 de abril a las 19:30 h |
|
25/04/2023 - 12:30
SO colloquio: Theoretical models for the formation and evolution of Ultra-Cool Dwarf planetary systems Rocky planets located in the habitable zones around very low-mass objects are ideal targets for searching for life outside our Solar System. In order to better understand their formation and evolution, N-body simulations are needed. These simulations are developed assuming a star close to the substellar mass limit as the central object. The simulations include tidal and general relativistic effects that incorporate the contraction and evolution... Dr. Mariana Sánchez |
|
11/05/2023 - 12:30
Off-centre supermassive black holes in bright central galaxies Supermassive black holes (SMBHs) are believed to reside at the centre of massive galaxies such as brightest cluster galaxies (BCGs), the most massive galaxies which can be found in today's Universe. However, as BCGs experienced numerous galaxy mergers throughout their history, the central BH can be significantly kicked from the central region by these dynamical encounters. By combining the Illustris-TNG300 simulations and orbital integration... Dr. Aline Chu |
|
13/04/2023
El Futuro de la Astrofísica de muy altas energías a través del Open Science: Oportunidades con el Cherenkov Telescope Array Observatory (CTAO) “El Futuro de la Astrofísica de muy altas energías a través del Open Science: Oportunidades con el Cherenkov Telescope Array Observatory (CTAO)” El evento, que busca explorar la ciencia abierta y hablar de las oportunidades que ofrece el CTAO, se celebrará en el Salón de Actos del IAA-CSIC (Granada) el día 27 de abril de 2023 |
|
05/10/2023 - 12:30
SO colloquio: A Light in the Dark - Massive Star Birth Through Cosmic Time Massive stars are important throughout the universe, but their formation remains poorly understood. I review current understanding of how massive stars form in our Galaxy, in particular examining observational tests of various predictions of Core Accretion and Competitive Accretion theories. Finally, I discuss how massive star formation may have been different in the very early universe and how the first stars may have become supermassive... Dr. Jonathan C. Tan |
|
01/06/2023 - 12:30
SO webloquio: The impact of stellar composition: from galactic chemical evolution to planet formation The characterization of solar-type stars is fundamental for various fields in astrophysics, including exoplanet detection and the chemical evolution of our Galaxy. In particular, the determination of chemical abundances for stars at different metallicities and ages provides us with a key insight on how and when the various chemical elements were formed within the Galaxy. The chemical trends observed in different parts of the Galaxy (thin disk,... Dr. Elisa Delgado Mena |
|
04/05/2023 - 12:30
SO colloquio: Pulsar astrophysics in the era of large surveys History tells us that with new telescopes and new data processing techniques come new discoveries and breakthroughs in pulsar astrophysics. Despite nearly 55 years since their discovery, fundamental open questions remain in almost all areas of research. Examples include the birth properties and environments, the magnetic field configuration and evolution, the interactions of the superfluid interior with the solid crust, the processes of... Dr. Aris Karastergiou |
|
30/03/2023 - 19:00
Lo que debemos a los astrónomos del Egipto antiguo: una perspectiva desde la ciencia y la cultura El Egipto antiguo fascina por sus monumentos y sus tesoros, y algunos de sus personajes figuran en el acervo colectivo. Sin embargo, en general, se ignora que Egipto también tuvo una contribución substancial a la ciencia, la astronomía incluida. Los filósofos griegos viajaban a Egipto en busca de sabiduría. Aquí analizaremos cómo un calendario gobernado por las inundaciones anuales del Nilo acabó convirtiéndose en el calendario que regula la... Juan Antonio Belmonte |
|
28/03/2023 - 12:30
International Asteroid Impact Defense Collaboration The defense of our planet against asteroid impacts counts on international collaboration. NASA's OSIRIS-REx and Japan's Hyabusa2 spacecraft studied two potentially hazardous asteroids Bennu & Ryugu and bring samples back to Earth. NASA's DART, Italy's LICIACube and ESA's Hera spacecraft test a method of planetary defense against asteroids. Dr. Humberto Campins |
|
16/03/2023
Finaliza la visita al IAA-CSIC de su Comité Científico Asesor Externo (ESAB) Durante los días 14 y 16 de marzo se ha desarrollado la visita a las instalaciones del IAA-CSIC por parte del Comité Científico Asesor Externo (ESAB), compuesto por investigadores e investigadoras de reconocido prestigio internacional cuyo principal objetivo es revisar las actividades del IAA y proporcionar asesoramiento en acciones futuras. |
|
13/03/2023
