Publication type: Non-refereed

  • Publication
    Measuring the Magnetic Vector with the He I 10830 Å Line: A Rich New World
    The triplet of the He I transitions around 10830 Å not only shows a rich variety of Stokes profiles, but also allows the full magnetic vector in the upper...
  • Publication
    Measuring the Masses of the TOI-700 Planets with ESPRESSO
    Over the past three decades, astronomers have discovered that small, rocky planets in temperate orbits are common around our neighboring stars. Whether or not...
  • Publication
    Measuring the stellar mass of a z=6.3 submillimeter galaxy
    HerMES, the Herschel/SPIRE extragalactic GTO program, is detecting high redshift sources which were once the domain of high redshift QSOs. Our most spectacular...
  • Publication
    Measuring the true supernova rate in galaxies
    One of the best tracers of massive stars is the rate of supernovae in galaxies. Studies of the supernova rate in galaxies are though severely affected by the...
  • Publication
    Measuring vector magnetic fields in solar prominences
    We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow solar prominence. The data were taken with the Tenerife...
  • Publication
    Mechanical design of ELMER instrument for GTC telescope
    ELMER is an optical instrument for the GTC designed to observe between 370 and 1000 nm. The observing modes for the instrument at Day One shall be: imaging...
  • Publication
    Mechanics of LIRIS (long-slit intermediate-resolution infrared spectrograph) at first commissioning
    LIRIS is a near-infrared intermediate resolution spectrograph with added capabilities for multi-slit, imaging, coronography, and polarimetry, developed by the...
  • Publication
    Medium-Resolution Optical Spectroscopy of Ultracool Dwarfs
    Not Available
  • Publication
    Medium-term Variability in Emission from the Orion Nebula
    Measuring the surface brightness changes in HST images in Hα and [O III]5007 Å taken with a time interval of 6.84 yr, we show how to detect separately the...