Formato de una charla: Seminario

  • Charla
    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...
  • Charla
    Peering into the origin of substructures in M31 using planetary nebulae
    Planetary nebulae (PNe) are excellent tracers to study the chemistry, kinematics, and stellar populations of galaxies. They can be used to constrain the...
  • Charla
    Per Aspera ad astar simul: ERASMUS+ mobility and collaboration opportunities with Czech and Slovak institutes
    We will introduce the ERASMUS+ program that offers mobility exchanges between IAC, Czech, and Slovak research institutes and universities. The major part of the...
  • Charla
    Perspectives for speckle cameras at the GTC and WHT
    I will present a short introduction to speckle imaging and the so-called speckle holography technique. Subsequently, I will present results of speckle...
  • Charla
    Photometric study of Pre-Main Sequence Stars in massive star-burst clusters
    Current planet formation theories are bound to comply with the observational constraint that protoplanetary disks have lifetime of ~3 Myr. This timescale is...
  • Charla
    Photometric surveys and BAO & RSD. 2MPZ angular power spectrum
  • Charla
    Photometric surveys and BAO & RSD. Alhambra novel analysis techniques
  • Charla
    Photometric surveys and BAO & RSD. DES angular correlation function
  • Charla
    Physical Characterization of Brown Dwarfs
    The initial mass function describes the distribution of masses for a population of stars and substellar objects when they are born. It defines the evolution of...