Lines of instrumentation: Visible instrumentation

Visible instrumentation

From its origins, the Instrumentation Division has participated in the construction of instrumentation to detect and analyze light in the visible range of the spectrum. Cameras, spectrographs, polarization analyzers, optical fibers fed systems, among others, have been designed, built, integrated and verified in our facilities.

  • Grant
    UV-sensitive detection system for the OSIRIS instrument in the GTC
  • Grant
    Vacuum equipment, cryogenics and automatic safety control in cryogenic infrastructures
    We propose the acquisition of specific technological equipment for the adaptation and safety control of the IAC infrastructures dedicated to the realization of...
  • Capability
    Valorization of technology and promotion of synergies with the productive environment
    Another purpose of the IAC is to increase the value of the research results generated by the center. The transfer of knowledge for the development of new...
  • Publication
    VLA and ALMA observations of the lensed radio-quiet quasar SDSS J0924+0219: a molecular structure in a 3 μJy radio source
    We present Karl G. Jansky Very Large Array (VLA) and Atacama Large Millimetre Array (ALMA) observations of SDSS J0924+0219, a z = 1.524 radio-quiet lensed...
  • Publication
    VLT FORS2 optical imaging and spectroscopy of nine luminous type 2 AGN at 0.3 < z < 0.6 - I. Ionized gas nebulae
    We present optical imaging and long slit spectroscopic observations of nine luminous type 2 active galactic nuclei (AGN) within the redshift range 0.3 z 0.6...
  • Publication
    Warm molecular and ionized gas kinematics in the type-2 quasar J0945+1737
    We analyse Near-Infrared Integral Field Spectrograph (NIFS) observations of the type-2 quasar (QSO2) SDSS J094521.33+173753.2 to investigate its warm molecular...
  • Project
    WEAVE - WHT Enhanced Area Velocity Explorer
    New multi-object spectrograph planned for the 4.2m William Herschell Telescope (WHT) located in the Observatorio del Roque de los Muchachos, on La Palma island.
  • News
    WEAVE is ready to start operating in La Palma
    All the main components of the new multiobject spectrograph WEAVE on the William Herschel Telescope (WHT) in the Roque de los Muchachos Observatory (Garafía, La...
  • Grant
    WEAVE: Exploring new scientific horizons through spectroscopic surveys.
    The William Herschel Telescope (WHT) has been a key player in the take-off of Spanish astronomy in the last 25 years. With the access of the Spanish community...