Table 2:

Herschel observing geometries for our seven targets, including properties derived from ground-based visible observations and the obtained radiometric solutions.

Target	r [AU]	[AU]		HV [mag]		P [h]	Ref.
2003 AZ84	45.376	44.889	1.11	3.83 0.04	0.14 0.03	6.79 h	1, 2, 3	850-970	0.05-0.09	2-10	1.31
2001 YH140	36.576	36.169	1.44	5.8 0.2	0.13 0.05	13.2 h	4	300-390	0.06-0.10	0-10	1.2
1997 CS29	43.509	43.241	1.27	5.65 0.09	<0.08, <0.22	--	5, 6, 7, 8	250-420	0.06-0.14	0-25	1.2
2000 YW134	44.125	43.833	1.25	4.88 0.05	<0.10	--	9, 10	<500	>0.08	0-25	--
Typhon	17.943	18.376	2.84	7.68 0.04	0.07 0.01	9.67 h	4, 11, 12	134-154	0.065-0.085	1-10	0.96
2006 SX368	11.972	12.271	4.48	9.5	--	--	MPC	70-80	0.05-0.06	0-40	1.2
2005 TB190	46.377	46.683	1.17	4.58 0.22	0.12 0.02	12.68 h	13	335-410	0.15-0.24	0-25	1.2

Notes. r: Sun-target distance, : Herschel-target distance, : phase angle; H_V magnitudes, lightcurve  , and the rotation period P; references for the preceeding three columns, derived effective diameter  in [km] and geometric albedo  values from the TPM analysis, the corresponding possible thermal inertias  [J m^-2 s^-0.5 K^-1], and the fitted NEATM  value (: for a fixed value).

References. (1) Fornasier et al. (2004); (2) DeMeo et al. (2009); (3) Perna et al. (2010); (4) Thirouin et al. (2010); (5) Sheppard & Jewitt (2002); (6) Romanishin & Tegler (1999); (7) Davies et al. (2000); (8) Boehnhardt et al. (2001); (9) Sheppard & Jewitt (2003); (10) Doressoundiram et al. (2005); (11) Rabinowitz et al. (2007); (12) Tegler et al. (2003); (13) Thirouin et al., in prep.; MPC: http://www.cfa.harvard.edu/iau/lists/Centaurs.html