Table 3
Characteristics of the catalogues from the observations that covered the sky paths of TNOs.
Target ID | #Frames | Complete | #Entries | σ α ∗ σ δ | Proper motions (%) | f0 (%) | Predictions | ||||
R | (mas) | UC4 | 2M | UB1 | 2012.5 | 2013 | 2014 | ||||
|
|||||||||||
(8405) Asbolus | 103 | 18.5 | 218 863 | 50 53 | 15.7 | 39.3 | 31.7 | 97.7 | 34 | 48 | 40 |
(24835) 1995 SM55 | 52 | 19.0 | 54 357 | 51 53 | 16.2 | 37.1 | 28.5 | 96.4 | 7 | 7 | 8 |
(10199) Chariklo | 131 | 19.0 | 2 986 471 | 56 56 | 6.6 | 34.4 | 8.7 | 96.2 | 415 | 768 | 689 |
(26375) 1999 DE9 | 39 | 19.0 | 24 340 | 49 49 | 13.9 | 32.9 | 32.9 | 96.2 | 1 | 3 | 7 |
(47171) 1999 TC36 | 58 | 20.0 | 43 333 | 49 48 | 9.2 | 22.4 | 27.9 | 91.4 | 4 | 8 | 4 |
(38628) Huya | 67 | 19.5 | 97 374 | 49 48 | 11.1 | 26.0 | 32.3 | 96.1 | 11 | 12 | 10 |
(54598) Bienor | 122 | 19.0 | 96 379 | 49 51 | 16.8 | 32.5 | 32.3 | 96.0 | 27 | 17 | 21 |
(55565) 2002 AW197 | 40 | 18.0 | 19 381 | 52 52 | 21.7 | 38.8 | 21.1 | 96.3 | 6 | 3 | 3 |
(55576) Amycus | 98 | 18.5 | 2 704 031 | 56 55 | 6.1 | 28.6 | 9.7 | 93.7 | 655 | 601 | 540 |
(83982) Crantor | 87 | 19.5 | 2 952 104 | 56 56 | 4.9 | 12.1 | 14.4 | 92.3 | 1240 | 622 | 257 |
(119951) 2002 KX14 | 21 | 19.0 | 149 784 | 54 53 | 6.8 | 31.9 | 29.6 | 96.7 | 21 | 48 | 40 |
(307261) 2002 MS4 | 42 | 19.0 | 887 401 | 58 58 | 1.7 | 45.7 | 1.5 | 95.0 | 55 | 130 | 125 |
(84522) 2002 TC302 | 44 | 19.5 | 48 318 | 48 48 | 12.1 | 25.1 | 25.0 | 95.2 | 1 | 8 | 7 |
(55637) 2002 UX25 | 43 | 19.5 | 26 332 | 49 48 | 13.0 | 30.9 | 30.9 | 93.5 | 0 | 5 | 5 |
(55638) 2002 VE95 | 67 | 19.5 | 174 945 | 51 49 | 12.8 | 27.2 | 31.9 | 97.4 | 9 | 19 | 17 |
(119979) 2002 WC19 | 27 | 19.0 | 103 449 | 51 51 | 13.3 | 34.1 | 29.8 | 98.1 | 16 | 27 | 12 |
(120132) 2003 FY128 | 36 | 19.0 | 38 338 | 49 49 | 12.1 | 24.9 | 27.0 | 95.5 | 5 | 4 | 8 |
(174567) 2003 MW12 | 46 | 18.5 | 141 589 | 50 50 | 10.3 | 31.2 | 39.3 | 97.2 | 15 | 17 | 20 |
(120178) 2003 OP32 | 50 | 19.5 | 59 373 | 49 48 | 12.7 | 27.6 | 39.7 | 96.4 | 4 | 10 | 6 |
2003 UZ413 | 46 | 19.5 | 28 386 | 48 47 | 13.0 | 31.9 | 25.0 | 94.1 | 3 | 2 | 4 |
(84922) 2003 VS2 | 52 | 19.0 | 154 542 | 53 55 | 11.0 | 45.2 | 23.5 | 97.4 | 8 | 21 | 26 |
(90568) 2004 GV9 | 45 | 19.0 | 91 313 | 48 48 | 11.3 | 27.5 | 36.4 | 97.2 | 5 | 10 | 9 |
2004 NT33 | 73 | 19.0 | 233 652 | 52 51 | 13.0 | 25.4 | 35.7 | 98.1 | 20 | 34 | 35 |
(175113) 2004 PF115 | 47 | 19.5 | 39 361 | 50 47 | 11.4 | 25.8 | 41.9 | 94.7 | 3 | 4 | 4 |
