The first image of a new gaseous component in a planetary nebula.
False color image of the planetary nebula NGC 6778. In blue, the emission associated with weak lines of ion O++ recombination, taken with the OSIRIS tunable filter blue instrument in the GTC. In green, emission of the same ion in the excited lines by coll
Advertised on
Jorge García Rojas: jogarcia_ext [at] iac.es (jogarcia_ext[at]iac[dot]es)
The Instituto de Astrofísica de Canarias (IAC) has again shown its high quality in the field of international research. Two of its Research Professors, Carme Gallart and Enric Pallé, have been selected by the European Research Council (ERC) to receive ERC Advanced Grant s , the most prestigious and competitive grants of the Horizon Europe programme. This call for proposals is aimed at researchers who are leaders in their fields, with consolidated records and highly innovative proposals. Each grant can reach up to 2.5 million euros over five years, with additional funding for specific needs
From March 9–12, 2026, the Heidelberg Institute for Theoretical Studies – HITS hosted the Second Annual Meeting of the EDUCADO Doctoral Network (MSCA DN), a network coordinated and led by the Instituto de Astrofísica de Canarias. This pivotal gathering marks a significant milestone in the project’s timeline, bringing together international research groups from across the consortium. The meeting featured the 11 Doctoral Candidates as the central focus, providing them with a platform to present their research progress in applying AI to galaxy evolution and astronomical big data. A highlight of
The Near-Infrared Spectrometer and Photometer (NISP) on board the Euclid space mission has obtained near-infrared (NIR) spectra of millions of objects, including hundreds of ultracool dwarfs (UCDs). Euclid observations retrieve images and slitless spectra simultaneously. This observing mode marks a new era in the discovery of new objects, such as L- and T-type dwarfs, which can be found from direct identification through the H2O and CH4 absorption bands. NISP spectral resolution (R ∼ 450) is enough to classify the objects by the spectral type using known standard templates. Q1 provided more
