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Table 1

Herschel in-band fluxes at all three PACS bands for the “new” objects, and for two objects with updated fluxes, presented in this work.

Object Dyn. OBSID tOBS JD rh Δ α F70 F100 F160
cl. (sec) (day) (AU) (AU) (deg) (mJy) (mJy) (mJy)
(26181) 1996 GQ21 SDO 1342212818/...821 5656 2455579.43 41.6056 41.9751 1.26 4.51 ± 1.01 6.78 ± 1.28 7.53 ± 2.15
1342213075/...078 5656 2455580.23 41.6063 41.9628 1.26
(523588) 2000 CN105 Res 9:5 1342197691/...694 3400 2455351.20 46.5639 46.6134 1.25 <1.31 <1.50 <1.63
1342197781/...784 3400 2455352.41 46.5641 46.6340 1.25
(82075) 2000 YW134 Res 8:3 1342196008/...011 4528 2455325.61 44.2099 44.3812 1.30 4.88 ± 1.07 5.13 ± 1.47 4.88 ± 2.13
1342196133/...036 4528 2455326.83 44.2105 44.4024 1.29
1342187074 5666 2455154.17 44.1263 43.8338 1.25
(82155) 2001 FZ173 SDO 1342236630/...633 4528 2455933.26 32.4131 32.5753 1.72 8.51 ± 1.54 7.91 ± 1.77 5.01 ± 2.46
1342236908/...011 4528 2455934.17 32.4132 32.5596 1.73
(139775) 2001 QG298 Plutino 1342213211/...214 5656 2455585.66 31.7619 32.1381 1.64 <0.913 <1.19 <2.00
1342213266/...269 5656 2455586.32 31.7619 32.1489 1.64
2001 QX322 SDO 1342211619/...622 5656 2455557.80 41.3329 41.0520 1.32 <0.99 <1.06 <1.51
1342211807/...010 5656 2455558.58 41.3336 41.0646 1.32
(42301) 2001 UR163 SDO 1342199507/...510 2272 2455378.59 50.9591 51.3267 1.07 2.88 ± 1.37 <1.69 <3.09
1342199650/...653 2272 2455380.07 50.9601 51.3042 1.08
(126154) 2001 YH140 Res 5:3 1342206036/...039 3400 2455477.34 36.6150 36.9327 1.49 5.08 ± 1.40 3.67 ± 1.70 <1.95
1342206056/...059 3400 2455478.10 36.6151 36.9203 1.49
1342187062 5666 2455153.28 36.5768 36.1686 1.44
(119878) 2002 CY224 Res 12:5 1342195506/...509 3400 2455311.51 37.2072 36.8614 1.47 <1.59 <1.78 <2.1
1342195610/...613 3400 2455313.49 37.2082 36.8945 1.49
2002 GP32 Res 5:2 1342204144/...147 3400 2455448.42 32.1569 32.3768 1.76 3.09 ± 0.95 5.43 ± 1.53 3.58 ± 1.29
1342204204/...207 3400 2455449.05 32.1570 32.3875 1.75
(133067) 2003 FB128 Plutino 1342237146/...149 4528 2455938.19 34.2390 34.6867 1.47 3.22 ± 0.90 3.80 ± 1.44 <1.94
1342237226/...229 4528 2455938.85 34.2395 34.6769 1.47
(469505) 2003 FE128 Res 2:1 1342237150/...153 5656 2455938.25 35.8635 36.3139 1.40 3.08 ± 1.00 <1.39 <2.51
1342237230/...033 5656 2455938.91 35.8635 36.3037 1.41
(143707) 2003 UY117 Res 5:2 1342238745/...746 3392 2455965.35 32.8901 33.1340 1.67 6.13 ± 0.76 <2.16
1342238790/...791 3392 2455965.98 32.8903 33.1447 1.66
(455502) 2003 UZ413 Plutino 1342212760/...763 2272 2455578.11 42.6153 42.2946 1.26 21.49 ± 1.45 17.02 ± 1.71 14.82 ± 3.53
1342212858/...861 2272 2455579.85 42.6162 42.3239 1.27
(450265) 2003 WU172 Plutino 1342250794/...797 2836 2456180.54 29.6443 29.8432 1.91 6.29 ± 1.40 9.44 ± 1.38 3.92 ± 1.87
1342250830/...833 2836 2456181.36 29.6441 29.8292 1.92
(175113) 2004 PG115 SDO 1342219009/...012 2256 2455670.53 36.9594 37.3635 1.43 6.68 ± 2.39 8.43 ± 3.03 <3.15
1342219048/...051 2256 2455671.09 36.9596 37.3554 1.44
(145451) 2005 RM43 SDO 1342202281/...284 2272 2455417.29 35.4298 35.6640 1.60 15.20 ± 1.18 16.55 ± 2.87 14.79 ± 2.41
1342202320/...323 2272 2455417.99 35.4301 35.6527 1.60
(308379) 2005 RS43 Res 2:1 1342213502/...505 4528 2455592.24 42.4029 42.7677 1.24 3.09 ± 0.94 3.45 ± 1.46 <1.83
1342213558/...561 4528 2455593.00 42.4033 42.7805 1.24

(40314) 1999 KR16 (**) DO 1342212814/...817 5844 2455579.36 35.7593 36.0633 1.51 7.61 ± 1.44 5.21 ± 2.29 <1.98
1342213071/...074 5844 2455580.16 35.7589 36.0497 1.51
(303775) 2005 QU182 (*) SDO 1342212619/...622 2460 2455576.11 48.8994 49.1349 1.13 4.41 ± 1.28 6.94 ± 2.11 <2.73
1342212696/...699 2460 2455577.08 48.9008 49.1522 1.12

Notes. Column headings (from left to right): object name; dynamical classification (Res: resonant, SDO: scattered disk object, DO: detached object); OBSID: observation identifiers in the Herschel Science Archive; tOBS: total duration of the two visits; JD: measurement mid-time in Julian date; rh : heliocentric distance; Δ: observer-to-target distance; α: phase angle; F70, F100, and F160 : in-band flux densities obtained in the PACS 70, 100, and 160 μm bands, respectively. Upper limits correspond to 2σ uncertainties derived with the implanted source method (Vilenius et al. 2014; Kiss et al. 2014). (*) Target from Santos-Sanz et al. (2012) and (**)target from Vilenius et al. (2018) reanalyzed with the latest version of our data reduction pipeline.

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