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Fig. 3

image

O–C residual distributions taken for orbit determination for comets C/1937 N1 Finsler (upper panels, second-class GR/NG orbits) and C/1942 C1 Whipple-Bernasconi-Kulin (lower panels, first-class GR/NG orbits). For both comets three types of solutions are shown, from left to right: pure GR solution based on non-weighted data, pure GR solution based on weighted data, and NG solution derived using weighted data. The best-fitting Gaussian distributions are shown by magenta dots, each chosen to lie exactly in the middle of a histogram bin.

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