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
    Schwarzschild modelling of barred s0 galaxy NGC 4371
    We apply the barred Schwarzschild method developed by Tahmasebzadeh et al. (2022) to a barred S0 galaxy, NGC 4371, observed by IFU instruments from the TIMER...
  • Proyecto
    SCIDAR
    SCIntillation Detection And Ranging y Sensor de Frente de Onda. El SCIDAR es un instrumento que mide perfiles de turbulencia atmosférica, mediante la...
  • Publicación
    Scrutinizing evidence for the triggering of active galactic nuclei in the outskirts of massive galaxy clusters at z ≈ 1
    Environmental effects are believed to play an important yet poorly understood role in triggering accretion events onto the supermassive black holes (SMBHs) of...
  • Publicación
    SDSS galaxies with double-peaked emission lines: double starbursts or active galactic nuclei?
    With the aim of investigating galaxies with two strong simultaneous starbursts, we have extracted a sample of galaxies with double-peaked emission lines in...
  • Publicación
    Searching for molecular gas inflows and outflows in the nuclear regions of five Seyfert galaxies
    Active galactic nucleus (AGN) driven outflows are believed to play an important role in regulating the growth of galaxies, mostly via negative feedback. However...
  • Publicación
    Serendipitous detection of an overdensity of Herschel-SPIRE 250 μm sources south of MRC 1138-26
    We report the serendipitous detection of a significant overdensity of Herschel-Spectral and Photometric Imaging Receiver 250 μm sources in the vicinity of MRC...
  • Publicación
    SHARDS: An Optical Spectro-photometric Survey of Distant Galaxies
    We present the Survey for High-z Absorption Red and Dead Sources (SHARDS), an ESO/GTC Large Program carried out using the OSIRIS instrument on the 10.4 m Gran...
  • Subvención
    Sistema de detección sensible al UV para el instrumento OSIRIS en el GTC
  • Publicación
    Smooth kinematic and metallicity gradients reveal that the Milky Way's nuclear star cluster and disc might be part of the same structure
    Context. The innermost regions of most galaxies are characterised by the presence of extremely dense nuclear star clusters. Nevertheless, these clusters are not...