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Table A.1.

Observational circumstances for the sample of 67 NEOs observed.

Object Date Δ (au) r (au) α
4596 1981 QB 12/02/2016 1.813 2.573 16.8
5370 Taranis 02/05/2016 2.301 3.250 7.2
6050 Miwablock* 12/02/2016 2.458 3.129 15.0
02/05/2016 2.340 3.165 12.2
138852 2000 WN10 10/12/2015 0.289 1.197 37.9
142563 2002 TR69 10/12/2015 1.131 1.804 29.1
154275 2002 SR41 01/07/2014 0.224 1.182 38.8
155110 2005 TB 10/12/2015 0.782 1.526 34.4
159857 2004 LJ1 01/07/2014 1.256 2.080 21.2
162273 1999 VL12 10/12/2015 1.008 1.837 22.6
174806 2003 XL 10/12/2015 1.098 1.965 18.3
194126 2001 SG276 10/12/2015 0.874 1.756 20.3
242708 2005 UK1 01/07/2014 0.535 1.462 27.3
243566 1995 SA 01/07/2014 0.532 1.239 53.5
250706 2005 RR6 06/04/2016 0.689 1.512 32.4
267136 2000 EF104 06/04/2016 0.479 1.448 17.4
333578 2006 KM103 02/07/2016 0.360 1.223 47.8
334412 2002 EZ2* 06/04/2016 0.318 1.306 14.3
02/05/2016 0.403 1.302 36.9
334673 2003 AL18 02/12/2015 0.791 1.722 15.6
356285 2010 DE 06/04/2016 1.012 1.989 8.8
411201 2010 LJ14 02/05/2016 0.614 1.433 36.5
418416 2008 LV16 01/07/2014 0.231 1.206 31.7
430804 2005 AD13 12/02/2016 1.031 1.996 8.4
436771 2012 JG11* 03/06/2016 0.633 1.373 43.7
02/07/2016 0.608 1.370 43.3
441987 2010 NY65 01/07/2014 0.080 1.033 76.2
442243 2011 MD11 10/12/2015 0.808 1.559 33.0
443880 2001 UZ16 10/12/2015 0.446 1.329 33.0
445974 2013 BJ18 13/10/2015 0.690 1.683 5.3
447221 2005 UO5 02/05/2016 0.272 1.114 60.6
451370 2011 AK5 13/10/2015 0.192 1.165 27.2
452397 2002 PD130 02/12/2015 0.492 1.474 5.1
453729 2011 BO24* 12/02/2016 0.622 1.453 32.6
06/04/2016 0.490 1.231 51.3
455199 2000 YK4 10/12/2015 0.479 1.380 28.3
457663 2009 DN1 02/07/2016 0.284 1.156 54.2
458375 2010 WY8* 12/02/2016 0.249 1.209 24.3
06/04/2016 0.274 1.206 37.2
458723 2011 KQ12 12/02/2016 0.414 1.228 46.1
459046 2012 AS10 02/12/2015 1.354 2.328 4.7
463282 2012 HR15 06/04/2016 1.158 1.816 30.2
466508 2014 GY48 06/04/2016 0.582 1.198 56.4
467527 2007 LA15 02/05/2016 0.697 1.680 12.1
468005 2012 XD112 10/12/2015 0.274 1.237 20.4
468452 2003 SD170 02/07/2016 0.338 1.195 50.9
468468 2004 KH17 03/06/2016 0.114 1.055 66.2
468540 2006 MD12 02/07/2016 0.452 1.290 44.2
468741 2010 VM1 02/07/2016 0.234 1.177 42.4
469722 2005 LP40* 03/06/2016 0.530 1.288 48.2
02/07/2016 0.338 1.069 72.1
474238 2001 RU17 02/09/2016 0.164 1.167 15.0
482796 2013 QJ10 13/10/2015 0.531 1.368 37.2
503277 2015 RT83 10/12/2015 0.301 1.159 48.2
1994 CJ1 01/07/2014 0.092 1.063 57.8
1999 VR6 03/06/2016 0.317 1.292 25.4
2001 UG18 30/07/2016 0.302 1.256 32.7
2009 DL46* 06/04/2016 0.159 1.048 68.5
02/05/2016 0.080 1.012 85.0
2009 VY25 02/09/2016 0.293 1.241 33.1
2012 BF86 12/02/2016 0.106 1.067 39.7
2012 CK2 12/02/2016 0.657 1.549 24.1
2012 JR17 02/05/2016 1.095 2.077 8.7
2014 RC11 02/09/2016 0.370 1.333 24.5
2015 OL35 12/02/2016 0.692 1.549 27.4
2015 OS35 02/12/2015 0.675 1.649 7.8
2015 TX143 02/05/2016 0.293 1.086 66.8
2015 YN1 12/02/2016 0.246 1.172 37.0
2016 AF165 12/02/2016 0.343 1.311 16.7
2016 EM28 02/05/2016 0.382 1.289 36.5
2016 GN221 02/07/2016 0.258 1.226 32.2
2016 LY47 02/07/2016 0.420 1.280 43.5
2016 LZ10 30/07/2016 0.197 1.156 40.7
2016 NV 30/07/2016 0.415 1.268 44.6

Notes.

(a)

Notes. Δ and r are the topocentric and the heliocentric distance, respectively. α is the solar phase angle. Objects with an asterisk were observed twice, as explained in the text.

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