\begin{table}%t1
\caption{$\it SPEAR$ measured FUV emission line intensities (in LU) averaged over 
8$^{\circ} \times  8^{\circ}$ bins at sky positions~A--P.\label{tab1}}
%\centerline
 {\begin{tabular}{lccccccccc}
\hline
\hline
$\rm  Sky Pixel$&$l$&$b$&$I\rm  (OVI)$ &$I\rm (CIV)$&$I\rm (SiIV)$&$I\rm (SiII*)$&$I\rm (AlII)$&
$I\rm (OVI)/(CIV)$&$I{\rm (CIV)}/I\rm (SiIV)$\\
&&&(scaled doublet)&(doublet)&(scaled doublet)&&&&\\
&&&(LU)&(LU)&(LU)&(LU)&(LU)&&\\
\hline
A&301.5$^{\circ}$&+62.8$^{\circ}$&21~160~$\pm$~7500&7840~$\pm$~660&3530~$\pm$~610&
2995~$\pm$~655&6035~$\pm$~1780&2.7~$\pm$~0.98&2.2~$\pm$~0.55\\
B&312.8$^{\circ}$&+71.5$^{\circ}$&$<$6300&
7770~$\pm$~580&4290~$\pm$~2185&1830~$\pm$~690&4230~$\pm$~1080&$<$0.8&
1.8~$\pm$~1.0\\
C&341.6$^{\circ}$&+78.8$^{\circ}$&16~420~$\pm$~8000&7850~$\pm 310$&
2610~$\pm$~300&$2580\pm 335$&6335~$\pm$~2090&
$2.1\pm1.1$&$3.0\pm0.48$\\
D&303.8$^{\circ}$&+78.5$^{\circ}$&$<$6200&6890~$\pm$~405&2215~$\pm$~420&2355~$\pm$~455&
3400~$\pm$~1130&$<$0.9&$3.1\pm0.71$\\
E&292.0$^{\circ}$&+69.1$^{\circ}$&10~320~$\pm$~5500&$6350\pm450$&2490~$\pm$~765&
1925~$\pm$~445&3090~$\pm$~1515&1.6~$\pm$~0.96&2.6~$\pm$~0.98\\
F&287.5$^{\circ}$&+59.7$^{\circ}$&$<$6300&
8105~$\pm$~530&3330~$\pm$~485&$2200\pm430$&6285~$\pm$~1200&$<$0.8&$2.4\pm0.50$\\
G&276.3$^{\circ}$&+55.4$^{\circ}$&15~830~$\pm$~6500&6515~$\pm$~455&2365~$\pm$~630&
1475~$\pm$~410&4930~$\pm$~1290&
2.4~$\pm$~1.1&2.8~$\pm$~0.92\\
H&276.3$^{\circ}$&+64.9$^{\circ}$&9350~$\pm$~4200&4695~$\pm$~385&2140~$\pm$~385&
1860~$\pm$~405&4370~$\pm$~920&2.0~$\pm$~1.0&2.2~$\pm$~0.57\\
I&276.3$^{\circ}$&+74.7$^{\circ}$&$<$4000&3670~$\pm$~365&1565~$\pm$~370&1320~$\pm$~320&
3860~$\pm$~1525&$<$1.1&2.3~$\pm$~0.76\\
J&276.2$^{\circ}$&+84.8$^{\circ}$&6765~$\pm$~3900&5775~$\pm$~225&1830~$\pm$~220&
1910~$\pm$~315&4260~$\pm$~1470&1.2~$\pm$~0.7&3.2~$\pm$~0.50\\
K&248.7$^{\circ}$&+78.5$^{\circ}$&10~000~$\pm$~5000&4390~$\pm$~345&2140~$\pm$~700&
1435~$\pm$~295&4700~$\pm$~1310&$2.3\pm1.3$&$2.1\pm0.84$\\
L&260.6$^{\circ}$&+69.1$^{\circ}$&$<$5050&3175~$\pm$~520&1975~$\pm$~510&
2615~$\pm$~470&3595~$\pm$~920&$<$1.6&$1.6\pm0.67$\\
M&265.1$^{\circ}$&+59.7$^{\circ}$&$<$6000&$4715\pm645$&$2855\pm840$&$1540\pm470$&
$6020\pm1525$&$<$1.3&$1.7\pm0.73$\\
N&251.1$^{\circ}$&+62.8$^{\circ}$&$<$6200&$2035\pm730$&$<$1200&$<$600&$<$2500&$<$3.0&$>$1.7 \\
O&239.8$^{\circ}$&+71.5$^{\circ}$&$<$6580&$4455\pm570$&$<$1400&$2300\pm550$&
3275~$\pm$~840&$<$1.5&$>$3.1\\
P&211.1$^{\circ}$&+78.7$^{\circ}$&$<$7500&$4150\pm600$&$<$1300&1050~$\pm$~505&
3315~$\pm$~825&$<$1.8&$>$3.2\\
N.E.P.**&96.0$^{\circ}$&+29$^{\circ}$&5725~$\pm$~570&5820~$\pm$~280&1430~$\pm$~120&
2430~$\pm$~200&N/A&0.98~$\pm$~0.15&4.1~$\pm$~0.53\\
\hline
\end{tabular}}
\par
\smallskip
  ** Oservations of the North Ecliptic Pole (NEP) region by Korpela et~al. (2006).
\end{table}