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Table 1:

Future observing opportunities of fast rotating VSAs for which periods with $U \geq 2$ are known.
Asteroid Date V $\Delta V$ Asteroid Date V $\Delta V$
    [mag] [mag]     [mag] [mag]
2007 DD 2010-06-04 22.1 (22.1, 22.1) 2001 UF5 2016-04-05 20.1 (27.2, 26.7)
  2011-07-13 20.8 (20.8, 20.8) 2002 GD10 2017-11-02 21.9 (22.0, 21.8)
2000 WN148 2010-12-01 20.5 (18.2, 23.5)   2021-10-23 21.5 (21.7, 21.3)
2000 EB14 2011-02-23 20.2 (22.1, 24.2)   2025-10-15 21.6 (21.3, 21.8)
2008 DG4 2011-11-19 18.9 (25.8, 25.3) 2000 UO30 2017-11-12 21.0 (18.8, 22.3)
2007 TU18 2011-12-05 21.6 (23.3, 24.9) 2007 KE 2017-12-19 18.5 (22.9, 22.2)
2000 YA 2011-12-25 15.4 (15.6, 16.5) 2006 XY 2017-12-21 17.0 (14.7, 18.2)
2001 AV43 2013-11-13 18.7 (18.6, 18.9) 2007 LT 2018-06-14 20.6 (23.5, 22.0)
2001 SQ3 2014-03-07 20.7 (20.7, 20.7) 2007 RQ12 2019-09-13 18.0 (24.0, 24.8)
  2015-09-27 20.3 (20.3, 20.3) 2004 FH 2021-02-21 19.9 (20.0, 19.9)
  2021-03-14 18.5 (18.5, 18.5) 2007 DX40 2022 08 27 21.3 (25.8, 26.3)
  2022-10-03 21.5 (21.5, 21.5)   2026-02-25 21.4 (26.2, 26.3)
  2028-03-17 16.2 (16.2, 16.2) 1998 WB2 2024-04-02 18.8 (24.3, 23.8)
2000 HB24 2014-05-01 17.4 (16.9, 18.2) 2000 WQ148 2024 04 11 16.6 (26.1, 23.8)
  2017-06-10 20.0 (20.5, 20.3)   2026 12 12 17.5 (26.0, 27.6)
  2020-07-02 21.6 (19.2, 22.0) 1998 KY26 2024-05-27 20.0 (20.0, 20.0)
  2028-05-17 19.1 (17.7, 19.3) 1995 HM 2025-06-04 19.9 (20.3, 19.5)
  2029-08-06 18.8 (19.4, 18.4) 2007 VV83 2026-11-04 19.9 (19.7, 20.1)
2001 WR5 2016-01-04 19.4 (18.3, 20.5)        


Date is given in the YYYY-MM-DD order and V is the maximum asteroid brightness during the approach, computed from the nominal orbit. $\Delta V$, given as a range, is an estimate of the brightness uncertainty, obtained from variant orbits with $LOV=\pm 3\sigma$.


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