\begin{table}%T6 NON %ta.1
\par
\caption{\label{tabA}Observing Log for the NEP spectra. Scan numbers are from Gioia et~al. (\cite{Gioia2003}).}
\small%\centerline
{
\begin{tabular}{rcccccc} 
\hline
  \hline  
Scan    &  Date   &    RA	&     Dec  &      Spectral type&     $t_i$ (s)  & {\it S/N} \\ 
&&(h m s)&$^\circ~'$ ${}^{\prime\prime}$&&\\
\hline
  $^*$20 &  2004 Jun. 28 & 17 52 44.8 &+67 00 20&       G8  &  5400&70\\
 260 &  2004 Jun. 01 & 17 58 28.3 &+67 26 08&	  G2&	2400&50\\	
 330 &  2004 Jun. 02 & 17 59 23.6 &+66 02 55&	  G9&  1800&70\\
 370 &  2004 May 25 & 18 00 02.2 &+66 45 53&	  F8&  2400&90\\
$^*$1420 &  2004 Mar. 08 & 17 19 28.8 &+65 22 29&	  K0&  3600&60\\
$^*$1441 &  2004 Jan. 31 & 17 20 05.6 &+62 06 22&	  G2&  1200&100\\
1470 &  2004 Mar. 09 & 17 20 26.7 &+67 03 37&	  G8&  1800&80\\
1500 &  2004 Apr. 07 & 17 21 10.9 &+69 48 02&	  G2&  600&200\\
1511 &  2004 Feb. 03 & 17 21 42.5 &+62 00 32&	  K4&  3600&60\\
1580 &  2004 Apr. 07 & 17 24 00.4 &+69 40 30&	  K2&  3600&50\\
$^*$1600 &  2004 Mar. 08 & 17 24 26.8 &+64 12 23&	  G2&  1800&50\\
1601 &  2004 Mar. 09 & 17 24 38.8 &+64 40 51&	  G0&  1800&80\\
1690 &  2004 Mar. 09 & 17 26 45.4 &+69 37 53&	  G2&  2400&60\\
1800 &  2004 May 06 & 17 29 39.4 &+68 47 38&	  F5&  1200&110\\
1840 &  2004 May 25 & 17 30 19.9 &+69 55 27&	  G0&  1800&90\\
1960 &  2004 Apr. 07 & 17 33 16.9 &+67 12 08&	  F2&  600&170\\
2050 &  2004 Mar. 09 & 17 36 14.1 &+65 02 27&	  K0&  2400&70\\
2100 &  2004 May 06 & 17 36 26.6 &+68 20 37&	  M3&  600&170\\
2210 &  2004 Jun. 02 & 17 39 16.1 &+70 20 09&	  F8&  1200&80\\
2250 &  2004 Mar. 08 & 17 39 56.1 &+65 00 04&	  K0&  2400&200\\
2360 &  2004 Jun. 01 & 17 42 26.5 &+69 07 58&	  F8&  1200&120\\
2400 &  2004 Mar. 09 & 17 43 01.6 &+66 06 46&	  G2&  1800&90\\
2470 &  2004 Jun. 02 & 17 43 51.7 &+70 31 39&	  F3&  1800&40\\
2480 &  2004 Jun. 01 & 17 44 00.6 &+70 15 27&	  K0&	2400&50\\
$^*$2970 &  2004 Jan. 31 & 17 49 03.9 &+62 47 48&	  F2&  600&290\\
$^*$3080 &  2004 Jun. 28 & 17 50 25.3 &+70 45 36&	  K2.5&  1800&90\\
3220 &  2004 Jun. 01 & 17 52 56.0 &+66 25 10&	  K0&	600&150\\
3560 &  2004 Jun. 28 & 17 57 03.7 &+68 49 14&	  G8&  1800&110\\
3610 &  2004 May 06 & 17 58 01.4 &+64 09 34&	  K4&  2700&70\\
3690 &  2004 May 06 & 17 58 48.0 &+63 50 39&        A2&  1200&120\\
3710 &  2004 Jun. 30 & 17 59 13.8 &+64 08 33&	  F2&	1200&200\\
$^*$4090 &  2004 Jun. 28 & 18 05 30.5 &+69 45 17&	  G2&  2400&50\\
4100 &  2004 May 25 & 18 05 30.3 &+62 19 03&	  K0&  1200&150\\
4130 &  2004 Jun. 02 & 18 05 44.8 &+65 51 58&	  F5&  1200&80\\
4180 &  2004 May 25 & 18 06 41.0 &+64 13 18&	  K0&  600&440\\
4380 &  2004 Jun. 01 & 18 08 45.4 &+62 56 37&        G5&	1200&120\\
4470 &  2004 Jun. 29 & 18 09 55.8 &+69 40 39&	  K3&  1200&160\\
4530 &  2004 Jun. 29 & 18 10 49.9 &+70 16 09&	  G9&  4800&80\\
4780 &  2004 Jun. 29 & 18 13 48.6 &+68 31 32&	  K2&  2400&80\\
4810 &  2004 Jun. 03 & 18 13 51.4 &+64 23 57&	  F5&  180&300\\
$^*$4931 &  2004 Jun. 28 & 18 16 21.2 &+65 29 39&	  K8&  1200&170\\
4970 &  2004 Jun. 03 & 18 16 49.7 &+65 04 26&	  K2&  2400&60\\
5060 &  2004 Jun. 29 & 18 18 31.9 &+70 42 17&	  G5&  1800&90\\
5220 &  2004 Jun. 03 & 18 20 19.2 &+65 19 19&	  F8&  600&120\\
$^*$5320 &  2004 Jun. 28 & 18 21 46.8 &+63 57 10&	  K0&  1800&90\\
5510 &  2004 Jun. 03 & 18 25 09.0 &+64 50 21&	  K0&  600&260\\
5520 &  2004 Jun. 03 & 18 25 32.9 &+62 34 15&	  K4&  2400&60\\
5950 &  2004 Jun. 30 & 18 32 29.5 &+68 36 52&	  G0&  600&190\\
6030 &  2004 Jun. 29 & 18 33 47.8 &+65 13 33&	  K3&  1200&150\\
6051 &  2004 Jun. 29 & 18 34 33.6 &+69 31 45&	  K5&  3600&50\\
6160 &  2004 Jun. 30 & 18 36 13.5 &+65 29 15&	  F0&  300&230\\
6163 &  2004 Jun. 29 & 18 36 22.8 &+66 54 54&	  G3&  600&180\\
6350 &  2004 Jun. 29 & 18 39 25.4 &+69 02 54&	  M3&  2400&60\\
6400 &  2004 Jun. 29 & 18 40 44.4 &+70 38 47&	  K2&  1200&70\\
6410 &  2004 Jun. 30 & 18 40 56.6 &+62 44 54&	  K0&  300&300\\
6510 &  2004 Jun. 29 & 18 43 12.6 &+69 55 54&	  F0&  1200&80\\\hline
\end{tabular}}
\smallskip
* We lack the thorium-argon lamp exposures for the nights in which these~stars were acquired. They
were wavelength calibrated using lamp exposures of the nearest night.
\end{table}