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Table 5

Radiometric fit results for the objects sample.

Object Data D [km] pv [%] η Class.
(15874) 1996 TL66 PACS 341  ±  40 1.20  ±  0.35* SDO
(15874) 1996 TL 66 PACS/MIPS 339  ±  20 SDO
(82158) 2001 FP185 PACS 329  ±  42 1.20  ±  0.35* SDO
(82158) 2001 FP 185 PACS/MIPS 4.6  ±  0.7 SDO
(73480) 2002 PN34 PACS 110  ±  12 1.20  ±  0.35* SDO
(73480) 2002 PN 34 PACS/MIPS 112  ±  7 4.9  ±  0.6 SDO
(127546) 2002 XU93 PACS 173  ±  20 1.20  ±  0.35* SDO
(127546) 2002 XU 93 PACS/MIPS 164  ±  9 3.8  ±  0.4 SDO
2007 OR 10 PACS 1280  ±  210 1.20  ±  0.35* SDO
2007 RW 10 PACS 247  ±  30 1.20  ±  0.35* SDO
(65489) Ceto PACS 300  ±  39 1.20  ±  0.35* SDO
(65489) Ceto PACS/MIPS 281  ±  11 5.6  ±  0.6 1.04  ±  0.05 SDO
(42355) Typhon PACS 175  ±  17 1.20  ±  0.35* SDO
(42355) Typhon PACS/MIPS 185  ±  7 4.4  ±  0.3 1.48  ±  0.07 SDO
(40314) 1999 KR 16 PACS 254  ±  37 1.20  ±  0.35* DO
(120132) 2003 FY128 PACS 1.20  ±  0.35* DO
(120132) 2003 FY 128 PACS/MIPS 460  ±  21 7.9  ±  1.0 1.07  ±  0.08 DO
2005 QU 182 PACS 416  ±  73 1.20  ±  0.35* DO
(145480) 2005 TB 190 PACS 464  ±  62 1.20  ±  0.35* DO
2007 OC 10 PACS 309  ±  37 1.20  ±  0.35* DO
(229762) 2007 UK 126 PACS 599  ±  77 1.20  ±  0.35* DO
(136199) Eris PACS 1.20  ±  0.35* DO
(136199) Eris PACS/MIPS 2454  ±  117 84.5  ±  8.8 1.20  ±  0.35* DO

Notes. These are the results obtained by the application of an hybrid-STM to the fluxes obtained by Herschel-PACS (with Spitzer-MIPS data when are available). Preferred results for each target are in bold. Object: SDO or detached object observed with Herschel-PACS (and Spitzer-MIPS when available). Data: PACS, model results using only fluxes from Herschel-PACS. PACS/MIPS, model results using fluxes from Herschel-PACS and Spitzer-MIPS. D [km]: diameter and uncertainty, in kilometres, obtained from the thermal model. pv [%]: geometric albedo and uncertainty, in V-band, obtained from the thermal model.  ⋆  Indicates geometric albedos derived from HR magnitudes instead of HV, (i.e., pr [%]). η: beaming factor from the thermal model application. * Objects for which there are not Spitzer-MIPS fluxes available, in this case we assume a mean η value to perform the radiometric fits. Class., dynamical classification following Gladman et al. (2008). SDO = scattered disc object, DO = detached object.

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