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OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release

  • Authors: Michele T. Bannister, Brett J. Gladman, J. J. Kavelaars, Jean-Marc Petit, Kathryn Volk, Ying-Tung Chen, Mike Alexandersen, Stephen D. J. Gwyn, Megan E. Schwamb, Edward Ashton, Susan D. Benecchi, Nahuel Cabral, Rebekah I. Dawson, Audrey Delsanti, Wesley C. Fraser, Mikael Granvik, Sarah Greenstreet, Aurélie Guilbert-Lepoutre, Wing-Huen Ip, Marian Jakubik, R. Lynne Jones, Nathan A. Kaib, Pedro Lacerda, Christa Van Laerhoven, Samantha Lawler, Matthew J. Lehner, Hsing Wen Lin, Patryk Sofia Lykawka, Michaël Marsset, Ruth Murray-Clay, Rosemary E. Pike, Philippe Rousselot, Cory Shankman, Audrey Thirouin, Pierre Vernazza, and Shiang-Yu Wang

2018 The Astrophysical Journal Supplement Series 236 18.

  • Provider: AAS Journals

Caption: Figure 1.

Spatial relationship of the regions of sky targeted by OSSOS to the geometry of the outer solar system. The eight sky blocks are indicated by blue wedges, flattened from their low 0°–10° inclinations into the plane (the on-sky projection is shown in Figure 2). The blocks were placed to avoid the dense star fields of the galaxy (schematically indicated by gray shading). Gray dots show the predicted position density of the observable fraction (mr < 24.7) of objects in the 3:2 resonance with Neptune, as modeled by Gladman et al. (2012). Blue dots are the 840 characterized OSSOS discoveries (Table 3), which were found at heliocentric distances between 6 and 83 au. The sensitivity of OSSOS to distant moving objects extends beyond the figure boundaries to ∼100–130 au and is discussed in Section 2.9.

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