Severo Ochoa Programme

Technology News

  • 2nd LIOM International Workshop

    From 14 to 16 February, the second scientific meeting of the Laboratory for Innovation in Opto-Mechanics (LIOM) will be held at the IACTEC building managed by the Instituto de Astrofísica de Canarias (IAC) in the Science and Technology Park of La Laguna (Tenerife). This project is dedicated to the development of new optical and mechanical technologies that will form part of the next generation of telescopes capable of detecting biomarkers on exoplanets. One year after its creation, the IAC's Laboratory for Innovation in Opto-Mechanics (LIOM), is holding its second international meeting

    Advertised on
  • Yesterday, 30 October 2023, from the telescope itself at the Roque de los Muchachos Observatory on the island of La Palma, the WEAVE instrument, a powerful state-of-the-art multi-fibre spectrograph, was publicly unveiled. The inauguration ceremony brought to La Palma the leaders of the science funding agencies from the partner countries of the Isaac Newton Group of Telescopes (ING), as well as a strong representation from the 500 members of the science teams and the organisations involved in the design and construction of WEAVE, making it the largest ever gathering of people inside the dome

    Advertised on
  • ExoLife Finder (ELF)

    From 13th to 17th of February, in IACTEC, the technical collaboration zone of the Instituto de Astrofísica de Canarias, the first scientific meeting of the Laboratory for Innovation in Optomechanics (LIOM) is taking place. This is a project for the development of new optical and mechanical technology which will form part of the next generaton of telescopes, such as the ExoLife Finder (ELF), aimed at the search for life outside the Solar System. The meeting has brought together 30 specialists in optics and photonics from Europe, Canada, and the United States. During the course of this week

    Advertised on
  • The Isaac Newton Group of Telescopes (ING) and the WEAVE instrument team present the first observations with this new instrument. This is a powerful latest generation multi-fibre spectrograph which, in synergy with the Gaia satellite of the European Space Agency (ESA), will be used to obtain spectra of several million stars in the disc and the halo of our Galaxy, permitting in-depth “archaeology” of the Milky Way. In addition, other galaxies, both nearby and distant, will be studied, some of them detected by the LOFAR radio telescope, in order to get to know their evolution. WEAVE, on the

    Advertised on
  • Image of the placement of the four legs of the test cryostat in the AIV room of the IAC. Credit: Inés Bonet (IAC).

    The pre-optics for HARMONI, the optical and infrared spectrograph to be installed on the Extremely Large Telescope (ELT) at Cerro Armazones (Chile), has passed successfully the test of the optomechanical design produced by the Instituto de Astrofísica de Canarias (IAC). The instrument will now proceed to the Final Design Phase, prior to the start of the building of the instrument for this telescope of 39 metres in diameter, the largest project in optical and infrared astronomy of the European Southern Observatory (ESO).

    Advertised on
  • Evolution of large-scale structure as calculated by supercomputers. The boxes show how filaments and superclusters of galaxies grow over time, from billions of years after the Big Bang to current structures. Credit: Modification of work by CXC/MPE/V. Springel

    The detection of the axion would mark a key episode in the history of science. This hypothetical particle could resolve two fundamental problems of Modern Physics at the same time: the problema of Charge and Parity in the strong interaction, and the mystery of dark matter. However, in spite of the high scientific interest in finding it, the search at high radio frequency -above 6 GHz- has been almost left aside for the lack of the high sensitivity technology which could be built at reasonable cost. Until now.

    Advertised on