The Centro de Astrobiología (CAB) is bringing together leading astronomers for the «Galaxy Origins in the JWST Era: A Crisol of Stars, ISM, and Supermassive Black Holes» conference in Toledo, Spain, from May 12–16, 2025. The event will highlight the latest breakthroughs in galaxy formation and evolution research, driven by data from the James Webb Space Telescope (JWST) and other major observatories.
Key topics include the emergence of the first stellar populations, the role of gas and dust in the interstellar medium, and the mechanisms behind supermassive black hole growth. The conference will host 150 participants from across the world.
Against the historic backdrop of Toledo, the conference will foster discussions that bridge observational data and theoretical frameworks, providing a comprehensive view of the early universe. More information is available at https://galaxy-crisol25.github.io/website/index.html.
![This image of the GOODS-North field, captured by Webb’s Near-Infrared Camera (NIRCam), shows compass arrows, a scale bar, and a colour key for reference. The north and east compass arrows show the orientation of the image on the sky. Note that the relationship between north and east on the sky (as seen from below) is flipped relative to direction arrows on a map of the ground (as seen from above). The scale bar is labelled in angular distance on the sky, where one arcsecond is one 3600th of a degree. The scale bar is 60 arcseconds long. This image shows invisible near-infrared wavelengths of light that have been translated into visible-light colours. The colour key shows which NIRCam filters were used when collecting the light. The colour of each filter name is the visible light colour used to represent the infrared light that passes through that filter. [Image description: A rectangular image shows thousands of galaxies of various shapes and colours on the black background of space. The pullout features a galaxy labelled GN-z11, seen as a fuzzy yellow dot. Above it is another galaxy, seen as a fuzzy red oval. To the left of the small box, a scale bar is labelled 60 arcseconds. It extends about one tenth of the way across the image. Below the image, a list of NIRCam filters show what colours were used to make the image. Filters shown in blue are F090W, F115W, and F150W. Filters shown in green are F200W, F277W, and F335M. Filters shown in red are F356W, F410M, and F444W.]](https://cab.inta-csic.es/wp-content/uploads/elementor/thumbs/GN-z11_in_the_GOODS-North_field_notadeprensa-GO4-scaled-r41otowxrgxj9g29st0pwp42yavxtox44fqhbthxc8.jpg "GN-z11 in the GOODS-North field (compass image)")