Los premios ‘Granada, Ciudad de la Ciencia y la Innovación 2022’ El Ayuntamiento de Granada reconoce con los premios ‘Granada, Ciudad de la Ciencia y la Innovación 2022’ el esfuerzo y la aportación de la comunidad científica granadina en la consecución del proyecto de IFMIF-Dones. Destacamos a nuestros investigadores premiados, Ascensión del Olmo y Jose Luis Gomez, y la mención especial al granadino Rafael Rodrigo Montero, que fue director del Instituto de Astrofísica durante trece años. |
|
08/05/2023 - 10/05/2023
https://www.granadacongresos.com/skaopenscience Granada |
|
15/06/2023 - 12:30
Radio continuum halos in nearby galaxies and the CHANG-ES project About a decade ago, the upgrade from the classic Very Large Array into the EVLA, i.e. the Karl G. Jansky Very Large Array (VLA), made it possible to observe fainter radio continuum emission than ever before. The project Continuum Halos in Nearby Galaxies - an EVLA Survey (CHANG-ES, PI: J. Irwin) has allowed us to probe gaseous halos of 35 edge-on galaxies with arcsecond details and faint microJansky/beam sensitivities, and to begin answering... Theresa Wiegert |
|
03/03/2023
8M: Día Internacional de la Mujer 2023 El Instituto de Astrofísica de Andalucía participa en la celebración del Día Internacional de la Mujer a través de dos actividades: el "Primer Encuentro de Científicas y Empresarias de Granada" y la mesa redonda online "Igualdad y Sociedades Científicas" ... |
|
22/06/2023 - 12:30
SO colloquium: X-ray Polarimetry: a New Window to the Universe Polarimetry is a very important technique for understanding magnetic fields and high-energy processes in the Universe. While we have been studying polarization in the radio and optical side of the electromagnetic spectrum for decades, what happens at higher energies has, until recently, eluded us. In 2021 NASA finally launched the first X-ray polarimeter, the Imaging X-ray Polarimetry Explorer - IXPE, offering us a completely new window to the... Dr. Yannis Liodakis |
|
27/04/2023 - 12:00
El Futuro de la Astrofísica de muy altas energías a través del Open Science: Oportunidades con el Cherenkov Telescope Array Observatory (CTAO) El jueves 27 de abril a las 12:00 CEST, el Cherenkov Telescope Array Observatory (CTAO) y el Instituto de Astrofísica de Andalucía (IAA-CSIC) celebrarán un evento gratuito y abierto para investigadores interesados en la Ciencia Abierta y posibles sinergias con el CTAO, así como para estudiantes de grado, máster y doctorado que deseen desarrollarse profesionalmente en el campo de la Astrofísica de muy altas energías. El seminario, que tendrá... Dr. Roberta Zanin, Dr. Juan Cortina, Dr. Rubén López Coto y Dr. Francisco Colomer |
|
02/03/2023 - 12:30
J-PAS: a survey for tracing the role that star formation and environment play in galaxy evolution The processes that explain the evolution of galaxies from the blue cloud to the red sequence are still under discussion. Internal processes, named as mass-quenching, because they are linked to the galaxy mass or AGN feedback, could be responsible of the rapid quench of the star formation in galaxies. Besides the stellar mass, the evolution of the galaxy populations is also a function of the environment. Unlike the mass quenching, the... Dr. Rosa González Delgado |
|
04/10/2021 - 08/10/2021
http://apn8.iaa.csic.es Granada |
|
13/04/2023 - 12:30
Coloquio SO: A holistic approach to exoplanet spectroscopy During the last two decades, multiple observation techniques have enabled the study of exoplanet atmospheres, informing us about their chemical composition, thermal distribution and transport processes. The most successful techniques include low-resolution transit and eclipse spectroscopy, phase curves, and high-resolution Doppler spectroscopy. In all cases, the extraction of the atmospheric signal presents a challenge, being comparable to or... Guiseppe Morello |
|
07/03/2023 - 12:30
Sub-milliarcsecond astronomy with Imaging Atmospheric Cherenkov Telescopes The angular size of a star is a critical factor in determining its basic properties. Together with the distance, it provides the physical diameter of the star which can be used to yield luminosity and mass estimates. Direct measurement of stellar angular diameters is difficult: at interstellar distances stars are generally too small to resolve by any individual imaging telescope. This fundamental limitation can be overcome by several methods... Dr. Tarek Hassan |
|
21/04/2023 - 12:30
Gamma rays as cosmic ray tracers: how can CTAO contribute to the cosmic ray physics Gamma-ray emission produced by interactions of cosmic rays with interstellar matter and radiation fields is a probe of non-thermal particles in galaxies. After decades of instrumental improvements in the field of gamma-ray astronomy, different scales and environments are now accessible and their gamma-ray observations reveal several properties of cosmic rays, especially in our Galaxy. I will provide a short review of the status of the subject... Roberta Zanin |
