Astrofísicas: Espectroscopia

  • Charla
    The Sloan Digital Sky Survey: News and Prospects from the IAC
    This has been an exciting year for the SDSS-III collaboration. BOSS has made spectacular progress and it is running 6 months ahead of schedule. APOGEE has...
  • Publicación
    The TESS-Keck Survey: Science Goals and Target Selection
    The Kepler and TESS missions have demonstrated that planets are ubiquitous. However, the success of these missions heavily depends on ground-based radial...
  • Publicación
    The Veritas and Themis asteroid families: 5-14 μm spectra with the Spitzer Space Telescope
    Spectroscopic investigations of primitive asteroid families constrain family evolution and composition and conditions in the solar nebula, and reveal...
  • Publicación
    Three-micron spectroscopy of highly reddened field stars.
    Not Available
  • Publicación
    Time-resolved Low-resolution Spectra of BLAP-009 and BLAP-014
    We present time resolved low resolution spectra of BLAP-009 and BLAP-014 collected with SPRAT on the Liverpool Telescope. The spectra were median-stacked in...
  • Publicación
    TOI-1696: A Nearby M4 Dwarf with a 3 R <SUB>⊕</SUB> Planet in the Neptunian Desert
    We present the discovery and validation of a temperate sub-Neptune around the nearby mid-M dwarf TIC 470381900 (TOI-1696), with a radius of 3.09 ± 0.11 R ⊕ and...
  • Publicación
    TOI-954 b and K2-329 b: Short-period Saturn-mass Planets that Test whether Irradiation Leads to Inflation
    We report the discovery of two short-period Saturn-mass planets, one transiting the G subgiant TOI-954 (TIC 44792534, V = 10.343, T = 9.78) observed in TESS...
  • Noticia
    Un congreso en La Palma consolida la colaboración científica en astronomía entre España y China
    Del 25 al 28 de julio, se celebra en Fuencaliente (La Palma) el congreso China-Spain collaboration on astronomical high-resolution spectroscopy que tiene como...
  • Publicación
    Visible spectroscopy of the Polana-Eulalia family complex: Spectral homogeneity
    The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three...