\begin{table}
\caption{VLT late-time NIR observations of SN~2003hv.}
\label{tab:VLTIRLOG} %\centering
\par
\begin{tabular}{ccccccc}
\hline\hline
Date & MJD & Phase & Filter & Exposure$^a$ & Airmass & Seeing  \\
(UT) &(days)     &  (days) &        & (s)      &         & (arcsec) \\
\hline
2004 08 18  & 53235.37    &  344.2  & $J_{s}$     &   30 $\times$ 4 $ \times$ 24 & 1.04 & 0.55\\
2004 08 29  & 53246.25    &  355.1  & $K_{s}$     &   10 $\times$ 6 $\times$ 30 & 1.37 & 0.47 \\
2004 08 29  & 53246.29    &  355.1  & $H$     &   10 $\times$ 6 $\times$59 & 1.17 & 0.75\\
2004 08 29  & 53246.32    &  355.1  & $K_{s}$     &   10 $\times$ 6 $ \times$ 30 & 1.07 & 0.57 \\
2004 08 29  & 53246.39    &  355.2  & $H$     &   10 $\times$ 6 $\times$ 30 & 1.00 & 0.75 \\
2004 08 30  & 53247.26    &  356.1  & $J_{s}$     &   30 $\times$ 4 $\times$ 23 & 1.29 & 0.77 \\
2004 08 30  & 53247.30    &  356.1  & $K_{s}$     &   10 $\times$ 6 $\times$ 30 & 1.13 &  0.50  \\
2005 01 24  & 53394.02    &  502.8  & $K_{s}$     &   10 $\times$ 6 $\times$ 60 & 1.03 &  0.47\\
2005 01 24  & 53394.09    &  502.9  & $H$     &   10 $\times$ 6 $\times$ 30 & 1.24 &  0.74 \\
2005 02 24  & 53425.99    &  534.8  & $K_{s}$     &   10 $\times$ 6 $\times$ 30 & 1.18 & 0.62 \\
2005 02 25$^b$  & 53426.99    &  535.8  & $J_{s}$     &   30 $\times$ 4 $\times$ 46 & 1.19 & 0.83 \\
2005 02 27  & 53428.99    &  537.8  & $H$     &   10 $\times$ 6 $\times$ 30 & 1.22 & 0.55 \\
2005 02 28  & 53429.99    &  538.8  & $J_{s}$     &   30 $\times$ 4 $\times$ 23 & 1.22 & 0.56\\
2005 10 13  & 53656.18    &  765.0  & $J_{s}$     &   30 $\times$ 4 $\times$ 46 & 1.11 & 0.70 \\
2005 10 13  & 53656.35    &  765.2  & $J_{s}$     &   30 $\times$ 4 $\times$ 23 & 1.14 & 0.56 \\
2005 10 14  & 53657.21    &  766.0  & $J_{s}$     &   30 $\times$ 4 $\times$ 46 & 1.04 & 0.54\\
2005 10 14  & 53657.32    &  766.1  & $H$     &   10 $\times$ 6 $\times$ 60 & 1.05 & 0.72 \\
2005 10 15  & 53658.31    &  767.1  & $H$     &   10 $\times$ 6 $\times$ 30 & 1.04 & 0.40\\
  \hline%\\[-1mm]
\end{tabular}
\par
\begin{tabular}{lll}
$^a~$Detector integration time (DIT) $\times$ number of DITs per
exposure $\times$ number of exposures. && \\
$^b$ Image not included in the final photometry as it is a poor
image and
gives bad results. %\\
\end{tabular}
\end{table}