|
23/03/2023 - 12:30
SO coloquio: Investigating the impact of quasar feedback on the central kiloparsecs of galaxies Active galactic nuclei (AGN) feedback is the effect that nuclear activity produces in the interstellar and circumgalactic medium of galaxies. Different modes of AGN feedback, which can be broadly divided into radiative/quasar and kinetic/radio, are now considered key processes in the evolution of massive galaxies by regulating black hole and galaxy growth. Indeed, a wealth of observational evidence demonstrates that feedback from supermassive... Dr. Cristina Ramos Almeida |
|
16/02/2023 - 12:00
School visit School visit Sara Garcia. |
|
16/03/2023 - 12:30
An observational study of massive star forming regions at radio wavelengths In their early stages, massive stars have a profound impact on their hosting cloud as reflected by signposts like shocks, bars and shells of swept material resulting from prominent stellar winds, or photo-ionized (HII) regions produced by energetic irradiance. This activity must be taken into account in the study of the mechanism of formation of either massive stars or nearby lower mass companions affected by such harsh conditions. It is known... Josep Maria Masqué |
|
09/03/2023 - 12:30
When accretion is as vital as extreme: from massive young stars to binary black holes Accretion is vital for understanding the properties of a number of astrophysical objects, including massive young stars and black holes. For the former, accretion drives the stellar mass growth and multiplicity through gas fragmentation. It also powers strong outflows that regulate the interstellar medium. For black holes, only accretion allows for electromagnetic detection. Hence, the multi-messenger astronomy, for which the loudest sources of... Dr. Raphael Mignon-Risse |
|
23/02/2023 - 19:00
Contaminación Lumínica: Cuando nuestras estrellas más cercanas no se ven entre ellas Conferencia de divulgación sobre las consecuencias del exceso de iluminación artificial nocturna. José Ramón Guzmán Alvarez |
|
23/02/2023 - 12:30
ALMA: Planned Sensitivity Upgrades, and Molecular Gas Imaging of a z=0.376 HI-Detected Galaxy This talk will cover two distinct topics in progress, one programmatic and the other science: I will first discuss the ALMA Wideband Sensitivity Upgrade (WSU), and then I'll talk about ALMA followup of the highest redshift HI detection in the COSMOS HI Large Extragalactic Survey (CHILES) made with the first 178 hours of observing. With regard to the WSU, the ALMA Project is embarking on a partner-wide initiative to at least double, and... Dr. Jennifer Donovan Meyer |
|
30/03/2023 - 12:30
Preparation and Asteroseismic exploitation of the PLATO Mission Thanks to ultra-precise space missions, we are living an era of big scientific discoveries in the stellar and planetary physics fields. PLATO will capitalise on the developments of successful past missions such as CoRoT, Kepler/K2, TESS and CHEOPS that studied stars and their planetary systems. PLATO will detect and characterise terrestrial exoplanets at orbits up to the habitable zone of solar-type stars. Transit measurements and... Dr. Javier Pascual |
|
25/01/2023
VI Meeting of AGN Research in Spain in the Era of the New Observatories Tras el éxito de las reuniones anteriores sobre AGNs convocadas en nuestro país, el IAA-CSIC acoge esta reunión, que permitirá revisar la comprensión actual en la investigación sobre AGNs |
|
26/01/2023 - 19:00
El cambio climático. Una puesta al día Revisamos el nuevo informe del Grupo Intergubernamental de Expertos sobre el Cambio Climático (IPCC) Rainer Schödel |
|
30/01/2023 - 12:30
SO Coloquio: Dirty Dancing: piercing the dusty environment of merging supermassive black holes It is a posit of modern astrophysics that most massive galaxies host a super- massive black hole (millions to billions of times more massive than the Sun). These black holes affect the evolution of galaxies well beyond their gravitational sphere of influence (which does not extend wider than 1/1000th of the typical galaxy linear size). In turn, the evolution of galaxies affects the growth of black holes through, e.g., galaxy merging.... Matteo Guainazzi |
|
15/12/2022 - 19:00
Los genes como recortables. La edición genética basada en la tecnología CRISPR En el año 2012, un trabajo publicado en la revista Science demostró que la tecnología CRISPR podía ser usada de una manera precisa y eficiente en la edición del genoma de un ser vivo. Desde entonces, el método ha llevado a miles de laboratorios a utilizarlo en aplicaciones que van desde biomedicina hasta agricultura. Francisco Martínez-Abarca |
|
02/11/2022 - 04/11/2022
https://home.iaa.csic.es/fundcosmo22/ Granada |
|
18/10/2022 - 21/10/2022
