Table 7:

The Hipparcos asteroid photometric dataset.

Object Number		N<0.01	N<0.02	N<0.03	N<0.04	N<0.05
1	65	40	63	65	65	65	0.010
2	63	20	43	56	60	62	0.017
3	60	12	38	58	60	60	0.018
4	58	48	58	58	58	58	0.008
5	81	1	18	42	60	70	0.032
6	91	16	63	85	90	91	0.018
7	69	23	52	66	68	69	0.015
8	56	4	24	41	52	55	0.024
9	40	4	22	38	40	40	0.020
10	51	3	11	30	46	48	0.029
11	68	8	25	46	56	64	0.027
12	24	1	10	16	19	21	0.028
13	34	0	3	14	24	29	0.035
14	45	4	17	30	38	42	0.027
15	83	6	32	62	75	82	0.024
16	49	1	10	21	31	41	0.035
18	100	4	27	54	80	93	0.030
19	30	0	2	11	18	24	0.039
20	61	5	19	38	48	57	0.028
22	63	1	10	24	43	50	0.039
23	66	2	8	20	35	46	0.042
27	35	3	14	24	30	32	0.027
28	33	0	2	11	16	25	0.041
29	74	9	41	63	71	73	0.021
30	48	0	3	13	28	35	0.044
31	14	0	0	8	13	14	0.033
37	32	1	2	17	24	27	0.036
39	112	7	50	82	102	109	0.024
40	103	2	14	37	53	73	0.041
42	51	4	22	40	49	49	0.024
44	53	4	13	29	41	49	0.030
51	14	1	1	7	10	14	0.035
63	12	0	3	8	10	11	0.031
88	36	0	0	10	16	31	0.040
115	33	0	5	9	16	19	0.047
129	40	0	6	18	28	37	0.035
192	32	0	4	12	21	28	0.037
196	14	0	1	4	10	13	0.038
216	21	1	3	6	14	19	0.037
230	35	2	8	20	30	32	0.031
324	73	5	22	40	58	67	0.030
349	92	1	24	64	80	88	0.028
354	98	0	24	48	73	86	0.032
451	29	0	3	13	20	25	0.036
471	112	2	21	48	80	94	0.034
511	64	1	15	26	42	47	0.038
532	40	4	19	29	37	39	0.024
704	82	4	12	33	55	77	0.034

Note:

For each object, identified by its number, the total number of observations is shown, as well as the number of observations with nominal accuracy less than 0.01, 0.02, 0.03, 0.04, 0.05 mag, respectively. The last column gives the average error of the observations. Bold characters in the Table are used to indicate objects with data for which the nominal requirements for successful inversion as derived from Fig. 4 are met.