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Table 1

Trans-Neptunian objects studied in this paper.

Name kp:k LY07 GL08 GL12 SH16 BA16 a 0 η 0 −2πJ ω

2001 KG76 4:9 × 51.718 0.939 0.02 2.668 34.017

(42301) 2001 UR163 4:9 × 51.719 0.958 0.04 6.148 36.974

(95625) 2002 GX32 3:7 × 52.987 0.901 0.07 3.359 33.146

2002 CZ248 3:7 52.987 0.919 0.026 5.252 32.413

(131696) 2001 XT254 3:7 × 52.988 0.946 0.04 3.294 35.910

(181867) 1999 CV118 3:7 × 52.988 0.949 0.04 2.650 37.493

(79978) 1999 CC158 5:12 × 53.991 0.904 0.017 1.841 39.096

(119878) 2002 CY224 5:12 × 53.991 0.896 0.011 2.689 35.275

(84522) 2002 TC302 2:5 × 55.474 0.784 0.13 1.585 39.002

(26375) 1999 DE9 2:5 × 55.478 0.897 0.18 2.884 32.283

(60621) 2000 FE8 2:5 × 55.479 0.909 0.05 2.739 33.109

(38084) 1999 HB12 2:5 × 55.480 0.890 0.105 1.052 32.615

2004 KZ18 2:5 55.480 0.847 0.0015 0.136 34.310

2004 EG96 2:5 55.481 0.871 0.045 0.185 32.110

2002 GP32 2:5 × 55.481 0.907 0.0013 0.463 32.081

2000 SR331 2:5 × 55.481 0.896 0.023 3.812 31.157

(143707) 2003 UY117 2:5 × 55.481 0.899 0.064 1.895 32.510

(135571) 2002 GG32 2:5 × 55.481 0.907 0.03 4.140 35.905

(69988) 1998 WA31 2:5 × 55.481 0.890 0.12 5.571 31.581

(119068) 2001 KC77 2:5 × 55.482 0.913 0.24 3.239 35.455

2004 HO79 2:5 55.482 0.907 0.08 2.359 32.507

2001 XQ254 2:5 × 55.484 0.894 0.19 0.189 31.089

2015 GP50 2:5 ×

2012 FH84 2:5 ×

(82075) 2000 YW134 3:8 × 57.920 0.909 0.00035 5.489 41.146

2004 XR190 3:8 ×

2015 FJ345 1:3 × 62.649 0.809 0.065 1.391 50.905

(136120) 2003 LG7 1:3 × 62.660 0.817 0.5 5.913 32.483

2015 KH162 1:3 ×

2013 FQ28 1:3 ×

(160148) 2001 KV76 2:7 × 69.430 0.835 0.076 4.098 34.421

(126619) 2002 CX154 3:11 ×

2014 FC69 3:11 ×

2014 FZ71 1:4 × 75.900 0.860 0.035 4.277 56.117

2015 RR245 2:9 82.100 0.802 0.075 4.360 33.942

(26181) 1996 GQ21 2:11 ×

2008 ST291 1:6 × 99.453 0.761 0.003 5.721 42.566

(184212) 2004 PB112 5:27 × 107.575 0.713 0.0055 0.158 35.392

Notes. The resonance ratios kp:k are all with Neptune. The references used are abbreviated in LY07 (Lykawka & Mukai 2007), GL08 (Gladman et al. 2008), GL12 (Gladman et al. 2012), SH16 (Sheppard et al. 2016) and BA16 (Bannister et al. 2016). A cross indicates that the object is classified as “resonant”; a star indicates that the article provides also the oscillation amplitude of the resonant angle with its uncertainty. In LY07 and GL12, the star is omitted if the classification is said “insecure”. The right part of the table gives the characteristics of the resonant secular models obtained in this paper: a0 is the reference semi-major axis chosen (au) whereas η0 (no unit) and −2πJ (au2 rad2 yr-1) are the fixed parameters. Finally, ω (rad) and (au) are the current secular argument of perihelion and reference perihelion distance of the object (see Sect. 2.1). Blank fields mean that the object was found non-resonant in the numerical integration starting from the nominal orbit given by AstDyS database. In the particular case of 2014 FZ71, a secular model was developed although the nominal orbital solution was not resonant (see Sect. 3.3). In theory, the 1-sigma error bars would allow it also for 2015 GP50, 2012 FH84 and 2013 FQ28.

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