| Objecta | (B-V) | (V-R) | (R-I) | (R-J) | (J-HS) | Vis. slope | Ref.b | Family? | |
| # | Designation | (mag) | (mag) | (mag) | (mag) | (mag) | (%/100 nm) | ||
| 24835 | 1995 SM 55
|
0.65 
0.01
|
|
0.36
0.02
|
0.65
0.03
|
- | 2.0
0.8
|
1-8 | Y |
| 1996 RQ 20 | 0.96
0.13
|
0.46
0.05
|
0.71
0.12
|
- | - | 22.4
6.8
|
9, 10 | N | |
| 19308 | 1996 TO 66
|
0.68
0.02
|
0.39
0.01
|
0.37
0.02
|
0.61
0.10
|
- | 2.9
0.5
|
1, 10-14 | Y |
| 1998 HL 151 | 0.67
0.18
|
0.42
0.16
|
0.79
0.31
|
- | - | 18.1
16.9
|
15, 16, 32 | ? | |
| 181855 | 1998 WT 31 | 0.76
0.32
|
0.51
0.25
|
0.60
0.28
|
- | - | 16.6
5.2
|
32 | N |
| 1999 CD 158 | 0.83
0.06
|
0.51
0.05
|
0.54
0.06
|
1.38
0.09
|
- | 15.8
0.6
|
6, 32 | N | |
| 40314 | 1999 KR 16 | 1.07
0.03
|
0.75
0.02
|
0.74
0.02
|
1.56
0.08c
|
0.56
0.13
|
40.9
6.2
|
9, 16-18, 32 | N |
| 1999 OH 4 | 2.99
0.48
|
0.21
0.20
|
0.44
0.47
|
- | - | 20.2
35.6
|
32 | ? | |
| 86047 | 1999 OY 3
|
0.75
0.03
|
0.26
0.03
|
0.33
0.04
|
0.80
0.12
|
-0.26
0.36
|
-0.5
5.3
|
3, 32 | Y |
| 86177 | 1999 RY 215 | - | - | - | 0.99
0.18
|
0.52
0.22
|
- | 28 | N |
| 2000 CG 105 | 1.11
0.25
|
0.39
0.13
|
0.21
0.22
|
- | - | 6.7
17.5
|
32 | ? | |
| 2001 FU 172 | 2.91
1.53
|
0.66
0.19
|
0.53
0.22
|
- | - | 39.8
27.9
|
32 | N | |
| 2001 QC 298 | 0.66
0.07
|
0.37
0.07
|
0.63
0.07
|
1.06
0.21
|
0.52
0.14
|
9.7
10.0
|
19, 32 | N | |
| 55565 | 2002 AW 197 | 0.93
0.03
|
0.62
0.02
|
0.55
0.02
|
1.16
0.04
|
0.39
0.08
|
22.8
3.5
|
20-22, 32 | N |
| 2002 GH 32 | 0.91
0.06
|
0.66
0.06
|
0.56
0.05
|
- | - | 24.8
4.7
|
19, 23 | N | |
| 55636 | 2002 TX 300
|
0.66
0.02
|
0.36
0.02
|
0.32
0.03
|
- | -0.47
0.13
|
0.2
1.1
|
21, 23, 32 | Y |
| 136108 | Haumea
|
0.64
0.01
|
0.33
0.01
|
0.34
0.01
|
0.88
0.01
|
-0.60
0.11
|
-0.6
0.9
|
21, 24, 25, 32 | Y |
| 2003 HX 56 | 1.27
1.37
|
-0.26
2.07
|
1.28
2.10
|
- | - | 18.4
32.7
|
32 | ? | |
| 120178 | 2003 OP 32
|
0.70
0.05
|
0.39
0.06
|
0.37
0.05
|
- | -0.51
0.08
|
3.4
1.1
|
9, 26, 32 | Y |
| 2003 SQ 317 | - | - | - | 0.43
0.04
|
-0.45
0.20
|
- | 32 | Y | |
| 2003 TH 58 | 0.58
0.12
|
0.29
0.13
|
0.59
0.15
|
-0.13
0.15
|
1.29
0.20
|
3.6
11.4
|
32 | N | |
| 2003 UZ 117
|
- | - | - | - | -0.62
0.12
|
1.1
0.7d
|
22, 27, 28, 32 | Y | |
| 2004 PT 107 | 0.82
0.21
|
0.65
0.10
|
0.68
0.10
|
1.15
0.16
|
0.54
0.22
|
27.9
8.4
|
32 | N | |
| 2005 CB 79 | 0.73
0.04
|
0.37
0.05
|
0.36
0.05
|
0.71
0.08
|
-0.50
0.17
|
3.1
2.5
|
32 | Y | |
| 136472 | Makemake | 0.83
0.02
|
0.5
0.1e
|
0.3
0.1e
|
- | - | 7.7
8.8
|
21, 29 | N |
| 2005 GE 187 | - | - | - | 1.22
0.19
|
0.65
0.14
|
- | 32 | N | |
| 145453 | 2005 RR 43
|
0.77
0.06
|
0.41
0.04
|
0.29
0.08
|
0.48
0.04
|
