Recent Talks

List of all the talks in the archive, sorted by date.


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Tuesday April 20, 2021
Dr. Sebastian Trujillo Gomez
Heidelberg University

Abstract

In this talk I will discuss how the stellar, globular cluster (GC), and gas components of galaxies allow us to trace the assembly of galaxies and their dark matter (DM) haloes, and how they constrain the complex physics of galaxy formation. I will use examples from three studies: in the first one, I will describe how the study of the phase-space distribution of the MW GC system using Gaia in the context of the E-MOSAICS simulations provides a detailed quantitative picture of the formation of the Galaxy. In the second example, I will show how the unusual GC populations in galaxies like the infamous NGC1052-DF2 and DF4 can be used to rewind the clock and obtain a snapshot of their galactic progenitors at cosmic noon. A simple model of star cluster formation points to an extremely dense birth environment and strong structural evolution, providing clues of the effect of clustered star formation on galaxy evolution. In the last part I will describe a follow-up study of the impact of clustered star formation on galaxy structure that provides clues on the origin of ultra-diffuse galaxies (UDGs), which are difficult to explain in the current paradigm of galaxy formation. I will show how anchoring an analytical model on galaxy scaling relations and numerical simulations predicts the emergence of UDGs that lack DM driven by clustered feedback from young GCs.


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Friday April 9, 2021
Jorge Quintero
IAC

Abstract

En la presente charla hablaremos de la sobre la actualización que se está llevando a cabo en el software de control del Instrumento Gris de Gregor y como se ha intentado poner en marcha un sistema de integración continua. Además, se comentará la idea de montar un banco polar basado en un sistema de integración continua.

 


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Friday March 26, 2021
Eduardo David González
IAC

Abstract

Durante el presente seminario hablaremos sobre el estado actual del banco óptico GTCAO. Se hará énfasis en las tareas mecánicas en curso referentes a las instalaciones auxiliares para la integración y comisionado del banco, planteando problemáticas generales de las tareas y soluciones adoptadas.

 

 

 

Enlace Youtube: https://youtu.be/4WTGKMGwd7o


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Thursday March 18, 2021
Jorge A. Pérez Prieto
Instituto de Astrofísica de Canarias

Abstract

In the last decade, Python went from being a moderated-used programming language in the astronomical community to the de-facto standard in Astronomy. Its recent growth has been spectacular, thanks to the coordination and work of the community to create astropy, the core astronomy library, as well as other base libraries like numpy and matplotlib. However, the current scientific/astronomical ecosystem for Python is huge and sparse, introducing many types of objects and methods, often confusing at the beginning.

 

In this SMACK talk I will describe the current status of the Python ecosystem for astronomy and introduce the most import elements of the core libraries, numpy and astropy, showing with practical examples how they provide new impressive capabilities to deal with data, catalogs, coordinates and much more, making life easier for astrophysicists.


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Tuesday March 16, 2021
Dr. Nicolás Sanchis-Gual
Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications (CIDMA)

Abstract

The detections of gravitational waves are opening a new window to the Universe. The nature of black holes and neutron stars may now be unveiled, but gravitational radiation may also lead to exciting discoveries of new exotic compact objects, oblivious to electromagnetic waves. In particular, Advanced LIGO-Virgo recently reported a short gravitational-wave signal (GW190521) interpreted as a quasi-circular merger of black holes, one at least populating the pair-instability supernova gap. We found that GW190521 is also consistent with numerically simulated signals from head-on collisions of two (equal mass and spin) horizonless vector boson stars (aka Proca stars). This provides the first demonstration of close degeneracy between these two theoretical models, for a real gravitational-wave event. 


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Friday March 12, 2021
Txinto Vaz
IAC

Abstract

A la hora de planificar un proyecto la gestión de las dependencias técnicas entre tareas ya supone un desafío.  Añadamos a la coctelera las dependencias circunstanciales y, por qué no, sumerjamos el experimento en una organización matricial donde todos los miembros del equipo trabajan en varios proyectos.

