The main objective of the NASA OSIRIS-REx mission is the collection of material from the surface of primitive asteroid (101955) Bennu, and to bring it back to...
The interstellar medium is an excellent laboratory to test physical processes that cannot be reproduced in Earth-based laboratories. In this study several...
Constraints on Ultra-Light Dark Matter from Galactic Rotation Curves by Prof. Diego Blas Imperial College
ABSTRACT Bosonic ultra-light dark matter (ULDM) in the mass range m ~ $10^{-22} - 10^{-21} \rm eV$ has been invoked as a motivated candidate with new input for...
Cosmic amorphous dust in the interstellar medium as a possible explanation for the Anomalous Microwave Emission
The main emission mechanisms of the interstellar medium (ISM) in the spectral range between the radio and the far infrared are very well characterised and...
With the advent of the new generation of galaxy surveys, such as eBOSS, DES, DESI, EUCLID, HETDEX, J-PAS, J-PLUS, LSST, PAU, Taipan, Vipers, Wallaby, WEAVE...
In addition to being a long-postulated particle that satisfactorily explains the absence of the neutron’s dipole moment observed in laboratories while...
DALI(PoP). Pioneering the tunable broad band search for axion dark matter above 25 μeV
The detection of the axion would be one of the most important events in the history of science. This hypothetical particle can simultaneously solve two...
Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars
Exoplanets smaller than Neptune are common around red dwarf stars (M dwarfs), with those that transit their host star constituting the bulk of known temperate...
La óptica adaptativa de GTC está en su fase final de integración y verificación. El primer instrumento que se tiene previsto utilizar es FRIDA que puede tener...