Publication type: Refereed

  • Publication
    The red giant branch phase transition: Implications for the RGB luminosity function bump and detections of Li-rich red clump stars
    We performed a detailed study of the evolution of the luminosity of He-ignition stage and of the red giant branch bump luminosity during the red giant branch...
  • Publication
    The red giant branches of Galactic globular clusters in the [(V-I)0,MV] plane: metallicity indices and morphology
    The purpose of this study is to carry out a thorough investigation of the changes in morphology of the red giant branch (RGB) of Galactic globular clusters (GGC...
  • Publication
    The redshift and broad-band spectral energy distribution of NRAO 150
    Context. NRAO 150 is one of the brightest radio and mm AGN sources in the northern sky, and is an interesting source to study extreme relativistic jet phenomena...
  • Publication
    The Redshift Distribution of Flat-Spectrum Radio Sources
    The redshift distribution of flat-spectrum radio sources with 5 GHz flux densities S5>~5 mJy is a key component in using current radio lens surveys to probe the...
  • Publication
    The redshift evolution of galactic bar pattern speed in TNG50
    In this paper, the redshift evolution of the galactic bar properties, like the bar length, pattern speed, and bar fraction, has been investigated for simulated...
  • Publication
    The redshift evolution of major merger triggering of luminous AGNs: a slight enhancement at z ˜ 2
    Active galactic nuclei (AGNs), particularly the most luminous AGNs, are commonly assumed to be triggered through major mergers; however, observational evidence...
  • Publication
    The Redshift of the BL Lac Object TXS 0506+056
    The bright BL Lac object TXS 0506+056 is the most likely counterpart of the IceCube neutrino event EHE 170922A. The lack of this redshift prevents a...
  • Publication
    The reflection nebula around HD 26676
    The gaseous component of the reflection nebula surrounding HD 26676 is investigated by comparing the UV spectrum of the star with that of the foreground star HD...
  • Publication
    The reflective surface of the MAGIC telescope
    The atmospheric Cherenkov telescope MAGIC for ground-based gamma-ray astronomy is operating since late 2003 on the Canary island of La Palma. Its 17 m diameter...