I will review some theoretical ideas in Cosmology different to the standard "Big Bang": the Quasi-steady State model, Plasma Cosmology model, non-cosmological...
Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
We present a new high-precision parametric strong lensing total mass reconstruction of the Euclid Early Release Observations (ERO) galaxy cluster Abell 2390 at...
Past, present and future of cosmic microwave background observations: implications for cosmology
Since its discovery in 1964, the cosmic microwave background (CMB) has been one of the basic pillars of the cosmological model. However, it is only very...
Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation
The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background...
Precision Measurement of the (e++e-) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
We present a measurement of the cosmic ray (e++e-) flux in the range 0.5 GeV to 1 TeV based on the analysis of 10.6 million (e++e-) events collected by AMS. The...
Presentados los últimos avances sobre el Modelo Estándar de Partículas y sus consecuencias para problemas como la materia oscura
HC2NP2019, el segundo congreso "Hadronic Contributions to New Physics Searches", organizado por el Instituto de Astrofísica de Canarias (IAC) en el Puerto de la...
Probing the early Universe with gravitational Wave Background
We will review both theoretical and obsevational aspects of gravitational wave backgrounds of cosmological origin. We will present a classifcation of...
Probing the low surface brightness outskirts of Milky Way dSphs: Sextans
Faint dwarf galaxies such as those found around the Milky Way (MW) display the largest known dynamical mass-to-light ratios (up to several 100s M⊙/L⊙). However...