**Table 2:** Physical data, taxonomic classification of the asteroids, and estimated ages for the breakup of their corresponding families.
Asteroid	H	D	$a_{\rm P}$	$e_{\rm P}$	$i_{\rm P}$	Taxon.	Family	Age of
	(mag)	(km)	(AU)			class		family^a
(1270) Datura	12.5	10.8	2.23	0.15	5.33	Sk	Datura	$450\pm50$ Ky
(60 151) 1999 UZ6	16.3	1.9	2.23	0.15	5.32	Sk	Datura	$450\pm50$ Ky
(90 265) 2003 CL5	15.4	2.9	2.23	0.15	5.32	Sq	Datura	$450\pm50$ Ky
2001 WY35	17.0	1.4	2.23	0.15	5.33	O/Q	Datura	$450\pm50$ Ky
(16 598)1992 YC2	14.7	3.9	2.59	0.18	17.22	Sq	(16598)	50-250 Ky
2004 XL40	17.0	1.4	2.28	0.13	5.31	Sq	Lucascavin	300-800 Ky

^a Determined by Nesvorný et al. (2006a), and the effective diameters (D)
were estimated assuming an albedo p_v=0.15.

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