Publication type: Non-refereed

  • Publication
    Determination of Time Dependence in the Temperature Structure of Ionized Interstellar Gas
    It is well known that the temperature structure of ionized interstellar gas departs considerably from homogeneity. This is detected in the form of ``temperature...
  • Publication
    Determining Magnesium and Silicon Abundances from CARMENES Spectra
    The study of chemical abundances of stars that host planets is critical to our current un- derstanding of the structure, formation, evolution of rocky planets...
  • Publication
    Determining the Local Black Hole Mass Function from the Pitch Angles of Nearby Spiral Galaxies
    We present pitch angle measurements of a nearly complete sample of nearby spiral galaxies. Using these results along with the relationship between supermassive...
  • Publication
    Determining the population of Cataclysmic Variables in the Globular Cluster NGC2808
    Close binaries, and in particular cataclysmic variables (CVs), play a vital role in the dynamical evolution of globular clusters. It is, therefore, important to...
  • Publication
    Deterministic Chaos in the Star Formation Rate in the Solar Vicinity
    Not Available
  • Publication
    Development and capabilities of the ISOPHOT interactive analysis (PIA), a package for calibration and astronomical analysis.
    The ISOPHOT Interactive Analysis PIA, is a calibration, scientific analysis and visualization tool for accessing and processing ISOPHOT data. ISOPHOT is one of...
  • Publication
    Development of a 35-micron slicer-based Integral Field Unit for high-resolution 2D solar spectroscopy
    Integral Field Spectropolarimetry (IFS) makes feasible the simultaneous measurement of a 2D field with the use of an Integral Field Unit (IFU). Slicer-based...
  • Publication
    Development of a field-of-view scanning system (FoV-SS): test results and lessons learned
    Here is presented the tests results and the lessons learnt concerning an opto-mechanical device to scan the GREGOR telescope field of view. The scanning is done...
  • Publication
    Development of a network of standard stars for the infrared between 1 and 30 microns
    Not Available