https://www.granadacongresos.com/severoochoa Granada |
|
09/09/2022 - 11/09/2022
https://iota-es.de/esop41/index.php Granada |
|
30/01/2023 - 01/02/2023
https://www.granadacongresos.com/agn2023 Granada |
|
24/11/2022 - 19:00
Asteroides activos y la misión DART de defensa planetaria Conferencia de divulgación sobre los asteroides activos, que muestran rasgos tanto de asteroide como de cometa Fernando Moreno |
|
12/01/2023 - 12:30
CARMENES-PLUS: a technical upgrade for CARMENES and the impact on its science CARMENES is a dual (VIS: 550 to 950 nm; NIR: 950 to 1700 nm) high-resolution spectrograph installed at the 3.5 m telescope at the Calar Alto Observatory (CAHA, Almería, Spain). The NIR channel spectrograph uses the radial-velocity method for detecting exoplanets around low-mass stars. Thus, a high thermal stability is required in the NIR cooling system to achieve a high precision in radial velocities. The cooling system was originally conceived... Roberto Varas González |
|
25/05/2023 - 12:30
SO colloquio: To be black, or not? Observational tests of strong field gravity are improving rapidly. This allows us to test whether the compact objects observed in the sky are truly black holes as described in general relativity or some other "exotic" objects. These tests, however, require exquisite theoretical modeling of black holes as well as their alternatives. This talk will discuss two such examples: the impact of the astrophysical environment on black holes and the... Dr. Béatrice Bonga |
|
24/11/2022 - 12:30
SO webloquio: The Milky Way Nuclear Star Cluster The Milky Way nuclear star cluster (NSC) is located within the nuclear stellar disc (NSD) in the Galactic centre. The NSC and NSD are distinct structures of the Milky Way, but also connected to the larger Milky Way structures, e.g. via the inflow and outflow of gas, and the infall of star clusters. Our knowledge of the larger Milky Way structures, Galactic disc, bulge and halo, has expanded in recent years through surveys and dedicated missions... Dr. Anja Feldmeier |
|
07/11/2022 - 12:30
The ASTRI Mini-Array and its Science The ASTRI Collaboration is building at the Teide Astronomical Observatory in Tenerife an array of 9 small Cherenkov telescopes capable of observing with good flux sensitivity, energy and angular resolution the gamma-ray sky above an energy threshold of several hundreds of GeV. The ASTRI telescopes adopt a dual-mirror Schwarzschild-Couder optical design. Entrapped amidst the two mirrors the ASTRI camera, based on silicon photon-multipliers... Dr. Giacomo Bonnoli |
|
29/11/2022 - 12:30
TARSIS: the Tetra-Armed IFU at Calar Alto designed for the CATARSIS galaxy cluster exploration In this talk I will present the design of the Integral Field Unit TARSIS, recently selected to be the next generation multi-object spectrograph for the 3.5m telescope at Calar Alto. In addition, I will describe the scientific goals of CATARSIS, the galaxy cluster exploration that will be carried out in the first years of the operation of TARSIS. Dr. Jorge Iglesias |
|
15/11/2022 - 12:30
The effect of pre-processing on the stellar population content of early-type dwarf galaxies According to the CDM model, galaxy clusters grow through the accretion of individual galaxies and galaxy groups. Thus, it is a true challenge to distinguish the possible role of the present-day host halo from that of previous ones, in the transformation of accreted galaxies. Dwarf early-type galaxies (dEs) are often regarded as statistically meaningful testbeds for investigating environmental effects mainly due to their high number density and... Dr. Bahar Bidaran |
|
13/10/2022
Congreso Severo Ochoa IAA: abordando las cuestiones clave en astrofísica desde Granada El Instituto de Astrofísica de Andalucía (IAA-CSIC) organiza un encuentro con especialistas de todo el mundo sobre los problemas más actuales que afronta la astrofísica |
|
27/10/2022 - 19:00
La génesis de las constelaciones. Mitos y literatura en la astronomía griega La esfera celeste se divide en la actualidad en 88 constelaciones. Son agrupaciones aparentes de estrellas que aparecen dibujadas sobre la esfera celeste, en un ejercicio intelectual que mucho tiene que ver con la cultura. Cada civilización ha recreado las constelaciones según sus creencias, aunque las aceptadas por la Unión Astronómica Internacional se basan, sobre todo, en la Era de los Descubrimientos y en la tradición grecorromana.... David Barrado Navascués |
|
15/09/2022
AstroSound 2022 El Instituto de Astrofísica de Andalucía es uno de los mayores centros de referencia en astrofísica y ciencias del espacio a nivel internacional. Además, destaca por su intensa actividad divulgadora; su Unidad de Cultura Científica es una de las más reconocidas de nuestro país, acercando la ciencia a la sociedad a través de formatos rompedores que han sido merecedores de diferentes reconocimientos a lo largo de los últimos años. ASTROSOUND... |
