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 robotic Transient Survey Telescope (TST) installed in the Teide Observatory of the Instituto de Astrofísica de Canarias (IAC) has successfully started its scientific observations. It is a 1 metre telescope which permits the detection of rapidly varying objects, and is set up to map the sky. The TST has been built and run via a public-private collaboration with Canary funding. The Transient Survey Telescope (TST) is a telescope with a 1 metre primary mirror, built to take long-term observations called surveys, for the detection of faint, rapidly varying objects over a wide area of the sky

Using observations made with the James Webb Space Telescope (JWST), an international scientific team, in which the Instituto de Astrofísica de Canarias (IAC) participates, has confirmed variations in morning and evening atmosphere of the exoplanet WASP-39 b, about 700 light-years away from Earth. The research has revealed differences in temperature and atmospheric pressure, as well as indications of different cloudiness and winds that could reach thousands of miles per hour. The results are published in Nature. WASP-39 b, a giant planet with a diameter 1.3 times greater than Jupiter, but