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Detailed Analysis of the Asteroid Pair (6070) Rheinland and (54827) 2001 NQ8

  • Authors: David Vokrouhlický, Petr Pravec, Josef Ďurech, Kamil Hornoch, Peter Kušnirák, Adrián Galád, Jan Vraštil, Hana Kučáková, Joseph T. Pollock, Jose Luis Ortiz, Nicolas Morales, Ninel M. Gaftonyuk, Donald P. Pray, Yurij N. Krugly, Raguli Ya. Inasaridze, Vova R. Ayvazian, Igor E. Molotov, and Carlos A. Colazo

2017 The Astronomical Journal 153 270.

  • Provider: AAS Journals

Caption: Figure 1.

Statistical quality of Rheinland’s pole solutions shown in a sinusoidal projection of the sky in ecliptic coordinates. The color coding, and the scale bar on the right, indicates the value of ﹩{\chi }^{2}﹩ value normalized by the number of observations. The globally best-fit solution at ﹩(\lambda ,\beta )=(124^\circ ,-87^\circ )﹩ (full circle) has ﹩{\chi }^{2}=1.4﹩ (normalized by the 4021 data points). The solid line delimits solutions within the formal ﹩3\sigma ﹩ confidence zone and represents our region of admissible solutions (see the main text for details).

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