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Table 1:

Observational circumstances.

Object
ra $\Delta$b $\alpha$c Rund Epochse
(#) (Designation) (AU) (AU) ($^\circ$)   B V R i
  1996 RQ 20 39.6 39.0 1.1 C     4  
20161 1996 TR 66 40.3 40.0 1.4 E 2 2 2 2
  1998 HL 151 38.9 38.2 1.0 A 2 2 2 2
181855 1998 WT 31 38.0 37.3 1.0 E 2 2 10 2
  1999 CD 158 47.6 46.5 0.6 E 1 1 24 1
40314 1999 KR 16 36.3 35.6 1.2 B        
  1999 OH 4 39.1 39.6 1.3 A 1 1 1 1
       '' 39.1 38.2 0.6 C 2 2 2 2
  1999 OK 4 46.4 45.8 1.1 A 1 1 1 1
86047 1999 OY 3 40.1 39.7 1.3 A     11  
''        '' 40.2 39.5 1.1 B        
''        '' 40.2 39.4 0.8 D        
86177 1999 RY 215 35.8 34.8 0.2 C     21  
''        '' 35.8 34.8 0.3 D        
  2000 CG 105 46.8 46.1 0.8 E 2 2 22 2
130391 2000 JG 81 34.8 33.8 0.5 A 1 1 1 1
  2001 FU 172 31.8 30.9 1.0 A 1 1 1 1
  2001 QC 298 40.6 39.6 0.3 C     17  
       '' 40.6 39.6 0.2 D        
55565 2002 AW 197 46.6 45.8 0.7 F        
  2002 GH 32 43.1 42.2 0.7 A 3 3 18 3
       '' 43.1 42.4 1.0 B        
55636 2002 TX 300 41.4 40.6 0.8 D        
136108 Haumea 51.1 50.6 1.0 A 1 1 1 1
''        '' 51.1 50.8 1.1 B        
''        '' 51.1 51.1 1.1 F        
  2003 HA 57 32.7 32.0 1.3 A 1 1 1 1
       '' 32.7 32.2 1.6 B        
  2003 HX 56 46.5 45.9 1.0 A 2 2 2 2
120178 2003 OP 32 41.4 40.6 0.6 D        
  2003 QX 91 33.6 32.6 0.5 C     4  
  2003 SQ 317 39.3 38.3 0.6 C     15  
       '' 39.3 38.3 0.4 D        
  2003 TH 58 36.0 35.1 0.5 E 2 2 23 2
       '' 36.0 35.1 0.7 F        
136199 Eris 96.7 95.9 0.4 D        
  2003 UZ 117 39.4 38.9 1.3 D        
  2004 PT 107 38.3 37.9 1.4 A 4 4 24 4
       '' 38.3 37.7 1.3 B        
       '' 38.3 37.4 0.7 D        
120347 2004 SB 60 44.0 43.1 0.6 C     16  
  2005 CB 79 40.1 39.3 0.9 E 1 1 2 1
       '' 40.0 39.2 0.8 F        
  2005 GE 187 30.8 29.9 0.9 A 3 3 33 3
       '' 30.8 30.1 1.3 B        
       '' 30.8 31.1 1.7 C     17  
       '' 30.8 31.3 1.6 D        
202421 2005 UQ 513 48.8 48.1 0.8 C     10  
''        '' 48.8 48.0 0.7 D        

Notes. (a) Heliocentric distance. (b) Geocentric distance. (c) Phase angle. (d) Runs: A = 2008 June 3rd-5th, EFOSC2; B = 2008 June 17th, Hawk-I; C = 2008 August 30th-September 1st, EFOSC2; D = 2008 September 9th, Hawk-I; E = 2008 December 29th-31st, EFOSC2; F = 2009 January 4th, Hawk-I. (e) Number of epochs observed in each filter (for EFOSC2 runs).


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