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. Author manuscript; available in PMC: 2020 Apr 30.
Published in final edited form as: Minor Planet Bull. 2020 Jan;47(1):37–41.

Table II.

Observing circumstances. The phase angle (α) is given at the start and end of each date range. LPAB and BPAB are the average phase angle bisector longitude and latitude (see Harris et al., 1984). The P2/P3 lines for 4495 Dassanowsky are for a secondary and tertiary period.

Number Name 20xx/mm/dd Phase LPAB BPAB Period(h) P.E. Amp A.E.
1268 Libya 19/09/07–09/11 1.5,0.4 350 0 17.572 0.009 0.20 0.01
2018 September-October
4495 Dassanowsky 18/09/16–10/19 4.3,5.9 327 3 502 3 0.21 0.02
P2 18.523 0.004 0.13 0.02
P3 (Monomodal) 2.631 0.001 0.05 0.01
P3 (Bimodal) 5.262 0.001 0.06 0.01
2019 September
4495 Dassanowsky 19/09/07–09/25 14.9,11.9 41 1 431 3 0.32 0.02
P2 18.10 0.02 0.05 0.01
P3 5.95 0.01 0.02 0.01
15373 1996 WV1 19/09/08–09/11 3.1,2.5 352 7 6.006 0.004 0.49 0.05