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Table 5

Modeling results sorted by modeling technique.

Object Data d [km] p V η
floating-η fits:
1999 TC36 HS
2000 GN171 HS
2002 VE95 HS
2002 XV93 H
2002 XV93 HS
2003 AZ84a HS
2003 VS2a HS
2004 EW95 H
2004 PF115 H
2004 UX10 H
2006 HJ123 H
Huya H
Huya HS
fixed-η fits:
1996 TP66 HS
1999 TC36 H
1999 TC36 HS
2000 GN171 H
2000 GN171 HS
2001 KD77 H
2001 QF298 H
2002 VE95 H
2002 VE95 HS
2002 VR128 H
2002 VU130 H
2002 XV93 H
2002 XV93 HS
2003 AZ84a H
2003 AZ84a HS
2003 UT292 H
2003 VS2 H
2003 VS2a H
2003 VS2a HS
2004 EW95 H
2004 PF115 H
2004 UX10 H
2006 HJ123 H
Huya H
Huya HS
Pluto/Charon H

Notes. “Data” denotes the dataset on which the modeling results are based: “H” equals Herschel data, “HS” equals Herschel and Spitzer data, respectively; diameter, geometric albedo and η are given including respective upper and lower uncertainties. We show all succesful model fit results in order to allow for a comparison of the reliability of the techniques and the data sets. In the case of all fixed-η modeling approaches, η = 1.20 ± 0.35 was applied.

(a)

Using averaged lightcurve observations.

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