Publication type: Refereed

  • Publication
    A Population of Dust-rich Quasars at z ~ 1.5
    We report Herschel SPIRE (250, 350, and 500 μm) detections of 32 quasars with redshifts 0.5
  • Publication
    A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions
    Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 au) on the formation and evolution of...
  • Publication
    A possible binary AGN in Mrk 622?
    Mrk 622 is a Compton thick active galactic nuclei (AGN) and a double-peaked narrow emission line galaxy, thus a dual AGN candidate. In this work, new optical...
  • Publication
    A possible black hole in the γ-ray microquasar LS 5039
    The population of high-energy and very high-energy γ-ray sources, detected with EGRET and the new generation of ground-based Cherenkov telescopes, forms a...
  • Publication
    A possible low-mass type Ia supernova
    IN the standard model for type Ia supernovae1, a massive white dwarf in a binary system accretes matter from the companion star until it reaches the...
  • Publication
    A possible misaligned orbit for the young planet AU Mic c
    The AU Microscopii planetary system is only 24 Myr old, and its geometry may provide clues about the early dynamical history of planetary systems. Here, we...
  • Publication
    A possible origin of the mass-metallicity relation of galaxies
    Observations show that galaxies follow a mass-metallicity relation over a wide range of masses. One currently favoured explanation is that less massive galaxies...
  • Publication
    A Possible Relationship between Quasars and Clusters of Galaxies
    The distribution on the sky of clusters of galaxies shows significant association with relatively nearby, large, active galaxies. The pattern is that of...
  • Publication
    A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
    Dwarf galaxies are excellent cosmological probes, because their shallow potential wells make them very sensitive to the key processes that drive galaxy...