|
19/12/2022 - 12:30
Fossil groups of galaxies: seeing the future looking at the past The nature of fossil groups of galaxies has been debated for over more than 3 decades. This is in part because of the lack of deep multiwavelength data and also due to the low purity of samples selected using solely magnitude gap criteria. The initial results of a sample of bonafide fossil groups using X-ray/optical observations has clarified many of their characteristics, such as high central metal abundances and concentration measurements.... Dr. Renato Dupke |
|
01/12/2022 - 12:30
SO Colloquio: Moving from high to extreme precision in air shower observations: From LOFAR to SKAO Cosmic rays play an interesting role in understanding the most violent objects in the universe. These charged atomic particles reach energies orders of magnitudes higher than achievable in accelerators on Earth, which points towards an origin of the most extreme objects in the universe, with strong magnetic shocks and mass transfer. However, these sources are not firmly identified. Astrophysical interpretations are currently limited by the... Dr. Anna Nelles |
|
17/11/2022 - 12:30
SO colloquio: A conclusive test of the cold dark matter model The ``Lambda cold dark matter'' (LCDM) cosmological model is one of the great achievements in Physics of the past thirty years. Theoretical predictions formulated in the 1980s turned out to agree remarkably well with measurements, performed decades later, of the galaxy distribution and the temperature structure of the cosmic microwave background radiation. Yet, these successes do not inform us directly about the nature of the dark matter. This... Dr. Carlos Frenk |
|
08/11/2022 - 12:30
The many “phases” of small bodies Asteroids, comets, and trans-Neptunian objects are collectively known as small bodies. In a way, they are the debris left by the planetary formation in the Solar system, and as such, they carry a lot of information regarding the processes that shaped it. But, small bodies are by no means stationary objects: not only do they move across the sky, but their brightness also changes due to different mechanisms, from rotational variations due to... Dr. Álvaro Alvarez-Candal |
|
25/10/2022 - 12:30
SO Colloquio: Galactic Center: Radiation from black hole candidates and the dynamics of high velocity stars We summarize recent research results on the radiation mechanism of the Super Massive Black Hole (SMBH) candidate SgrA* and ask the question if there are Intermediate Mass Black Hole (IMBH) candidates in the central stellar cluster. Furthermore we give an update on the most recent high velocity stars in the central arcsecond - that are closest to SgrA*. Here we concentrate on the high velocity star cluster dynamics and on the 4711+ stars with... Prof. Andreas Eckart |
|
26/09/2022 - 12:30
The EnVision mission to Venus: Discovering why our closest neighbour is so different EnVision was selected as ESA’s 5th Medium-class mission in the Agency’s Cosmic Vision plan, targeting a launch in the early 2030s. The mission is a partnership between ESA and NASA. The primary goal is to provide a holistic view of Venus, from its inner core up to its upper atmosphere by a single mission, and will be the first mission of its kind. More specifically, EnVision will characterise Venus’ core and mantle structure, in order to study... Dr. Anne Grete Straume |
|
13/09/2022 - 12:30
SO Colloquio: Studies on the origins of our solar system My goal in this colloquium is to apprehend globally the Solar System by describing a vast sample of small bodies, from Near Earth Asteroids to remote Trans-Neptunian Objects. This goes beyond projects that focused on certain populations only. The core of the talk is theoretical, with emphasis on inner structures and rings. Meanwhile, the stellar occultations by these objects will provide an exploratory route to characterize objects with widely... Dr. Bruno Sicardy |
|
29/06/2022
El Instituto de Astrofísica de Andalucía acoge el II Encuentro de Gestor@s de la alianza de centros Severo Ochoa y unidades María de Maeztu, SOMMa. Este viernes 1 de julio tendrá lugar en el Instituto de Astrofísica de Andalucía (IAA-CSIC) el II Encuentro de Gestor@s de la alianza SOMMa. Esta alianza reúne a los Centros de Excelencia Severo Ochoa y Unidades de María de Maeztu acreditadas con este sello, que otorga el Ministerio de Ciencia e Innovación a aquellos centros y unidades de investigación que destacan por su relevancia e impacto a nivel internacional. |
|
06/10/2022 - 12:30
