Astrophysical: Ephemerides

  • Publication
    A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole
    Two years after its outburst in 1989, the William Herschel Telescope has been used to find absorption features in V404 Cyg characteristic of a late G or early K...
  • Publication
    CHEOPS observations of the HD 108236 planetary system: a fifth planet, improved ephemerides, and planetary radii
    Context. The detection of a super-Earth and three mini-Neptunes transiting the bright (V = 9.2 mag) star HD 108236 (also known as TOI-1233) was recently...
  • Publication
    Correction to: Precision Ephemerides for Gravitational-wave Searches - IV. Corrected and refined ephemeris for Scorpius X-1
  • Publication
    EURONEAR: Data mining of asteroids and Near Earth Asteroids
    Besides new observations, mining old photographic plates and CCD image archives represents an opportunity to recover and secure newly discovered asteroids, also...
  • Publication
    Period, epoch, and prediction errors of ephemerides from continuous sets of timing measurements
    Space missions such as Kepler and CoRoT have led to large numbers of eclipse or transit measurements in nearly continuous time series. This paper shows how to...
  • Publication
    Precision Ephemerides for Gravitational Wave Searches. II. Cyg X-2
    Accreting neutron stars in low-mass X-ray binaries are candidate high-frequency persistent gravitational wave sources. These may be detectable with next...
  • Publication
    Precision Ephemerides for Gravitational-wave Searches - III. Revised system parameters of Sco X-1
    Neutron stars (NSs) in low-mass X-ray binaries are considered promising candidate sources of continuous gravitational waves. These NSs are typically rotating...
  • Publication
    Precision Ephemerides for Gravitational-wave Searches - IV. Corrected and refined ephemeris for Scorpius X-1
    Low-mass X-ray binaries have long been theorized as potential sources of continuous gravitational-wave radiation, yet there is no observational evidence from...
  • Publication
    Precision Ephemerides for Gravitational-wave Searches. I. Sco X-1
    Rapidly rotating neutron stars are the only candidates for persistent high-frequency gravitational wave emission, for which a targeted search can be performed...