Browsing by Author "Horner, J."

Now showing items 1-2 of 2

    • Does the presence of planets affect the frequency and properties of extrasolar kuiper belts? Results from ... 
      Moro Martín, A.; Marshall, J. P.; Kennedy, G.; Sibthorpe, B.; Mattheus, B. C.; Eiroa, C.; Wyatt, M. C.; Lestrade, J. F.; Maldonado, J.; Rodríguez, D.; Greaves, J. S.; Montesinos, B.; Mora, A.; Booth, M.; Duchene, G.; Wilner, D.; Horner, J. (The American Astronomical Society, 2015)
      The study of the planet–debris disk connection can shed light on the formation and evolution of planetary systemsand may help “predict” the presence of planets around stars with certain disk characteristics. In preliminary ...
    • Signals embedded in the radial velocity noise Periodic variations in the τ Ceti velocities 
      Tuomi, M.; Jones, H. R. A.; Jenkins, James Stewart; Tinney, C. G.; Butler, R. P.; Vogt, S. S.; Barnes, J. R.; Wittenmyer, R. A.; O’Toole, S.; Horner, J.; Bailey, J.; Carter, B. D.; Wright, D. J.; Salter, G. S.; Pinfield, D. (EDP Sciences, 2013)
      Context. The abilities of radial velocity exoplanet surveys to detect the lowest-mass extra-solar planets are currently limited by a combination of instrument precision, lack of data, and “jitter”. Jitter is a general ...