\begin{table}%t2
\caption{Selected nova systems.\label{systems}}
%\centerline
 {\begin{tabular}{lccccccr}
\hline
\hline
 System & $P_{\rm orb}$ & $M_{\rm 2}$ & $t_{\rm 3}$ & $M_{\rm 1}$ & $q$ & SH
 & Reference\\
  & [h] & [$M_{\rm \odot}$] & [d] & [$M_{\rm \odot}$] & & & \\
\hline
RW UMi & 1.418 & 0.07 & 140 & 0.64 & 0.11 & N & 1 \\
CP Pup & 1.474 & 0.08 & 8 & 1.19 & 0.07 & Y & 2 \\
V1974 Cyg & 1.950 & 0.14 & 42 & 0.90 & 0.16 & Y & 3, 4 \\
RS Car & 1.980 & 0.14 & (58) & 0.83 & 0.17 & N & 5 \\
DD Cir & 2.339 & 0.18 & (10) & 1.16 & 0.16 & N & 6 \\
IM Nor & 2.462 & 0.20 & 50 & 0.86 & 0.23 & N & 7, 8 \\
QU Vul & 2.682 & 0.23 & 40 & 0.91 & 0.25 & N & 9 \\
V2214 Oph & 2.804 & 0.24 & 100 & 0.71 & 0.34 & N & 10 \\
V630 Sgr & 2.830 & 0.25 & 11 & 1.14 & 0.22 & Y & 11 \\
V351 Pup & 2.837 & 0.25 & (32) & 0.95 & 0.26 & N & 11 \\
V5116 Sgr & 2.971 & 0.26 & 20.2 & 1.04 & 0.25 & N & this paper \\
V4633 Sgr & 3.014 & 0.27 & 42 & 0.90 & 0.30 & Y & 12 \\
DN Gem & 3.068 & 0.28 & 37 & 0.92 & 0.30 & N & 13 \\
V1494 Aql & 3.231 & 0.30 & 16 & 1.08 & 0.28 & N & 14, 15, 16 \\
V1668 Cyg & 3.322 & 0.31 & 23 & 1.02 & 0.30 & N & 17 \\
V603 Aql & 3.324 & 0.31(0.29) & 8 & 1.19(1.2) & 0.26(0.24) & Y & 18 \\
RR Cha & 3.370 & 0.31 & 58 & 0.83 & 0.37 & Y & 5, 19 \\
RR Pic & 3.481 & 0.33(0.4) & 150 & 0.62(0.95) & 0.53(0.42) & N & 20, 21 \\
V382 Vel & 3.508 & 0.33 & 9 & 1.17 & 0.28 & N & 22, 23 \\
V533 Her & 3.530 & 0.33 & 44 & 0.89 & 0.37 & N & 24, 25 \\
V2574 Oph & 3.550 & 0.34 & (33) & 0.95 & 0.36 & Y & 26 \\
OY Ara & 3.731 & 0.36(0.34) & ... & (0.82) & (0.41) & N & 27 \\
V1493 Aql & 3.740 & 0.36 & 7 & 1.21 & 0.30 & N & 14, 28 \\
V849 Oph & 4.146 & 0.41  & 175 & 0.59 & 0.69 & N & 29 \\
DQ Her & 4.647 & 0.48(0.40) & 94 & 0.72(0.60) & 0.67(0.67) & N & 30 \\
T Aur & 4.906 & 0.51(0.63) & 100 & 0.71(0.68) & 0.72(0.92) & N & 31 \\
V4745 Sgr & 4.987 & 0.52 & 32.8 & 0.95 & 0.55 & N & 32, 33 \\
HR Del & 5.140 & 0.54(0.55) & 230 & 0.54(0.67) & 1.00(0.82) & N & 34 \\
V1425 Aql & 6.139 & 0.57 & 39 & 0.91 & 0.63 & N & 14, 35 \\
V4743 Sgr & 6.718 & 0.74 & 15 & 1.10 & 0.67 & N & 36, 37 \\
BY Cir & 6.760 & 0.74 & 157 & 0.62 & 1.19 & N & 6 \\
V2540 Oph & 6.835 & 0.75 & 213 & 0.55 & 1.36 & N & 38 \\
V838 Her & 7.143 & 0.79(0.74) & 3.2 & 1.29(0.87) & 0.61(0.85) & N & 39 \\
V2275 Cyg & 7.548 & 0.84 & 7 & 1.21 & 0.69 & N & 40, 41 \\
BT Mon & 8.012 & 0.90(0.87) & (213) & 0.55(1.04) & 1.64(0.84) & N & 42 \\
V368 Aql & 8.285 & 0.93 & 42 & 0.90 & 1.03 & N & 43 \\
QZ Aur & 8.580 & 0.97(1.05) & 27 & 0.99(1.05) & 0.98(1.00) & N & 44 \\
\hline
\end{tabular}}
\par
\smallskip
Note: $P_{\rm orb}$ is the orbital period in hours, $M_{\rm 2}$ is the