(120347) Salacia | 53 | 19.0 | 53 301 | 49 49 | 14.2 | 31.5 | 30.7 | 96.0 | 4 | 2 | 5 |
(120348) 2004 TY364 | 60 | 20.0 | 37 313 | 50 50 | 11.2 | 27.5 | 31.8 | 91.1 | 9 | 6 | 6 |
(144897) 2004 UX10 | 47 | 19.0 | 25 330 | 50 50 | 13.8 | 32.2 | 27.9 | 92.4 | 4 | 2 | 5 |
2005 CC79 (2011 FX62) | 91 | 18.5 | 100 177 | 49 48 | 13.2 | 32.3 | 34.7 | 96.5 | 9 | 29 | 23 |
(303775) 2005 QU182 | 39 | 19.5 | 19 736 | 51 49 | 11.1 | 29.2 | 34.5 | 91.2 | 2 | 3 | 4 |
(145451) 2005 RM43 | 40 | 18.5 | 35 313 | 50 49 | 15.8 | 43.4 | 19.4 | 96.4 | 5 | 4 | 5 |
(145452) 2005 RN43 | 44 | 19.5 | 43 316 | 49 47 | 12.1 | 28.9 | 32.9 | 96.2 | 4 | 6 | 6 |
(145453) 2005 RR43 | 50 | 19.5 | 42 344 | 48 48 | 13.3 | 33.5 | 28.7 | 95.9 | 4 | 6 | 5 |
(202421) 2005 UQ513 | 49 | 19.0 | 47 355 | 50 51 | 18.1 | 31.5 | 32.9 | 96.3 | 2 | 4 | 6 |
2007 JH43 | 24 | 19.0 | 99 340 | 50 50 | 10.5 | 26.9 | 34.1 | 97.0 | 12 | 24 | 25 |
(278361) 2007 JJ43 | 34 | 19.0 | 231 336 | 50 49 | 7.5 | 28.5 | 26.7 | 97.5 | 15 | 38 | 27 |
(225088) 2007 OR10 | 15 | 19.5 | 16 362 | 49 50 | 12.4 | 26.4 | 38.7 | 96.9 | 6 | 4 | 3 |
(229762) 2007 UK126 | 51 | 20.0 | 55 328 | 51 49 | 11.8 | 29.1 | 27.0 | 95.4 | 2 | 6 | 3 |
2008 OG19 | 45 | 19.0 | 144 725 | 51 51 | 9.7 | 24.6 | 38.9 | 97.6 | 24 | 36 | 20 |
2010 EK139 | 60 | 19.0 | 126 373 | 50 50 | 12.1 | 29.9 | 37.0 | 97.1 | 12 | 17 | 9 |
Notes. Column 1: TNO ID; Col. 2: total number of WFI frames used to cover the sky path of the respective TNO from 2012.5 to the end of 2014; Col. 3: magnitude completeness; Col. 4: total number of entries for all three catalogues with positions and proper motions (WFI catalogues, see text); Cols. 5 and 6: standard deviation of the offsets (observed minus catalogue position) in right ascension and declination, respectively, for the UCAC4 stars; Cols. 7 to 9: per cent of stars whose proper motions came directly from the UCAC4 or from a combination between the observed (WFI) position and either 2MASS or USNO-B1; Col. 10: per cent of stars in the positions and proper motions catalogue that have f0 for quality astrometry. Flags range from 0 (f0: good astrometry) to 5 (f5: position derived from one measurement only). The lower the flag number, the more reliable the position (see Assafin et al. 2010, 2012 for further details); Cols. 11 to 13: number of predicted events per year. No selection was made in this counting so that, for instance, occultations occurring during daylight were also considered.
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