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Table 2:

Observed comets.
Comet $T_{\rm P}$ e a q Aph i P $T_{\rm J}$ Type
  (yyyy-mm-dd)   (AU) (AU) (AU) ($^\circ$) (yr)   L H
122P/de Vicoa 1995-10-06 0.96271 17.7 0.66 34.7 85 74.3 0.37 HF SP$_{\rm I}$
C/1996 B2 (Hyakutake) 1996-05-01 0.99990 2296 0.23 4591 125 110000 -0.34 EXT L
C/1995 O1 (Hale-Bopp)b,c 1997-04-01 0.99509 186.0 0.91 371.1 89 2537 0.04 EXT I
55P/Tempel-Tuttle 1998-02-28 0.90555 10.3 0.98 19.7 162 33.2 -0.64 HF SP$_{\rm I}$
C/1999 H1 (Lee) 1999-07-11 0.99974 2773 0.71 5545 149 146000 -0.90 EXT L
C/1999 S4 (LINEAR)d 2000-07-26 1.00010 - 0.77 - 149 - - NEW L
C/1999 T1 (McNaught-Hartley) 2000-12-13 0.99986 8502 1.17 17000 80 780000 0.23 EXT L
C/2001 A2 (LINEAR) 2001-05-25 0.99969 2530 0.78 5060 36 127000 0.88 EXT L
C/2000 WM1 (LINEAR)b 2002-01-23 1.00025 - 0.56 - 73 - - NEW L
153P/Ikeya-Zhanga 2002-03-19 0.99010 51.2 0.51 101.9 28 366.5 0.88 EXT IP
C/2002 X5 (Kudo-Fujikawa) 2003-01-29 0.99984 1175 0.19 2350 94 40300 -0.03 EXT L
C/2002 V1 (NEAT) 2003-02-18 0.99990 1010 0.10 2021 82 32100 0.06 EXT L
C/2002 Y1 (Juels-Holvorcem) 2003-04-13 0.99715 250.6 0.71 500.5 104 3967 -0.23 EXT I
88P/Howelld 2004-04-13 0.56124 3.1 1.37 4.9 4 5.5 2.95 JF SP$_{\rm IV}$
C/2002 T7 (LINEAR) 2004-04-23 1.00048 - 0.61 - 161 - - NEW L
C/2001 Q4 (NEAT)c 2004-05-16 1.00069 - 0.96 - 100 - - NEW L
C/2003 K4 (LINEAR)c 2004-10-14 1.00030 - 1.02 - 134 - - NEW L
9P/Tempel 1e 2005-07-05 0.51749 3.1 1.51 4.7 11 5.5 2.97 JF SP$_{\rm IV}$
73P-B/Schwassmann-Wachmann 3f 2006-06-08 0.69350 3.1 0.94 5.2 11 5.4 2.78 JF SP $_{\rm III}$
73P-C/Schwassmann-Wachmann 3f 2006-06-07 0.69338 3.1 0.94 5.2 11 5.4 2.78 JF SP $_{\rm III}$
C/2006 M4 (SWAN) 2006-09-29 1.00018 - 0.78 - 112 - - NEW L
17P/Holmesg 2007-05-04 0.43242 3.6 2.05 5.18 19 6.9 2.86 JF SP$_{\rm IV}$
8P/Tuttleh 2008-01-27 0.8198 5.7 1.03 10.4 55 13.6 1.60 HF SP$_{\rm I}$
C/2007 N3 (Lulin) 2009-01-10 1.00004 - 1.21 - 178 - - NEW L
a Jehin et al. (2004) - b Arpigny et al. (2000, 2003) - c Manfroid et al. (2005) - d Hutsemékers et al. (2005) - e Jehin et al. (2006) - f Jehin et al. (2008) - g Bockelée-Morvan et al. (2008a) - h Bockelée-Morvan et al. (2008b).
The elements are obtained from the JPL Solar System Dynamics website. $T_{\rm P}$ is the epoch of the perihelion, e the eccentricity, q the perihelion distance in AU, Aph the aphelion distance, i the inclination on the ecliptic, P the period, $T_{\rm J}$ the Tisserand parameter relative to Jupiter, the last columns give the classification according to Levison (1996) and Horner et al. (2003). The subdivision I-IV based on $T_{\rm J}$ is given for the SP comets only, all others being of the sub-type I.

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