It may interest you
-
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 moreAdvertised on -
A team from the Instituto de Astrofísica de Canarias (IAC) has tested a new technique capable of rapidly identifying the distortions that light undergoes as it passes through Earth’s atmosphere. The development, carried out by the Laboratorio para la Innovación en Optomecánica (LIOM) within the framework of the CELESTE project, could in the future contribute to the creation of more compact and simpler adaptive optics systems to improve the quality of astronomical observations. The technology combines an optical fibre approximately one centimetre long with artificial intelligence techniquesAdvertised on -
A team of scientists, including astrophysicist Carlos Hernández Monteagudo from the University of La Laguna (ULL) and the Canary Islands Institute of Astrophysics (IAC), has compiled one of the most comprehensive catalogues of small bodies in the Solar System, based on photometric observations made from Earth. The study, published in Monthly Notices of the Royal Astronomical Society, compiles data on 6,579 asteroids, comets and irregular satellites, mainly from the main belt located between Mars and Jupiter, opening up new possibilities for studying their composition and rotation. TheAdvertised on