However, by carefully keeping track of survey pointings on the sky, detection limits, tracking fractions, and rate cuts, the biases from a survey can be modeled in Survey Simulator software. 6Institut UTINAM, UMR 6213 Centre National de la Recherche Scientifique-Université de Franche Comté, Besançon, FranceĪll surveys include observational biases, which makes it impossible to directly compare properties of discovered trans-Neptunian Objects (TNOs) with dynamical models.5Department of Physics and Astronomy, The University of British Columbia, Vancouver, BC, Canada.4Astrophysics Research Centre, Queen's University Belfast, Belfast, United Kingdom.3Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan.2Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada.
1NRC-Herzberg Astronomy and Astrophysics, National Research Council of Canada, Victoria, BC, Canada.Bannister 4, Brett Gladman 5, Jean-Marc Petit 6 and Cory Shankman 1,2 † Kavelaars 1,2, Mike Alexandersen 3, Michele T.
0 kommentar(er)
