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.

  • Publication
    Quantifying the AGN-driven outflows in ULIRGs (QUADROS) IV: HST/STIS spectroscopy of the sub-kpc warm outflow in F14394+5332
    Considerable uncertainties remain about the nature of warm, AGN-driven outflows and their impact on the evolution of galaxies. This is because the outflows are...
  • Publication
    Quantifying the cool ISM in radio AGNs: evidence for late-time retriggering by galaxy mergers and interactions
    We use deep Herschel observations of the complete 2Jy sample of powerful radio active galactic nuclei (AGNs) in the local Universe (0.05 < z < 0.7) to probe...
  • Grant
    Quasar feedback and molecular gas reservoirs
    The broad scientific objective of this project is to advance in our understanding of active galactic nuclei (AGN) feedback and its connection with the galaxies...
  • Capability
    R&D&I project management
    The development of large and complex scientific instruments has led the IAC to specialize in project management techniques, a discipline to coordinate the human...
  • Publication
    Recovering Age-Metallicity Distributions from Integrated Spectra: Validation with MUSE Data of a Nearby Nuclear Star Cluster
    Current instruments and spectral analysis programs are now able to decompose the integrated spectrum of a stellar system into distributions of ages and...
  • Publication
    Resolving the AGN and Host Emission in the Mid-infrared using a Model-independent Spectral Decomposition
    We present results on the spectral decomposition of 118 Spitzer Infrared Spectrograph (IRS) spectra from local active galactic nuclei (AGNs) using a large set...
  • Publication
    Resolving the Nuclear Obscuring Disk in the Compton-thick Seyfert Galaxy NGC 5643 with ALMA
    We present ALMA Band 6 12CO(2–1) line and rest-frame 232 GHz continuum observations of the nearby Compton-thick Seyfert galaxy NGC 5643 with angular resolutions...
  • Project
    SCIDAR
    SCIntillation Detection And Ranging and Wave Front Sensor. The SCIDAR instrument creates profiles of atmospheric turbulence by observing binary stars.
  • Grant
    Science with OSIRIS-REX
    The objective of this project is to fund the activities of our group for the next four years related to our participation in the OSORIS-REx mission, our...