A team of astronomers led by ICE-CSIC analyzed for the first time a long radio-observation of a scallop-shell star in a pioneer study. The team observed the star using the Giant Metrewave Radio Telescope (GMRT) located in Pune (India), and related it to the photometric information from NASA’s Transiting Exoplanet Survey Satellite (TESS) and Las Cumbres Global Telescope Observatory. Scallop-shell stars are a recently discovered class of young M dwarfs. More than 70% of the stars in the Milky Way are M dwarfs, although there are only around 50 recently confirmed scallop-shell stars. They show

The President of the Cabildo of La Palma, Sergio Rodríguez inaugurated this morning the International Conference LSST@Europe 6 which has brought together over 140 people from over twenty countries in the field of astrophysical research. In the oficial inauguration there was also participation by the Director of the Instituto de Astrofísica de Canarias (IAC), Valentín Martínez Pillet, the director of the LSST constructive project Zeljko Ivezic and the president of the international organizing committee Mireia Montes Quiles. Sergio Rodríguez noted the importance of this type of scientific

The distribution of planets in the over five thousand distant solar systems discovered to date forms a complex puzzle. There is a region in the planetary orbit graph, known as the " Neptunian desert", where very few Neptune-like planets with orbits of between two and four days period around their star have been recorded to date. Now, a scientific team led by the Instituto de Astrofísica de Canarias (IAC) and the Instituto de Astrofísica de Andalucía-Consejo Superior de Investigaciones Científicas (IAA-CSIC) , using a novel technique, new planets around red dwarf stars located precisely in