Computational Intelligence in the Big Data Context Computational Intelligence (CI) commonly refers to a variety of bio-inspired and/or human-like techniques that can be applied in optimisation, learning and modelling problems. Broadly speaking, CI comprises Artificial Neural Networks, Fuzzy Sets and Fuzzy Logic and Evolutionary Computation. In the era of big data, CI in conjunction with data mining techniques are expected to help uncover useful knowledge from big data as they are very well... Dr. Isaac Triguero |
|
13/10/2022 - 12:30
New developments at the IAA cosmic dust laboratory The interpretation of astronomical observations of comets and asteroids and of extrasolar objects such as protoplanetary and debris disks is crucial for understanding the origin and evolution of planetary systems. Collecting electromagnetic radiation scattered or emitted by dust particles present in these objects with powerful telescopes is often our only way to observe and characterized them. In situ observations are available for a handful of... Dr. Juan Carlos Gómez |
|
20/05/2022 - 22/05/2022
COURSE ON DISSEMINATION TECHNIQUES. RECREATIONAL AND TRAINING DAYS "Practical classes and leisure activities". Granada |
|
31/12/2023 - 12:30
SO Colloquio: Present and future large radio surveys of the extreme universe Transient radio emission is a fundamental tracer and physical probe of the most extreme and transient events in the universe. In this talk I will discuss a number of recent developments with existing radio telescopes, including i. the ThunderKAT image-plane transients programme on MeerKAT, ii. The first citizen-science project to search for commensal radio transients, iii. First radio detections of 'VHE GRBs' detected by ground-based Cherenkov... Dr. Rob Fender |
|
10/11/2022 - 12:30
SO Colloquio: The Cherenkov Telescope Array: Status and Prospects The Cherenkov Telescope Array (CTA) will become the reference observatory for Very High Energy (VHE) Gamma Ray Astronomy during the next decades. CTA promises a jump in sensitivity and energy coverage of one order of magnitude over the current instruments, significantly improved energy and angular resolutions and full sky coverage. Over thousand new sources will foreseeably be identified in this range for the first time. VHE gamma rays are... Dr. Juan Cortina |
|
30/06/2022 - 19:00
El plano ondulado de la galaxia Conferencia sobre la Vía Láctea, la galaxia que alberga el Sistema Solar Emilio J. Alfaro |
|
28/10/2022 - 12:30
SO Colloquio: Cosmografía: las aportaciones de al-Ándalus y los reinos ibéricos a la Revolución Científica Si el Señor Todopoderoso me hubiese consultado, antes de embarcarse en la Creación, le habría recomendado algo más simple. Esta frase, supuestamente formulada por Alfonso X "el Sabio", muestra la complejidad del conocimiento cosmográfico en al-Ándalus y en los reinos cristianos que recibieron su acervo científico. La península Ibérica se convirtió a partir del siglo X en puente esencial para que el saber de la civilización grecorromana,... Dr David Barrado Navascués |
|
15/06/2022 - 15/06/2022
Matplotlib for beginners II - A brief Severo Ochoa training school Online |
|
21/07/2022 - 12:30
SO Webloquio: Cold gas constraints via HI Intensity Mapping in the SKA era Intensity mapping surveys of neutral hydrogen (HI) are a new way to measure the large-scale matter distribution of our universe over a wide range of redshifts, and thus constrain cosmological parameters describing the universal expansion. The next generation of radio telescopes and interferometers - in particular the Square Kilometre Array (SKA) - are being designed and built to include optimising the detection of the HI line at low spatial... Dr. Laura Wolz |
|
17/05/2022 - 18/05/2022
Gender Analysis in Research Granada |
|
11/05/2022
La ciencia, de nuevo, en la Feria del Libro El Instituto de Astrofísica de Andalucía, el Estación Experimental del Zaidín, el Parque de las Ciencias y la Feria del Libro organizan la quinta edición del Área de Ciencia de la Feria del Libro, que se ubicará en la plaza del Humilladero, frente a la Fuente de las Granadas |
|
22/09/2022 - 12:30
SO Web-loquio: Old/new problems with Active Galactic Nuclei and AGN application to cosmology After several decades of studies the basic nature of nuclear activity of galaxies is well understood. However, unexpected behaviour of AGN was already noted in the past, and with rise of the amount of data we see numerous evidences of phenomena which still require explanation, line Quasi-Periodic Ejection sources, and Changing-Look AGN. Also it is now time to address in more detail the physical nature of the simple AGN components like Broad Line... Prof. Bozena Czerny |
|
07/06/2022 - 12:30
Revisiting the intermediate- to high-mass star formation Intermediate and high-mass forming stars have a large impact on the interstellar medium and nearby star forming regions. Historically, the study of the general properties of intermediate- to high-mass pre-main sequence stars has been hampered by the lack of a well-defined, homogeneous sample, and because few and mostly serendipitously discovered sources were known. As a consequence, many open problems involving high-mass star formation suffer... Dr. Miguel Vioque |
