News

This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • Phellower realizando una observación solar en el Observatorio del Teide
    The Instituto de Astrofísica de Canarias (IAC) is joining the ninth edition of the PHE Festival , one of the most outstanding musical events of the summer in Tenerife. In this first collaboration, the IAC has organised a series of activities that bring astronomy closer to the general public, thus complementing the cultural offer of the festival. On 21 and 22 August, the IAC offered guided tours of the Teide Observatory, allowing visitors to get a first-hand look at one of the most important astronomical research centres in the world. These exclusive visits provided the opportunity to explore
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  • Laboratory of Integrated Circuits (LABIC)
    The Instituto de Astrofísica de Canarias has put itself on the frontier of astrophysical technology by developing the first integrated photonic circuit designed entirely within the Institute. This pioneering advance will permit the improvement of astronomical instruments, and the development of innovative systems for observing the universe. Astrophysical instrumentation, for both ground-based and space-based use is so specialized that often comercial systems and subsystems do not come up to the required specifications, This makes it necessary to buy high priced components or to delegate
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  • Neighbours of Garafía together with the staff of the Roque de los Muchachos Observatory during the Open House Days
    Today, Friday 16th August, the traditional Open Day of the Roque de los Muchachos Observatory (ORM) was held for the residents of the village of Garafía, in La Palma. With this event, the Instituto de Astrofísica de Canarias (IAC) participates in the programme of the Fiestas Patronales of the municipality where the Observatory is located. This fraternisation event, between the town and the scientific, technical and working staff who work at the centre's facilities, has been taking place since the first years of its opening and celebrates its 39th edition. The IAC and the scientific
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  • Magnetar surrounded by the nebula responsible for the radio emission associated with some FRBs
    A new international study, using observations from the Gran Telescopio Canarias at the Roque de los Muchachos Observatory on La Palma, has identified a plasma bubble as the source of the persistent emission observed in some of the so-called fast radio bursts (FRBs), one of the most powerful and unknown cosmic events in the Universe. The data also allow researchers to constrain the nature of the “engine” powering these mysterious sources. The results are published today in Nature. Discovered just over a decade ago, fast radio bursts (FRBs) emit millisecond-long pulses that release an immense
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  • Selection of galaxy images taken by Euclid
    A new citizen science project launched today by the European Space Agency (ESA) and the Euclid Consortium, in collaboration with the Zooniverse platform, will enable volunteers from around the world to identify the shapes of millions of galaxies in images taken by ESA's Euclid space telescope. The aim of the initiative is to train deep AI neural networks to build the largest morphology catalogue to date. In November 2023 and May 2024, the world got its first glimpse at the quality of Euclid’s images, targeting a variety of sources, from nearby nebulas to distant clusters of galaxies. And
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  • log_n_c_n_o_bsgs_ann_groups7
    Massive stars, those over ten times heavier than our Sun, are the conduits of most elements of the periodic table and drive the morphological and chemical makeup of their host galaxies. Yet the origin of the most luminous and hottest stars among them, called 'blue supergiants', has been debated for many decades. Blue supergiants are strange stars. First, they are observed in large numbers, despite conventional stellar physics expecting them to live only briefly. Second, they are typically found alone, despite most massive stars being born with companions. Third, the majority of them harbour
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