Esta mañana, Pablo Casado, presidente del Partido Popular (PP) y candidato a la Presidencia del Gobierno de España, visitó la sede central del Instituto de Astrofísica de Canarias (IAC), en La Laguna, junto con otros representantes de su partido. El político se mostró interesado en conocer la labor investigadora y de desarrollo tecnológico que se realiza en el IAC y en los Observatorios de Canarias, así como los proyectos de futuros telescopios. Acompañado por Casiana Muñoz-Tuñón, subdirectora del IAC, y otros miembros del Comité de Dirección de este centro, Casado recorrió las instalaciones y accedió a los talleres y laboratorios donde se diseñan, fabrican y montan los instrumentos que después se envían tanto a telescopios terrestres como al espacio.
Pablo Casado junto a representantes de su partido y miembros del Comité de Dirección del Instituto de Astrofísica de Canarias. Crédito: Jorge Dóniz (IAC).
Advertised on
It may interest you
-
Astronomers at the Instituto de Astrofísica de Canarias (IAC), using the 2-meter robotic Two-meter Twin Telescope (TTT) at the Teide Observatory, have obtained the deepest optical images ever taken of Malin 2, one of the largest and faintest spiral galaxies in the Universe. These ultra-deep observations have revealed previously unseen structures, including several diffuse stellar emissions and a striking, elongated spiral-like feature, hinting at past interactions with other galaxies. The team has also identified a potential ultra-diffuse dwarf galaxy (UDG) about 400,000 light-years fromAdvertised on -
Last night, the 5,000 fibre-optic ‘eyes’ of the Dark Energy Spectroscopic Instrument (DESI) reached a major milestone, having fully covered the area originally planned for its map of the universe. Thus, DESI’s five-year programme has concluded ahead of schedule and with far more data than expected, resulting in the largest high-resolution 3D map of the universe ever produced. This map will enable researchers to explore dark energy, which accounts for 70% of the universe and drives its accelerated expansion. By comparing how galaxies were distributed in the past with their currentAdvertised on -
An international team composed of Drs. Sylvain G. Korzennik, from the Center for Astrophysics | Harvard & Smithsonian , and Antonio Eff-Darwich Peña, from the University of La Laguna and the Instituto de Astrofísica de Canarias, has published a pioneering study aimed at improving our understanding of the Sun’s internal structure. The work, published in The Astrophysical Journal , stands out for its use of exceptionally long helioseismic time series, exceeding twenty-five years of continuous observations, to analyze the deepest layers of the Sun. Helioseismology is the study of patterns ofAdvertised on