|
16/09/2022 - 12:30
SO Colloquium: Sex and gender analysis in research and Innovation This lecture aims to increase researchers’ awareness of the current demands for the inclusion of sex and gender in their research. In fact, several governments and granting agencies, such as the European Commission and the Spanish Agencia Nacional de Investigación (AEI), now require that requests for funding address whether, and in what sense, sex and gender are relevant to the objectives and methodologies of the research proposed. Parallel with... Dr. Capitolina Díaz |
|
01/09/2022 - 12:30
SO Webloquio: Stellar Magnetism and Extra-Solar Space Weather The environment around the Sun and other late-type stars is controlled by magnetic fields. The coronal high-energy radiation (Extreme Ultra-Violet and X-ray photons), the structure and strength of stellar winds, as well as transients such as flares, coronal mass ejections (CMEs), and energetic particle events, are some examples of this magnetic influence. Apart from their direct consequences on the star and its evolution, these phenomena will... Dr. Julián Alvarado-Gómez |
|
23/05/2022 - 12:30
New insight into the magnetism of isolated white dwarfs Many stars evolve into magnetic white dwarfs, but we do not know when the magnetic field appears at their surface, if and how it evolves during the cooling phase, and, above all, what are the mechanisms that generate the field, and why they act on some but not all degenerate stars. Observations may help to find an answer to these questions, but their interpretation is dramatically affected by biases due to target selection and a non-homogeneous... Dr. Stefano Bagnulo |
|
27/10/2022 - 12:30
SO colloquio: A new look at the torus of active galactic nuclei The classical picture to explain the observations of active galactic nuclei (AGN) required a geometrically and optically thick torus of molecular gas and dust to obscure the central engine from some lines of sight. For more than two decades, the torus was believed to be a compact (pc-scale), isolated, and rotating structure. Our recent work in the Galactic Activity, Torus, and Outflow Survey (GATOS), using ALMA and high-angular resolution mid-... Dr. Almudena Alonso Herrero |
|
21/09/2022 - 16:30
SO Webloquio: Dwarf Galaxies and the Smallest Supermassive Black Holes Despite traditional thinking, an appreciable population of (relatively small) supermassive black holes may be lurking in dwarf galaxies. Before the last decade, nearly all known supermassive black holes were in the nuclei of giant galaxies and the existence of such black holes in dwarf galaxies was highly controversial. The field has now been transformed, with a growing community of researchers working on a variety of observational studies... Dr. Amy Reines |
|
21/06/2022 - 12:30
SO webloquio: Star-planet plasma interactions and radio emissions Exoplanets are expected to sustain various plasma interactions with their parent star, depending on the stellar and planetary magnetic field strengths and on the sub- or super-Alfvénic wind speed at the planet’s orbit. Three such interactions lead to electron acceleration and subsequent radio emissions in our solar system: magnetized planets hit by the super-Alfvénic solar wind, and the sub-Alfvénic interactions of the unmagnetized moon Io and... Dr. Philippe Zarka |
|
07/07/2022 - 12:30
SO Webloquio: Optical interferometric studies of star and planet formation A first step towards understanding planetary formation is the characterisation of the structure and evolution of protoplanetary discs. Although the large scale disc is understood in some detail, very little is known about the inner few au. In this region, dust grains sublimate, and accretion and ejection take place, affecting the entire disk structure and evolution. In this talk, I will review how optical interferometric observations can... Dr. Rebeca García López |
|
03/05/2022 - 12:30
Radio astronomy in the pre-SKA era: What can Apertif do for you? With the Square Kilometre Array still several years away, SKA pathfinder telescopes are already enabling transformational science in radio astronomy with their astounding improvements in field-of-view, sensitivity, spatial resolution, and spectral bandwidth coverage. The APERture Tile In Focus (Apertif) is one such SKA pathfinder: a phased array feed instrument upgrade to the Westerbork Synthesis Radio Telescope that increases the field-of-view... Dr Kelley Hess |
|
14/06/2022 - 12:30