secondary mass in solar masses derived from Smith \& Dhillon (\cite{Smith98}) (from
Ritter \& Kolb \cite{Ritter03}, in parentheses), $t_{\rm 3}$ is the decline time of three
magnitudes from maximum (value in parentheses is the value estimated from the
$t_{\rm 2}$ time using $t_{\rm 3} \simeq 2.75~t_{\rm 2}^{0.88}$ from Warner
\cite{Warner95}), $M_{\rm 1}$ is the primary mass derived from Livio (\cite{Livio92}) (from 
Ritter \& Kolb \cite{Ritter03}, in parentheses), $q$ is the mass ratio, SH is the information
about superhump detection (Y -- yes, N -- no), and Ref. is the reference.\\
%
References:
1 - Retter \& Lipkin (\cite{Retter01}), 2 - Patterson \& Warner (\cite{Patterson98}), 3 - Skillman 
et~al. (\cite{Skillman97}), 4 - Retter et~al. (\cite{Retter97}), 5 - Woudt \& Warner (\cite{Woudt02}), 6 - Woudt  \& Warner (\cite{Woudt03}c), 7 - Woudt \& Warner (\cite{Woudt03}b), 8 - Kato et~al. (\cite{Kato02}a), 9 -
Shafter \& Misselt (\cite{Shafter95}), 10 - Baptista et~al. (\cite{Baptista93}), 11 - 
Woudt \& Warner (\cite{Woudt01}), 12 - Lipkin et~al. (\cite{Lipkin01}), 13 - Retter et~al. (\cite{Retter99}), 14 - Arkhipova et~al. (\cite{Arkhipova02}), 15 - Kato et~al. (\cite{Kato04}), 16 - Barsukova \& Goranskii (\cite{Barsukova03}),
17 - Kaluzny (\cite{Kaluzny90}), 18 - Retter \& Naylor (\cite{Retter00}), 19 - Hoffmeister (\cite{Hoffmeister59}),
20 - Vogt (\cite{Vogt75}), 21 - Warner (\cite{Warner86}), 22 - Balman et~al. (\cite{Balman06}), 23 - Della Valle et~al. (\cite{DellaValle02}), 24 - Patterson (\cite{Patterson79a}), 25 - Thorstensen  \&  Cynthia
(2000), 26 - Kang et~al. (\cite{Kang06}a), 27 - Zhao \& McClintock (\cite{Zhao97}), 28 -
Dobrotka et~al. (\cite{Dobrotka06}b), 29 - Shafter et~al. (\cite{Shafter93}), 30 - Walker (\cite{Walker61}), 31 -
Walker (\cite{Walker63}), 32 - Cs\'ak et~al. (\cite{Csak05}), 33 - Dobrotka et~al. (\cite{Dobrotka06}a), 34 -
Kohoutek \& Pauls (\cite{Kohoutek80}), 35 - Retter \& Leibowitz (\cite{Retter98}), 36 - Kang 
et~al. (\cite{Kang06}b), 37 - Kato et~al. (\cite{Kato02}b), 38 - Ak et~al. (\cite{Ak05}), 39 - Leibowitz
et~al. (\cite{Leibowitz92}), 40 - Balman et~al. (\cite{Balman05}), 41 - Kiss et~al. (\cite{Kiss02}), 42 -
Robinson et~al. (\cite{Robinson82}), 43 - Diaz \& Bruch (\cite{Diaz94}), 44 - Campbell \& Shafter
(\cite{Campbell95}).\\
%
Aditional sources for orbital period, $t_{\rm 2}$/$t_{\rm 3}$ time and
catalogue masses: Duerbeck (\cite{Duerbeck87}), Warner (\cite{Warner86}, \cite{Warner95}, \cite{Warner02}), Diaz \& Bruch (\cite{Diaz97}), Ritter \& Kolb (\cite{Ritter03}).
\end{table}