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. Author manuscript; available in PMC: 2020 May 22.
Published in final edited form as: Minor Planet Bull. 2019 Jan-Mar;46(1):100–105.

Table I.

Summary of radar-optical opportunities in 2018 July-October. Data from the asteroid lightcurve database (Warner et al., 2009; Icarus 202, 134-146). *The SNRs for 2003 SD220 will be enormous: A: 1.76E+6, G: 96800.

Asteroid Period Amp App Last R SNR
(141053) 2001 XT1 - - - - A 14
NEA G -
(418884) 2008 WM64 - - - - A 1590
NEA G 90
2004 XP14 >100 - 1 2007 A 1850
NEA G 210
433 Eros 5.27 0.08 13+ 2016 A 900
NEA 1.40 G 100
2016 AZ8 - - - - A 1850
NEA G 210
(90403) 2003 YE45 - - - - A *52
NEA June
(454177) 2013 GJ35 - - - - A 43
NEA
(18736) 1998 NU - - - - A 11
NEA
(180186) 2003 QZ30 - - - - A 14
NEA
(419880) 2011 AH37 - - - - A 40
NEA
(137805) 1999 YK5 3.930 0.09 2 2016 A 55
NEA 0.38
2013 CW32 - - - - A 510
NEA G 55
(455176) 1999 VF22 - - - - A 370
NEA G 41
(381677) 2009 BJ81 - - - - A 10
NEA
(162361) 2000 AF6 - - - - A 20
NEA
(86667) 2000 FO10 26 0.7 1 2004 A 32
NEA 1.0
(163081) 2002 AG29 19.70 0.25 1 2011 A 299
NEA G 26
(88254) 2001 FM129 - - - - A 300
NEA G 33
(5189) 1990 UQ 6.676 1.02 1 2017 A *11
NEA July