• Charla
    Observing the polarized microwave sky: 10 years of the QUIJOTE experiment
    I will review the status of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a project led from the IAC with the aim of characterising the polarisation of the...
  • Charla
    Probing the Dark Flow signal in WMAP 9 yr and PLANCK cosmic microwave background maps.
    The ``dark flow'' dipole is a statistically significant dipole found at the position of galaxy clusters in filtered maps of Cosmic Microwave Background (CMB)...
  • Charla
    Road to primordial B-modes -- A strategy for CMB polarization
    Precise measurements of cosmic microwave background (CMB) polarization, especially its odd-parity patterns (B-modes) at large angular scale, prove a scenario of...
  • Charla
    The XLENS Project: Constrain the Initial Mass Function and the Luminous & Dark Matter distribution in massive Early-Type Galaxies
    I will present results from The X-Shooter Lens Survey (XLENS). With XLENS we are unambiguously separate the stellar from the dark-matter content in the internal...
  • Charla
    A Non-inflationary Signature in CMB Anisotropies
    The standard model of cosmology has been quite successful accounting for a broad range of data - at least until the past few years. But as the quality of...
  • Charla
    AGN Feedback in the Cores of Clusters of Galaxies
    Over the past decade there has been a growing body of evidence for a closely regulated balance of heating and cooling of the intracluster medium in the cores of...
  • Charla
    Application of simulation-based inference to problems in astrophysics
    The next decade will see a deluge of new cosmological data that will enable us to accurately map out the distribution of matter in the local Universe, image...
  • Charla
    Astrophysical probes of dark matter
    Dark matter makes up most of the mass of the Universe but remains mysterious. I discuss recent progress in constraining its properties by measuring its...