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Table 2.

Observational circumstances of the ACOs presented in this work.

ACO Group Telescope Date UT start X r (au) Δ (au) α (°) #a Exp.b (sec) Solar analogue
(6144) JFC-ACO INT 07/02/2015 05:46 1.5 1.512 3.036 3.0 4 700 HD 142801
(6144) JFC-ACO IRTF 14/05/2015 11:31 1.2 3.116 2.120 3.8 16 120 HD 1444821
(18916) JFC-ACO INT 22/07/2015 03:48 1.5 2.494 1.519 8.4 3 900 HD 198273
(30512) JFC-ACO GTC 17/12/2014 04:23 1.1 2.997 2.167 11.9 3 250 SA 98-978
(30512) JFC-ACO INT 02/03/2015 21:32 1.0 2.789 2.186 18.4 3 700 HD 259516
(30512) JFC-ACO IRTF 07/02/2015 08:01 1.0 2.864 1.947 8.8 32 120 HD 56513
(248590) JFC-ACO IRTF 09/04/2016 05:44 1.4 0.885 0.480 89.3 6 120 HD 29714
(315898) JFC-ACO GTC 19/01/2015 05:11 1.1 8.161 7.465 5.1 3 500 SA 102-1081
(347449) JFC-ACO INT 30/12/2014 02:42 1.1 3.290 2.347 5.8 3 900 HD 283886
(347449) JFC-ACO IRTF 09/03/2016 13:45 1.1 3.529 2.724 10.8 15 120 HD 142801
(366186) JFC-ACO GTC 17/12/2014 02:16 1.3 3.691 2.772 6.3 3 500 SA 98-978
(380282) JFC-ACO GTC 17/12/2014 06:09 1.0 4.595 3.928 9.8 3 400 SA 98-978
(397262) JFC-ACO INT 22/07/2015 02:34 1.1 2.744 1.797 9.5 3 1200 HD 206938
(405058) JFC-ACO IRTF 03/05/2016 11:33 1.3 2.858 1.869 4.9 36 120 SA 107-998
(465293) JFC-ACO GTC 17/12/2014 01:49 1.4 2.262 1.379 14.1 3 300 SA 98-978
2002 RP120 Damocloid INT 17/09/2002 05:31 1.2 2.482 1.988 22.7 5 900 Hyades 64
2002 RP120 Damocloid TNG 20/09/2002 05:17 1.3 2.480 1.928 22.1 6 240 Hyades 64
2005 NA56 JFC-ACO INT 07/02/2015 05:32 1.4 1.608 0.627 6.1 4 800 HD 79078
P/2006 HR30 Damocloid WHT 25/07/2006 01:49 1.1 2.413 1.618 18.3 3 900 SA 112-1333
2006 EX52 Damocloid WHT 25/12/2006 20:49 1.1 2.626 1.789 13.6 2 600 Hyades 64
2007 DA61 Damocloid WHT 10/03/2007 00:02 1.2 2.659 1.810 13.5 3 900 SA 102-1081
2009 FW23 Damocloid WHT 10/04/2009 21:16 1.3 1.783 0.960 25.2 3 300 SA 102-1081

Notes. Information shown in this table includes the airmass (X), heliocentric (r) and geocentric (Δ) distances and phase angle (α) at the time of the observation.

(a)

Column # is the number of exposures in the case of visible observations and the number of individual exposures taken in position A and B (AB) in the case of NIR observations.

(b)

Integration time of individual exposures (or AB in the case of NIR observations).

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