The Instituto de Astrofísica de Canarias (IAC) has received a visit from Robert P. Kirshner, Executive Director of the Thirty Meter Telescope International Observatory (TIO) . During his stay at the IAC headquarters in La Laguna, he was welcomed by the center’s director, Valentín Martínez Pillet, and by the deputy director, Eva Villaver Sobrino, along with other members of the research institute. During his visit, he was able to learn firsthand about the institution’s scientific and technological capabilities and gave a colloquium titled The Thirty Meter Telescope and Science of the Future

Massive stars in metal-poor galaxies often have close partners, just like the massive stars in our metal-rich Milky Way. This has been discovered by an international scientific team in which research staff from the Instituto de Aastrofísica de Canarias (IAC) and the Universidad de La Laguna (ULL) participate. They used the European Very Large Telescope in Chile to monitor the velocity of massive stars in the Small Magellanic Cloud. The research is published in Nature Astronomy . For the past twenty years, astronomers have known that many massive stars in the metal-rich Milky Way have a

The Instituto de Astrofísica de Canarias (IAC) has successfully completed the integration of the scientific detector into the FRIDA (inFRared Imager and Dissector for Adaptive Optics) instrument, an integra-field camera and spectrograph designed to work with the adaptive optics system of the Gran Telescopio Canarias (GTC or Grantecan), the world's largest optical and infrared telescope, located at the Roque de los Muchachos Observatory in La Palma. The integration was carried out in the laboratories of the National Autonomous University of Mexico (UNAM) in Mexico City by a team from the IAC