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...
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...
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...
Development of acquisition systems based on FPGAs. Applications to QUIJOTE MFI2, TMS, and MKIDs. Participation study in the Litebird satellite
The main objective of this proposal is to provide the instrumentation area of the IAC with the necessary experience to develop and program data acquisition...