Table I.
Summary of radar-optical opportunities for the current quarter. Period and amplitude data are from the asteroid lightcurve database (Warner et al., 2009; Icarus 202, 134–146). SNR values are estimates that are affected by radar power output along with rotation period, size, and distance. They are given for relative comparisons among the objects in the list.
| Asteroid | Period | Amp | App | Last | R | SNR |
|---|---|---|---|---|---|---|
| (437316) 2013 OS3 | – | – | – | – | A | 32 |
| NEA | G | – | ||||
| 2012 RK15 | – | – | – | A | 260 | |
| NEA | G | 90 | ||||
| (163373) 2002 PZ39 | – | – | – | – | A | 800 |
| NEA | G | 270 | ||||
| (35107) 1991 VH | 2.623 | 0.08 | 5 | 2014 | A | – |
| NEA BIN | 0.15 | G | – | |||
| 2011 EH | – | – | – | – | A | 890 |
| NEA | G | 300 | ||||
| 2017 BM123 | 2.150 | 0.37 | 1 | 2017 | A | 105 |
| NEA NHATS | G | 35 | ||||
| 2015 RH2 | – | – | – | – | A | 7 |
| NEA NHATS | G | – | ||||
| (65690) 1991 DG | – | – | – | – | A | 35 |
| NEA | G | – |