Publication type: Refereed

  • 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...
  • Publication
    A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO
    Context. Imaging atmospheric Cherenkov telescopes (IACTs) are used to observe very high-energy photons from the ground. Gamma rays are indirectly detected...
  • Publication
    A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling technique
    We present a new non-convex model of the binary asteroid (809) Lundia. A SAGE (Shaping Asteroids with Genetic Evolution) method using disc-integrated photometry...
  • Publication
    A new observational strategy in search for solar g-modes
    The aim of the present work is the detection of solar g-modes, by means of a new observational strategy based on the exploitation of their spatial and temporal...
  • Publication
    A new perspective on the stellar mass-metallicity relation of quiescent galaxies from the LEGA-C survey
    We investigated the stellar mass-metallicity relation (MZR) using a sample of 637 quiescent galaxies with 10.4 ≤ log(M */M ⊙) < 11.7 selected from the LEGA-C...
  • Publication
    A new planetary nebula in the outer reaches of the Galaxy
    Aims: A proper determination of the abundance gradient in the Milky Way requires the observation of objects at large galactiocentric distances. With this aim...
  • Publication
    A New Pleiades Member at the Lithium Substellar Boundary
    We present the discovery of an object in the Pleiades open cluster, named Teide 2, with optical and infrared photometry that places it on the cluster sequence...