Publication type: Non-refereed

  • Publication
    Gas temperature from line broadening in a neon microwave plasma at atmospheric pressure
    We have used the collisional broadening of neutral neon lines to determine the gas temperature of a microwave discharge at atmospheric pressure. The gas...
  • Publication
    Gas, Dust and Star Formation in Nearby Galaxies as Seen with the JCMT
    We combine 12CO J = 3 - 2 for 155 nearby galaxies, obtained as part of the James Clerk Maxwell Telescope (JCMT) Nearby Galaxies Legacy Survey (NGLS), with star...
  • Publication
    GATOS JWST Observations of NGC 5728: Polar Dust
    Recently, mid-infrared (MIR) interferometry and single-dish high angular resolution imaging has revealed the presence of dust in the polar regions of nearby...
  • Publication
    GATOS: A fast multi-channel imager and spectrograph for the Gran Telescopio Canarias
    GATOS (GTC Astrophysical Transient Octuple-channel imaging Spectrograph) is a multi-channel imager and spectrograph capable of simultaneously obtaining images...
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    Gaussian Analysis of the CMB with the Smooth Tests of Goodness of Fit
    The study of the Gaussianity of the cosmic microwave background (CMB) radiation is a key topic to understand the process of structure formation in the Universe...
  • Publication
    Gaveta de Astrofísica
    Como investigadores, trabajamos para la gente. Nuestra carrera científica suele estar financiada con fondos públicos y podemos ayudar a periodistas y...
  • Publication
    GCS component development cycle
    The GTC1 is an optical-infrared 10-meter segmented mirror telescope at the ORM observatory in Canary Islands (Spain). First light was at 13/07/2007 and since...
  • Publication
    GEISHA: Access to raw IRAS data
    Not Available
  • Publication
    Gemini 3D-Spectroscopy of IRAS 17002+5153 and IRAS 07598+6508: Evidence of Two New Exploding BAL + IR + Fe ii QSOs.
    New results of a program to study BAL + IR + FeII QSOs, using Gemini/GMOS-IFU spectroscopy and HST data, are presented for IRAS 17002+5153 and IRAS 07598+6508...