\begin{table}%t2
\caption{\label{cleanlist}Dataset for the ``clear cases'', i.e., the sample used for the analysis of the family's general properties$^1$.}
%\centering
\small 
\begin{tabular}{lccccc}
\hline\hline
\noalign{\smallskip}
Comet & $r_{\rm h}$ [AU] & I/O & Appearance & $q$ [AU] & $a$ [AU] \\
\hline
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 Sol\'a	&	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	\\
\hline
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	\\
\hline
\end{tabular}
\medskip
$^1$ $r_{\rm h}$ 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~\ref{list}. $q$ and~$a$ are the present perihelion distance and semi-major axis, respectively (derived from the JPL Horizon Data Base).
\end{table}