Claves de salud y longevidad en el planeta de los genes
En los últimos años, el extraordinario impulso de la Biología Molecular ha permitido el análisis riguroso y profundo de cuestiones esenciales acerca de la...
Dark Matter and the 511 keV Line: Clues from the Galactic Centre
Measurements of the 511 keV emission reveal the presence of a steady injection of positrons that is very concentrated around the Galactic centre, and whose...
Lambda Cold Dark Matter (LCDM) is the most successful theory for the formation of structure in the Universe. Although its predictions have been verified on...
Decoding the state transition in X-ray binaries: a spectral-timing perspective
X-ray binaries (XRBs) are binary systems where a compact object, either a black hole or a neutron star, accretes matter from a stellar companion via an...
Dust in the Wake of Supernovae: Reverse Shocks, Starbursts, and Blue Monsters at z > 10
Supernovae are usually cast as efficient dust destroyers. I will show that, when realistic environments are taken into account, they instead emerge as net dust...
Dust, molecules and gas in nearby AGN: JWST insights from GATOS (the Galaxy Activity, Torus, and Outflow Survey).
It is widely accepted that most galaxies undergo an active phase during their evolution. The impact of the energy released by active galactic nuclei (AGN) has...
Enabling data discovery and reproducible research with ESASky and the ESA Datalabs science platform for HST, JWST and Euclid
The ESAC Science Data Centre (ESDC) hosts the scientific archives from the astronomy, planetary, heliophysics, and human and robotic exploration missions from...
The diversity and prolific number of planets discovered have revolutionised our conception of the nature planet in the Universe. They have opened up the idea of...
We are living in a golden era for testing gravitational physics with precision experiments. This talk will present new results using a variety of tests with...