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.

  • Galería
    Centro de Sistemas Ópticos Avanzados (CSOA)
    Instalaciones y equipamiento de CSOA
  • Subvención
    Ciencia con OSIRIS-REX
    El objetivo de este proyecto es financiar las actividades de nuestro grupo para los próximos 4 años en la misión OSORIS-REx y la investigación en la...
  • Publicación
    Circumnuclear Star Formation and AGN Activity: Clues from Surface Brightness Radial Profile of PAHs and [{\rm{S}}\,{\rm{IV}}]
    We studied the circumnuclear mid-IR emission in a sample of 19 local active galactic nuclei (AGNs) with high spatial resolution spectra using T-ReCS (Gemini)...
  • Publicación
    Clear evidence for the early triggering of a luminous quasar-like active galactic nuclei in a major, gas-rich merger
    We present deep, intermediate resolution, long-slit Gemini GMOS-S optical spectra of the Sloan Digital Sky Survey (SDSS) type II quasar J002531-104022, which is...
  • Publicación
    CO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift
    To evaluate the role of radio activity in galaxy evolution, we designed a large archival CO survey of radio galaxies (RGs) to determine their molecular gas...
  • Publicación
    CO kinematics unveil outflows plausibly driven by a young jet in the gigahertz peaked radio core of NGC 6328
    We report the detection of outflowing molecular gas in the center of the nearby (z = 0.014) massive radio galaxy NGC 6328. The radio core of the galaxy, PKS...
  • Publicación
    Cold molecular gas and PAH emission in the nuclear and circumnuclear regions of Seyfert galaxies
    We investigate the relation between the detection of the 11.3 μm polycyclic aromatic hydrocarbon (PAH) feature in the nuclear (∼24-230 pc) regions of 22 nearby...
  • Publicación
    Comparative internal kinematics of the H II regions in interacting and isolated galaxies: implications for massive star formation modes
    We have observed 12 interacting galaxy pairs using the Fabry-Perot interferometer GH αFaS (Galaxy H α Fabry-Perot system) on the 4.2-m William Herschel...
  • Publicación
    Complex AGN feedback in the Teacup galaxy. A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
    Context. The z ∼ 0.1 type-2 QSO J1430+1339, known as the " Teacup", is a complex galaxy showing a loop of ionised gas ∼10 kpc in diameter, co-spatial radio...