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Table 2:

Summary of available results from image analysis of Long Period Comets.

Comet
$r_{\rm h}^a$ log$_{10}\rho$ (km)b mRc A f$\rho $ (cm) d Reference
C/1999 T2 (LINEAR) 3.35 ? 15.9   Szabó et al. (2001)
C/2000 H1 (LINEAR) 3.89 3.9 19.7 38$^\ddagger$ Szabó et al. (2001)
C/2000 SV74 (LINEAR) 4.04 2 15.3 1892 Szabó et al. (2002)
C/1995 O1 (Hale-Bopp) 4-13     3 $\times $ 103 - 8 $\times $ 104e  
C/1999 N4 (LINEAR) 5.5 ? 18.8$^\dagger$   Szabó et al. (2001)
C/1999 F2 (Dalcanton) 5.51 4.07 19.1 172$^\ddagger$ Szabó et al. (2001)
C/2000 K1 (LINEAR) 6.43 ? 18.4$^\dagger$   Szabó et al. (2001)
C/2003 O1 (LONEOS) 7.02-8.18 $^\S$ 11.37-12.9$^\char93 $ 1.3 $\times $ 103 - 318 Meech et al. (2009)
C/1999 J2 (Skiff) 7.14 ? 17.7$^\dagger$   Szabó et al. (2001)
  7.11-10.1 $^\S$ 9.9-13.4$^\char93 $ 4.7 $\times $ 103 - 234 Meech et al. (2009)
C/2001 Q4 (NEAT) 8.6 4   1500 Tozzi et al. (2003)
  5.84 $^\S$ 13.11$^\char93 $ 304 Meech et al. (2009)
C/2001 G1 (LONEOS) 8.32-11.22 $^\S$ 11.1-14.2$^\char93 $ 1.8 $\times $ 103 - 28 Meech et al. (2009)
C/2003 A2 (Gleason) 11.49-14.04 $^\S$ 11.6-12.8$^\char93 $ 1.2 $\times $ 103 - 407 Meech et al. (2009)
C/1995 O1 (Hale-Bopp) 13 5.3   3 $\times $ 104 Weiler et al. (2003)
C/1983 O1 (Cernis) 19.4 ? 23   Meech (1992)
C/1995 O1 (Hale-Bopp) 25.8 ? 20   Szabó et al. (2008)
a Heliocentric distance (AU) of observation. b Linear radius of the reference aperture at the comet. The symbol $\S$ corresponds to values by Meech et al. (2009) computed all using a 3.0 $^{\prime\prime}$ radius photometric aperture. c Integrated R magnitude in the reference aperture. $^\dagger$ Indicates a value obtained as the mean of the given light curve. # Indicates the average reduced R magnitude for $r
= \Delta = 1$ and $\alpha = 0^{\circ}$. d $^\ddagger$ Indicates that the value is not given by the respective authors in the reference, but it has been computed for this paper with their data by means of Eq. (2) (see text). e Derived from a theoretical model.

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