- | 3.3
6.0
|
8, 22, 26 | Y |
| 202421 | 2005 UQ 513 | - | - | - | 1.39
0.08
|
0.30
0.12
|
18.1
2.0d
|
27, 28, 30, 32 | N |
| 136199 | Eris | 0.78
0.01
|
0.45
0.03
|
0.33
0.02
|
0.52
0.02
|
0.25
0.11
|
5.9
5.6
|
21, 22, 31, 32 | - |
Notes.
(a) There are no
published colours for candidates 1996 TR66, 1997
RX9, 1999 OK4, 2000 JG81,
2003 HA57. For 2003 QX91
and 2004 SB60 we measured R-band
photometry, but not colours. None of these candidates are included in
the table.
(b) References: [1]
Boehnhardt
et al. (2001); [2] Gil-Hutton &
Licandro (2001); [3] Doressoundiram
et al. (2002); [4] McBride et al.
(2003); [5] Tegler
& Romanishin (2003); [6] Delsanti et al. (2004);
[7] Doressoundiram
et al. (2007); [8] Rabinowitz et al.
(2008); [9] Jewitt
& Luu (2001);
[10] Tegler &
Romanishin (1998);
[11] Jewitt et al.
(1998);
[12] Barucci
et al. (1999);
[13] Davies
et al. (2000);
[14] Hainaut
et al. (2000);
[15] Hainaut &
Delsanti (2002);
[16] Trujillo &
Brown (2002);
[17] Sheppard &
Jewitt (2002);
[18] Delsanti
et al. (2006);
[19] Santos-Sanz
et al. (2009); [20] Doressoundiram
et al. (2005a);
[21] Rabinowitz
et al. (2007);
[22] DeMeo et al.
(2009);
[23] Doressoundiram
et al. (2005b);
[24] Rabinowitz
et al. (2006);
[25] Lacerda
et al. (2008);
[26] Perna et al.
(2010);
[27] Pinilla-Alonso
et al. (2007);
[28] Alvarez-Candal
et al. (2008);
[29] Ortiz et al.
(2007);
[30] Fornasier
et al. (2009);
[31] Brown et al.
(2005b);
[32] This work.
Where colours for a given object are published by multiple authors, we
quote a weighted mean.
(c) (R-J)
calculated from near simultaneous R and J
observations by [17] and [18] respectively. No correction is made to
this (or any other colour in the table) for possible differences due to
changes in rotational phase, although [17] show 1999 KR16
to have a light-curve amplitude of 
mag.
(d) Although no
photometry is published, measurements of the spectral slope for these
objects (derived from optical spectra) can be found in Table 2
of Fornasier
et al. (2009). We give a weighted mean for each
object, and list the references to the original papers in the table.
(e) The colours for
Makemake are calculated from the BVI photometry
from [21] along with the R-band photometry from
[26]. We use a phase function of 
mag deg-1 to correct the R-band
photometry to zero phase angle, as [21] show that 
is approximately constant at this value between the V
and I bands. The uncertainty is dominated by the
uncertainty on the R-band photometry.
These objects listed
as confirmed family members by Ragozzine
& Brown (2007).
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