Publication type: Refereed

  • Publication
    A new line list for the A2Σ+ -X2 Π electronic transition of OH
    A new line list for the A2Σ+ -X2 Π electronic transition of OH has been calculated. Line positions have been taken from the literature and refitted with Western...
  • Publication
    A new linelist for the A3Π-X3Σ- transition of the NH free radical
    A new linelist for the A3Π-X3Σ- electronic transition of NH has been prepared using line positions from the literature and calculated line intensities. High...
  • Publication
    A new look inside planetary nebula LoTr 5: a long-period binary with hints of a possible third component
    LoTr 5 is a planetary nebula with an unusual long-period binary central star. As far as we know, the pair consists of a rapidly rotating G-type star and a hot...
  • Publication
    A New Method Based on Artificial Neural Network Techniques for Determining the Fraction of Binaries in Star Clusters
    We present a new method based on artificial neural networks techniques aimed at determining the fraction of binary systems populating star clusters. We address...
  • Publication
    A new method for age-dating the formation of bars in disc galaxies. The TIMER view on NGC1433's old bar and the inside-out growth of its nuclear disc
    The epoch in which galactic discs settle is a major benchmark for testing models of galaxy formation and evolution but remains largely unknown. Once discs...
  • Publication
    A new method for instrumental profile reconstruction of high-resolution spectrographs
    GJ 9827 is a bright, nearby K7V star orbited by two super-Earths and one mini-Neptune on close-in orbits. The system was first discovered using K2 data and then...
  • Publication
    A new method of determining the inclination angle in interacting binaries
    We describe a method of determining the system parameters in non-eclipsing interacting binaries. We find that the extent to which an observer sees the shape of...
  • Publication
    A New Method of Estimating the Mass-to-Light Ratio of the Ursa Minor Dwarf Spheroidal Galaxy
    Dwarf satellite galaxies undergo strong tidal forces produced by the main galaxy potential. These forces disturb the satellite and produce asymmetries in its...
  • Publication
    A new method of measuring centre-of-mass velocities of radially pulsating stars from high-resolution spectroscopy
    We present a radial velocity analysis of 20 solar neighbourhood RR Lyrae and three Population II Cepheid variables. We obtained high-resolution, moderate-to...