 


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Thursday March 11, 2021
Dr. Tomer Shenar
KULeuven

Abstract

"Classical Wolf-Rayet (WR) stars" represent a class of hot, hydrogen-depleted stars wtih powerful stellar winds and are prominent progenitors of black holes. Next to their unparalleled radiative and mechanical energy feedback, they offer unique probes of massive-star evolution at the upper-mass end. To become a classical WR star, single stars require substantial mass-loss to strip their outer, hydrogen-rich layers, implying that only very massive stars could enter the WR phase. However, mass-transfer in binaries can further aid in the stripping of stars and form Wolf-Rayet stars, or more generally helium stars, at lower masses.  Due to the decrease of mass-loss with metallicity, it has been predicted that WR stars at low metallicity tend to form in binaries. However, this has so far not been supported by observations.

In my talk, I will give an overview on our current knowledge of the properties of Wolf-Rayet populations in the Galaxy and the Magellanic Clouds based on exhaustive spectral analyses. I will illustrate why binary formation does not necessarily dominate the evolution of WR stars at low metallicity, and highlight important discrepancies between theory and observations of WR stars. I will discuss the observed rarity of intermediate mass helium stars, and present recent reports of unique helium stars in the exotic binaries LB-1 and HR 6819.

 


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Tuesday March 9, 2021
Dr. Teimuraz Zaqarashvili
University of Graz

Abstract

Recent progress in observations of Rossby-type waves on the Sun revived the interests towards the waves. Though the hydrodynamic Rossby waves are well studied in the Earth context, ubiquitous existence of magnetic field in the atmosphere/interior of the Sun requires to study the waves in magnetohydrodynamics. The talk will cover the recent direct observations of Rossby waves on the Sun, theoretical development of magneto-Rossby wave theory and the possible connection of the waves to observed long and short term variations in solar magnetic activity.


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Tuesday March 2, 2021
Dr. Pedro Figueira
ESO

Abstract

The search for extrasolar planets is one of the fastest-growing fields of astronomy. This rapid growth was both made possible by the development of instrumentation and motivated it, creating a virtuous cycle that impacted positively several fields of research.

In this talk I will present the latest planet-hunting spectrograph ESPRESSO, installed at ESO's VLT. Targeting a radial velocity precision of 10 cm/s, ESPRESSO has the declared goal of detecting an Earth-mass planet inside the habitable zone of a main-sequence dwarf star. I will discuss the first results, ongoing campaigns, and reveal a bit of what the future holds for us.



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Friday February 26, 2021
Noé A. Rodríguez González
IAC- EST PO

Abstract

La gestión de documentos es una tarea compleja que implica múltiples cuestiones, especialmente en proyectos como la definición y creación de un telescopio.  Una correcta gestión documental requiere entre otras cuestiones:

  • Ser fuente única de verdad: Los documentos deben gestionarse desde un punto central que actúe como fuente única de verdad permitiendo la localización y actualización de los mismos.
  • Permitir búsquedas ágiles, simples y eficaces: Aunque el volumen de documentos sea elevado las búsquedas deben mantenerse ágiles y sencillas permitiendo localizar los documento en base a sus características o a la información que contienen.
  • Facilitar la coherencia de formato: Los documentos creados en un proyecto deben mantener un formato y esquema coherente mediante la utilización de plantillas.
  • Agilizar la creación de documentos: La solución debe permitir la creación de nuevos documentos de forma sencilla realizando de forma automatizada tantas tareas como sea posible (codificación, pre-formateo del documento,...).
  • Gestión bibliográfica: los documentos requieren de un mecanismo de codificación que permita la identificación de los mismos.
  • Permitir versionado de documentos: Los documentos evolucionan a lo largo de su ciclo de vida dando lugar a versiones que deben ser almacenadas e identificadas.

Las plataformas de gestión documental existentes "out of the box" no cubren el 100%  de estos requisitos. Sin embargo, ofrecen mecanismos de extensión que permiten ampliar sus capacidades. Desde la oficina de proyecto del EST hemos desarrollado una herramienta para la gestión de los documentos del proyecto,  a partir de soluciones libres como Alfresco o Carbone.io, que cubre todas estas necesidades.



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Recent Talks