Collision of C-type Ryugu’s parent body with a rocky object
Hayabusa2’s optical navigation camera (ONC) found many anomalously bright boulders on the dark surface of the carbonaceous (or C-type) asteroid Ryugu...
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...
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...
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...
Detection of TiO and Na in the atmosphere of the hot Jupiter HAT-P-65b
We present the low-resolution transmission spectra of the puffy hot Jupiter HAT-P-65b (0.53 MJup, 1.89 RJup, Teq = 1930 K), based on two transits observed using...