Publication type: Non-refereed

  • Publication
    The deep spectrophotometric mosaic of the Orion Nebula. Preliminary results
    We present a deep spectrophotometric mosaic of the Orion Nebula obtained with the Potsdam Multi-Aperture Spectrophotometer (PMAS) at Calar Alto Observatory. The...
  • Publication
    The Deepest Near-Infrared View of the Universe
    We present very deep near-infrared imaging in the Js, H and Ks-bands of the HDF-S and the field around the z=0.83 cluster MS1054-03 with ISAAC on the VLT. For...
  • Publication
    The Delta Scuti star KW284 in the Praesepe cluster revisited
    As targets of the fourth photometry campaign of the STEPHI network, the Delta Scuti stars BNCnc (HD73576) and BUCnc (HD73763) were simultaneously monitored...
  • Publication
    The DENIS database (Epchtein+, 1999)
    DENIS is a project to survey the all-southern sky in three wavelength bands (Gunn-i 0.82 μm; J, 1.25 μm; and K_s, 2.15 μm) with limiting magnitudes 18.5, 16.5...
  • Publication
    The DENIS database first release (Epchtein+, 1999)
    DENIS is a project to survey the all-southern sky in three wavelength bands (Gunn-i 0.82 μm; J, 1.25 μm; and K_s, 2.15 μm) with limiting magnitudes 18.5, 16.5...
  • Publication
    The Density Profiles of Dark Matter Halos from Dwarf Galaxy Rotation Curves
    Not Available
  • Publication
    The dependence of the Lyman-α Luminosity Function on redshift using SHARDS
    We report in this work on a project aimed at determining Lyα luminosity functions from z=3 to z=6. The project is based on the use of very deep photometry from...
  • Publication
    The design of the WEAVE spectrograph
    WEAVE is the next-generation optical spectroscopy facility for the William Herschel Telescope and aims at spectroscopic follow-up of ground-based (LOFAR) and...
  • Publication
    The Detectability of Dark Galaxies Through Image-Splitting Effects
    In principle, dark galaxies in the dwarf-galaxy mass range may be detectable through additional, small-scale image splitting of quasars that are already known...