Table 2:

Dataset for the ``clear cases'', i.e., the sample used for the analysis of the family's general properties¹.

Comet	[AU]	I/O	Appearance	q [AU]	a [AU]
2P/Encke	3.1	O	S	0.34	2.22
4P/Faye	3.5	O	A	1.67	3.85
6P/d-Arrest	5.4	O	S	1.35	3.5
7P/Pons-Winnecke	4.7	I	S	1.25	3.43
8P/Tuttle	6.3	I	S	1.03	5.7
9P/Tempel 1	3.5	O	A	1.51	3.12
10P/Tempel 2	4.2	I	S	1.43	3.07
14P/Wolf	4.0	I	S	2.72	4.25
17P/Holmes	4.7	I	S	2.05	3.62
19P/Borrelly	3.8	I	S	1.35	3.61
22P/Kopff	4.2	O	A	1.58	3.46
26P/Grigg-Skjellerup	3.8	O	S	1.12	3.04
28P/Neujmin 1	5.4	I	S	1.55	6.91
30P/Reinmuth 1	5.7	I	N	1.88	3.77
32P/Comas Solá	3.1	I	A	1.83	4.26
36P/Whipple	4.1	O	A	3.09	4.17
37P/Forbes	3.6	I	S	1.57	3.42
40P/Vaisala 1	4.6	O	A	1.8	4.89
43P/Wolf-Harrington	4.4	I	A	1.58	3.47
45P/Honda-Mrkos-Pajdusakova	5.1	I	S	0.53	3.02
46P/Wirtanen	3.1	O	A	1.06	3.09
49P/Arend-Rigaux	3.3	O	S	1.37	3.53
50P/Arend	3.0	O	A	1.92	4.09
51P/Harrington A	5.3	I	N	1.57	3.58
53P/Van Biesbroek	4.5	O	A	2.41	5.39
54P/de Vico-Swift-NEAT	5.4	I	N	2.15	3.77
55P/Tempel-Tuttle	3.5	I	S	0.98	10.33
56P/Slaughter-Burnham	3.8	O	A	2.53	5.11
57P/du Toit-Neujmin-Delporte A	5.1	O	N	1.73	3.45
61P/Shajn-Schaldach	4.4	I	S	2.11	3.68
63P/Wild 1	3.8	I	N	1.96	5.6
64P/Swift-Gehrels	3.6	O	S	1.34	4.38
65P/Gunn	4.4	O	A	2.44	3.59
67P/Churyumov-Gerasimenko	3.2	O	A	1.25	3.47
69P/Taylor	4.0	O	A	1.94	3.64
70P/Kojima	4.8	I	S	2.01	3.68
72P/Denning-Fujikawa	3.3	O	N	0.78	4.33
73P/Schwassmann-Wachmann 3	3.0	I	A	0.93	3.06
74P/Smirnova-Chernyk	4.6	O	A	3.56	4.17
75P/Kohoutek	3.5	I	S	1.78	3.54
77P/Longmore	4.8	I	S	2.31	3.6
78P/Gehrels 2	3.8	O	A	2.01	3.74
82P/Gehrels 3	4.0	O	A	3.63	4.14
83P/Russell 1	3.0	O	N	1.61	3.34
86P/Wild 3	3.4	O	S	2.3	3.63
89P/Russell 2	3.0	O	A	2.29	3.8
92P/Sanguin	4.5	I	S	1.81	5.37
94P/Russell 4	4.1	O	S	2.24	3.52
96P/Machholz 1	4.9	I	S	0.12	3.02
97P/Metcalf-Brewington	3.7	O	S	2.61	4.8
98P/Takamizawa	3.3	I	S	1.66	3.8
103P/Hartley 2	5.0	O	A	1.04	3.45
109P/Swift-Tuttle	5.3	O	A	0.96	26.1
110P/Hartley 3	3.6	I	S	2.49	3.62
111P/Helin-Roman-Crockett	3.5	I	S	3.48	4.05
113P/Spitaler	4.2	I	N	2.13	3.69
114P/Wiseman-Skiff	3.8	I	S	1.58	3.55
115P/Maury	6.4	O	S	2.04	4.26
116P/Wild 4	4.7	I	A	2.17	3.45
117P/Helin-Roman-Alu 1	3.3	I	A	3.04	4.09
118P/Shoemaker-Levy 4	4.1	O	A	2.01	3.48
119P/Parker-Hartley	3.4	I	A	3.04	4.29
120P/Mueller 1	3.1	I	S	2.75	4.14
121P/Shoemaker-Holt 2	3.1	O	A	2.65	4.01
124P/Mrkos	4.2	I	S	1.47	3.21
128P/Shoemaker-Holt 1-A	3.7	O	A	3.05	4.45
129P/Shoemaker-Levy 3	4.6	I	A	2.81	3.74
131P/Mueller 2	3.5	O	S	2.42	3.69
135P/Shoemaker-Levy 8	3.6	I	N	2.72	3.83
136P/Mueller 3	4.8	I	N	2.96	4.19
137P/Shoemaker-Levy 2	4.2	O	S	1.87	4.44
139P/Vaisala-Oterma	3.4	O	A	3.4	4.51
143P/Kowal-Mrkos	3.9	O	S	2.54	4.3
147P/Kushida-Muramatsu	4.1	I	N	2.75	3.8
152P/Helin-Lawrence	5.8	O	A	3.11	4.48
159P/LONEOS	4.0	O	A	3.65	5.89
160P/LINEAR	4.0	O	S	2.08	3.98
202P/Scotti	5.0	I	N	2.52	3.78
P/1996 A1 (Jedicke)	5.5	I	S	4.05	7.18
P/1998 U4 (Spahr)	6.1	O	A	3.84	5.57
P/2001 H5 (NEAT)	4.6	O	S	2.4	5.99
P/2002 T5 (LINEAR)	5.2	O	A	3.93	6.99
P/2003 S1 (NEAT)	3.5	O	A	2.6	4.56
P/2003 S2 (NEAT)	3.6	O	S	2.46	3.83
P/2004 DO29 (Spacewatch-LINEAR)	4.2	O	A	4.09	7.47
P/2004 H2 (Larsen)	3.7	O	A	2.62	4.5
P/2004 H3 (Larsen)	3.7	O	S	2.44	3.89
P/2004 T1 (LINEAR-NEAT)	3.8	O	N	1.71	3.47
P/2004 V5-A (LINEAR-Hill)	4.4	I	A	4.41	7.95
P/2004 V5-B (LINEAR-Hill)	4.4	I	A	4.41	7.95

¹ is the heliocentric distance adopted for the analysis (see Sect. 2.4 for the adopted criteria). ``I'' and ``O'' refer to whether the comet was inbound (pre-perihelion) or outbound (post-perihelion). Appearance (S - stellar, A - active, N - not detected) is the same indicated in Table 1. q and a are the present perihelion distance and semi-major axis, respectively (derived from the JPL Horizon Data Base).