Characterisation of candidate members of (136108) Haumea's family

C. Snodgrass; B. Carry; C. Dumas; O. Hainaut

doi:10.1051/0004-6361/200913031

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Volume 511 (February 2010)

A&A, 511 (2010) A72

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Table 3:

Photometry. Mean apparent magnitudes for each object at each epoch.
Object		Run^a	B	V	R	I	J	H_S	$\Delta m_R$ ^b
	1996 RQ 20	C	-	-	22.95 $\pm$ 0.05	-	-	-	-
	1998 HL 151	A	25.37 $\pm$ 0.28	24.25 $\pm$ 0.12	23.87 $\pm$ 0.13	23.08 $\pm$ 0.17	-	-	-
181855	1998 WT 31	E	24.52 $\pm$ 0.15	23.81 $\pm$ 0.11	23.24 $\pm$ 0.06	22.69 $\pm$ 0.14	-	-	0.1
	1999 CD 158	E	23.08 $\pm$ 0.07	22.31 $\pm$ 0.06	21.68 $\pm$ 0.01	21.20 $\pm$ 0.06	-	-	0.6
40314	1999 KR 16	B	-	-	-	-	20.02 $\pm$ 0.07	19.47 $\pm$ 0.10	-
	1999 OH 4	C	25.01 $\pm$ 0.22	22.39 $\pm$ 0.09	22.19 $\pm$ 0.10	21.76 $\pm$ 0.32	-	-	-
86047	1999 OY 3	A,D	-	-	22.26 $\pm$ 0.03	-	21.78 $\pm$ 0.10	22.04 $\pm$ 0.35	0.1
86177	1999 RY 215	C,D	-	-	22.16 $\pm$ 0.01	-	21.19 $\pm$ 0.14	20.66 $\pm$ 0.17	0.1
	2000 CG 105	E	24.14 $\pm$ 0.09	22.60 $\pm$ 0.04	22.62 $\pm$ 0.02	22.52 $\pm$ 0.09	-	-	0.45
	2001 FU 172	A	26.71 $\pm$ 1.52	23.80 $\pm$ 0.15	23.13 $\pm$ 0.12	22.66 $\pm$ 0.19	-	-	-
	2001 QC 298	C,D	-	-	22.18 $\pm$ 0.03	-	21.16 $\pm$ 0.08	20.65 $\pm$ 0.12	0.4
55565	2002 AW 197	F	-	-	-	-	18.50 $\pm$ 0.05	18.11 $\pm$ 0.06	-
	2002 GH 32	A	23.91 $\pm$ 0.09	21.87 $\pm$ 0.05	21.87 $\pm$ 0.02	19.96 $\pm$ 0.09	-	-	0.75
55636	2002 TX 300	D	-	-	-	-	18.67 $\pm$ 0.07	19.14 $\pm$ 0.10	-
136108	Haumea	F	-	-	-	-	16.46 $\pm$ 0.07	17.06 $\pm$ 0.08	-
	2003 HX 56	A	25.25 $\pm$ 0.36	24.03 $\pm$ 0.16	23.68 $\pm$ 0.16	23.42 $\pm$ 0.43	-	-	-
120178	2003 OP 32	D	-	-	-	-	19.08 $\pm$ 0.05	19.58 $\pm$ 0.06	-
	2003 QX 91	C	-	-	23.66 $\pm$ 0.12	-	-	-	-
	2003 SQ 317	C,D	-	-	22.05 $\pm$ 0.02	-	21.59 $\pm$ 0.05	22.04 $\pm$ 0.19	1.0
	2003 TH 58	E	23.50 $\pm$ 0.05	22.89 $\pm$ 0.04	22.51 $\pm$ 0.02	22.03 $\pm$ 0.04	21.73 $\pm$ 0.09	20.45 $\pm$ 0.18	0.1
	2003 UZ 117	D	-	-	-	-	20.24 $\pm$ 0.07	20.86 $\pm$ 0.10	-
	2004 PT 107	A,D	-	-	21.66 $\pm$ 0.01	-	20.41 $\pm$ 0.14	19.87 $\pm$ 0.18	0.05
120347	2004 SB 60	C	-	-	20.21 $\pm$ 0.01	-	-	-	0.2
	2005 CB 79	E,F	21.45 $\pm$ 0.02	20.71 $\pm$ 0.03	20.36 $\pm$ 0.02	19.98 $\pm$ 0.03	19.67 $\pm$ 0.07	20.18 $\pm$ 0.16	-
	2005 GE 187	A	23.76 $\pm$ 0.10	22.78 $\pm$ 0.09	22.02 $\pm$ 0.01	21.47 $\pm$ 0.11	-	-	0.1
	"	C,D	-	-	22.13 $\pm$ 0.03	-	20.84 $\pm$ 0.08	20.18 $\pm$ 0.12	0.5
202421	2005 UQ 513	C,D	-	-	20.30 $\pm$ 0.01	-	18.89 $\pm$ 0.07	18.59 $\pm$ 0.10	0.3
136199	Eris	D	-	-	-	-	17.73 $\pm$ 0.07	17.49 $\pm$ 0.09

Notes. ^(a) Runs A-F as listed in Table 1. ^(b) $\Delta m_R$ is the variation in R-band magnitude seen for objects where (partial) light-curves were obtained. The uncertainty on each is $\sim$ 0.1 mag.

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