Líneas de instrumentación: Instrumentación visible

Instrumentación visible

Desde sus orígenes, el Área de Instrumentación ha participado en la construcción de instrumentación para detectar y analizar luz en el rango visible del espectro. Cámaras, espectrógrafos, analizadores de polarización, sistemas alimentados por fibras ópticas, entre otros, han sido diseñados, construidos, integrados y verificados en nuestras instalaciones.

  • Publicación
    Low-metallicity globular clusters in the low-mass isolated spiral galaxy NGC 2403
    The globular cluster (GC) systems of low-mass late-type galaxies, such as NGC 2403, have been poorly studied to date. As a low mass galaxy (M * = 7 × 10 9 M ⊙)...
  • Publicación
    Low-power jet-interstellar medium interaction in NGC 7319 revealed by JWST/MIRI MRS
    We present JWST/MIRI MRS spectroscopy of NGC 7319, the largest galaxy in the Stephan's Quintet, observed as part of the Early Release Observations (ERO). NGC...
  • Publicación
    Lyman-continuum leakage as dominant source of diffuse ionized gas in the Antennae galaxy
    The Antennae galaxy (NGC 4038/39) is the closest major interacting galaxy system and is therefore often studied as a merger prototype. We present the first...
  • Publicación
    Mapping diffuse interstellar bands in the local ISM on small scales via MUSE 3D spectroscopy. A pilot study based on globular cluster NGC 6397
    Context. We map the interstellar medium (ISM) including the diffuse interstellar bands (DIBs) in absorption toward the globular cluster NGC 6397 using VLT/MUSE...
  • Publicación
    Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
    We present spaxel-by-spaxel stellar population fits for the ~10 000 MaNGA data cubes. We provide multiple extension fits files, nominated as MEGACUBES, with...
  • Galería
    MASCARA-2b /KELT-20b Júpiter ultracaliente
    Analizada la atmósfera de un nuevo Júpiter ultracaliente. La combinación de observaciones realizadas con el instrumento CARMENES, instalado en el telescopio de...
  • Publicación
    Mass constraints to Sco X-1 from Bowen fluorescence and deep near-infrared spectroscopy
    More than 50 years after the dawn of X-ray astronomy, the dynamical parameters of the prototypical X-ray binary Sco X-1 are still unknown. We combine a Monte...
  • Blog
    MICRORRELATOS CÓSMICOS: El maquillaje
    Como novedad de 2021, periódicamente publicaremos “Microrrelatos cósmicos”, una nueva categoría dentro de nuestro blog “C/ Vía Láctea, S/N”. Os invitamos a...
  • Publicación
    Modeling the Strongest Silicate Emission Features of Local Type 1 AGNs
    We measure the 10 and 18 μm silicate features in a sample of 67 local (z < 0.1) type 1 active galactic nuclei (AGN) with available Spitzer spectra dominated by...