Publication type: Refereed

  • Publication
    A polarization model for the German Vacuum Tower Telescope from in situ and laboratory measurements
    It is essential to properly calibrate the polarimetric properties of telescopes, if one wants to take advantage of the capabilities of high precision spectro...
  • Publication
    A Polarized Accretion Disk Flare in OJ:287
    A very rapid swing in the polarization position angle (PA) in the optical region was observed in blazar OJ 287 during one night of our five nights UBVRI...
  • Publication
    A polarized fast radio burst at low Galactic latitude
    We report on the discovery of a new fast radio burst (FRB), FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time...
  • 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 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...