Detailed equilibrium and dynamical tides: impact on circularization and synchronization in open clusters Binary stars evolve into chemically-peculiar objects and are a major driver of the Galactic enrichment of heavy elements. During their evolution they undergo interactions, including tides, that circularize their orbits and synchronize stellar spins, impacting both individual systems and stellar populations. My recent work introduces an accurate implementation of equilibrium and dynamical tides in the stellar population code binary_c, relying... Dr. Giovanni Mirouh |
|
31/05/2022 - 12:30
SO Webloquio: Empirical and physical properties of Lyman continuum emitters Lyman continuum emitters are galaxies showing escaping ionizing radiation, which thus contributes to ionizing the intergalactic medium. They may be the dominant source of cosmic reionization. I will present an overview of the observations and modeling of low-z analogs of the sources of cosmic reionisation recently discovered. HST observations, including UV spectroscopy with COS and rest-UV imaging with the WFC3, combined with ground-based... Dr. Daniel Schaerer |
|
24/05/2022 - 12:30
Time domain astronomy with future X-ray satellites Accreting black holes emit in X-rays at the wave-band in which THESEUS will be observing (0.3 keV-20 MeV) due to their extreme physical conditions. The softer energy range is devoted to thermal emission from the accretion disc and the harder is due to the existence of a hard X-ray emitting corona (with undefined geometry so far). The importance of one component versus the other gives rise to the diverse state classification of accreting black... Dr. Maria D. Caballero-Garcia |
|
14/07/2022 - 12:30
A journey into the Perseus cluster of galaxies The central black hole of active galaxies accretes large amounts of matter and powers jets of relativistic particles that can propagate beyond the host galaxy. Radio galaxies are particularly bright at ∼ GHz frequencies, when the accelerated electrons interact with the magnetic field and produce strong synchrotron emission. Such galaxies residing in clusters evolve in a hot, diffuse, X-ray emitting plasma (the intracluster medium, ICM) which is... Dr. Marie-Lou Gendron-Marsolais |
|
26/04/2022 - 12:30
Destroying Planetary Systems Modern astronomy invests a large amount of effort to search and characterise planetary systems around solar-like stars. In particular, at early stages of their formations in proto-planetary disks. However, we barely know much about the capacities of the planets to survive the harsh environments produced by their host stars during their evolution. In this talk, I will describe the effects a planet can produce by helping shape the mass loss of... Dr. Jesús Toala |
|
24/03/2022 - 12:30
Is it possible to simulate time machines in a laboratory? General Relativity is the most succesful theory we have for describing gravitational phenomena. Its range of applicability is vast: from solar system scales to cosmological scales. It is well-known that GR allows the existence of time machines: devices that are able to generate Closed-Timelike-Curves (CTCs). Although these kind of objects are allowed in GR, most researchers believe that they cannot occur on macroscopic scales. However, it is... Gerardo Garcia |
|
20/05/2022 - 11:30
Imaging the supermassive black hole at the galactic center with the EHT We present the first Event Horizon Telescope (EHT) observations of Sagittarius A* (Sgr A*), the Galactic center source associated with a supermassive black hole. These observations were conducted in 2017 using a global interferometric array of eight telescopes operating at a wavelength of λ = 1.3 mm. The EHT data resolve a compact emission region with intrahour variability. A variety of imaging and modeling analyses all support an image that... José Luis Gómez, Rocco Lico, Guang-Yao Zhao, Ilje Cho, Antonio Fuentes, y Thalia Traianou |
|
11/05/2022 - 12:30
SO Coloquio: Stellar clustering connecting the formation and evolution of galaxies to the formation and evolution of us The clustered nature of star formation leaves a long-term imprint on galaxies, stars, and planets. At young ages, stellar clustering subdivides galaxies into individual building blocks undergoing vigorous, feedback-driven life cycles that vary with the galactic environment. These units structure the interstellar medium spatially, dynamically and chemically, and collectively define how galaxies form stars. At old ages, the relics of clustered... Dr. Diederik Kruijssen |
|
12/05/2022 - 12:30
SO Coloquio: The cloud-scale baryon cycle across the nearby galaxy population The cycling of matter in galaxies between molecular clouds, stars and feedback is a major driver of galaxy evolution. However, it remains a major challenge to derive a theory of how galaxies turn their gas into stars and how stellar feedback affects the subsequent star formation on the cloud scale, as a function of the galactic environment. Star formation in galaxies is expected to be highly dependent on the galactic structure and dynamics,... Dr. Mélanie Chevance |