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  • ESA/Webb, NASA & CSA, H. Dannerbauer
    Press release
    The IAC finds surprises in Spiderweb protocluster field
    A team of researchers from the Instituto de Astrofísica de Canarias (IAC), collaborating with other international institutions, has managed to find new galaxies in the Spiderweb protocluster. This was possible thanks to the James Webb Space Telescope, which is a project of the space agencies of the United States (NASA), Europe (ESA) and Canada (CSA). Exploring the populations of galaxies, and discovering their physical properties in large scale structures helps astronomers to understand galaxy formation and how their assembly is determined by their environment. The “ Spiderweb” protocluster
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  • El programa Investigadores Visitantes Fundación Occident
    Press release
    El IAC recibe este otoño a un nuevo grupo de personal investigador dentro del programa de Visitantes de Fundación Occident
    El programa Investigadores Visitantes Fundación Occident del Instituto de Astrofísica de Canarias (IAC) sigue su curso con la recepción de un nuevo grupo de personal investigador procedente de distintos centros del mundo. Los investigadores cubrirán un amplio espectro de disciplinas, desde cosmología y astrofísica de partículas hasta física estelar, formación de galaxias y sistemas planetarios. Su presencia y colaboración con el personal investigador del IAC fortalecerá la actividad científica tanto del centro canario como de las personas invitadas y de sus centros de origen, fortaleciendo
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  • Artist’s impression of the accoustic oscillations of normal (“baryonic”) matter, taken from one of thousands of simulations used in the study/ Francisco-Shu Kitaura & Francesco Sinigaglia
    Press release
    The light from quasars, a key to the measurement of the expansion of the distant universe
    The Instituto de Astrofísica de Canarias (IAC) in collaboration with the University of Geneva (Switzerland), the University of Osaka (Japan), and the University of Zhejiang (China) has made a key contribution to a more precise measurement of the expansion of the Universe. This is because they have made an improvement in the precision of the calculation of the scale of the universe in its early stages using the analisis of the distribution of gas in intergalactic space, measurements which reach back to epochs between 10,000 and 12,000 million years ago. This result comes from the análisis of
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