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\def\phg{\phm{$>$}}
\def \arcsec       {$^{\prime\prime}$} 
\def \arcmin       {$^{\prime}$} 
\def\ef{$>$22.5} 
\def \etal         {{\it et~al.} } 
\def \flxx {erg cm$^{-2}$s$^{-1}$}
\begin{document}

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\begin{deluxetable}{lrrrrrrrrrrrrlrrlc}
\tablecolumns{18}
\tablewidth{0pt}
\tablenum{1}
\tablecaption{ Compact X-ray/Radio Sources in the NEP}
\tablehead{
\multicolumn{5}{c}{Radio Data} & \colhead{} & \multicolumn{6}{c}{X-ray Data} &\colhead{} &  \multicolumn{4}{c}{Optical Data} & \colhead{Notes} \\
\cline{1-5} \cline{7-12} \cline{14-17} & \\
\multicolumn{1}{c}{VLA Source} & \multicolumn{1}{c}{$\alpha_{2000}$} & \multicolumn{1}{c}{$\delta_{2000}$} & 
\multicolumn{1}{c}{S$_{1.5}$} & \multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{ROSAT source} &
\multicolumn{1}{c}{$\Delta$} & \multicolumn{1}{c}{Loc} & \multicolumn{1}{c}{MaxL} & \multicolumn{1}{c}{F$_x$} & 
\multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{$\Delta\alpha$} & 
\multicolumn{1}{c}{$\Delta\delta$} & \multicolumn{1}{c}{B} & 
}
\startdata
1732.9+6533 & 17 32 54.8 & 65 33 26.7 &1057.9 & 51.1 
    && RXS J173254.8+653318 & 8 & o &  73 &  37.4 &  4.9 && S & -6   & -2  &\phg 17.6    & \tablenotemark{1} \nl
1738.0+6654 & 17 38 \phn2.2 & 66 54 14.9 &   1.4 &  0.2 
    &&RXS J173803.3+665343 &32 & o &  28 &  17.5 &  3.4 && E & \nd  & \nd &    $>$22.5  &   \nl
1743.8+6544 & 17 43 48.9 & 65 44 23.9 &  20.3 &  0.9 
    &&RXS J174349.4+654418 & 6 & i &   8 &  13.5 &  5.1 && S &  0   & 0   &\phg 21.5 b  &   \nl
1747.2+6813 & 17 47 12.4 & 68 13 17.4 &   2.7 &  0.2 
   &&RXS J174711.5+681316 & 5 & o &   7 &   6.9 &  2.7 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{2} \nl
1747.2+6532 & 17 47 13.6 & 65 32 35.6 & 375.0 & 12.4
    &&RXS J174710.5+653225 &22& i &  10 &  30.8 &  8.5 && E & \nd  & \nd &    $>$22.5 & \tablenotemark{3} \nl
1748.5+7005 & 17 48 32.8 & 70 \phn5 51.0 & 711.6 & 21.7
    &&RXS J174833.1+700554 & 4 & o & 345 & 126.6 &  8.9 && S &  0   & -1  &\phg 17.5 b  & \tablenotemark{4} \nl 
1748.6+6842 & 17 48 38.2 & 68 42 17.4 &   2.5 &  0.3 
    &&RXS J174837.9+684220 & 3 & o &  98 &  38.2 &  4.8 && G &  0   & -3  &\phg 16.3    & \tablenotemark{5} \nl
1751.5+7013 & 17 51 31.8 & 70 13 21.6 &  29.2 &  1.3 
    &&RXS J175131.5+701332 &10& o &  17 &  17.8 &  4.5 && E & \nd  & \nd &    $>$22.5  &   \nl
1753.1+6746 & 17 53 \phn6.0 & 67 46 57.7 &  76.4 &  2.9 
    &&RXS J175308.8+674642 &21& i &  23 &  22.5 &  5.9 && G &  3   & -2  &\phg 19.5 b  &   \nl
1755.1+6519 & 17 55  \phn5.3 & 65 19 58.2 &   1.2 &  0.1 
    &&RXS J175505.7+651954 & 4& i & 585 & 193.8 & 14.3 && G &  2   & -3  &$\sim$15.5 b & \tablenotemark{6} \nl
1755.3+6747 & 17 55 16.6 & 67 47 50.9 &   3.7 &  0.4 
    &&RXS J175518.0+674804 &15& i &  25 &  21.0 &  5.2 && E & \nd  & \nd &    $>$22.5  &   \nl
1758.8+6349 & 17 58 46.0 & 63 49 21.5 &   9.8 &  0.4 
    &&RXS J175841.3+634900 &37& o &  10 &  11.6 &  3.5 && E & \nd  & \nd &    $>$22.5  &   \nl
1759.3+6902 & 17 59 15.2 & 69 \phn2 22.0 &   3.8 &  0.3 
    &&RXS J175919.1+690229 &22& o &   9 &   8.8 &  2.9 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{7} \nl
1800.1+6636 & 18  \phn0  \phn7.1 & 66 36 54.3 &  30.6 &  1.0 
    &&RXS J180007.5+663652 & 3& i & 115 &  13.4 &  1.5 && G &  1   &  1  &\phg 14.6    & \tablenotemark{8} \nl
1800.5+6705 & 18  \phn0 29.1 & 67  \phn5 49.9 &   5.8 &  0.3 
    &&RXS J180029.0+670548 & 1& i &  32 &  11.5 &  2.4 && S & -3   &  1  &\phg 20.8 c  & \tablenotemark{9} \nl
1802.2+6527 & 18  \phn2  \phn9.3 & 65 27 28.4 &  33.1 &  1.2 
    &&RXS J180209.6+652736 & 8& i &   6 &   6.0 &  2.5 && E & \nd  & \nd &    $>$22.5  &   \nl
1803.0+6450 & 18  \phn3  \phn0.8 & 64 50 16.5 &   1.5 &  0.1 
    &&RXS J180301.6+645028 &13& i &   8 &   7.6 &  3.1 && S & -3   & 1   &\phg 20.5 b  &   \nl
1805.2+6415 & 18  \phn5 11.8 & 64 15 55.1 &   3.4 &  0.5 
    &&RXS J180508.6+641609 &25& o &   5 &   4.3 &  1.9 && E & \nd  & \nd &    $>$22.5  &   \nl
1805.7+6701 & 18  \phn5 42.4 & 67  \phn1 35.3 &   0.9 &  0.2 
    &&RXS J180541.6+670139 & 6& i &  31 &  18.7 &  4.2 && G &  2   & 3   &\phg 20.0 b  &   \nl
1807.9+6509 & 18  \phn7 53.9 & 65  \phn9 40.5 &   2.5 &  0.2 
    &&RXS J180753.0+650952 &13& i &   7 &   9.9 &  4.4 && S &  1   & 2   &    $>$22.5  & \tablenotemark{10} \nl
1808.8+6744 & 18  \phn8 48.4 & 67 44 45.8 &   5.3 &  0.3 
    &&RXS J180847.9+674442 & 4& i &  12 &  14.6 &  5.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1812.1+6353 & 18 12  \phn8.4 & 63 53 40.5 &   1.2 &  0.2 
    &&RXS J181207.1+635334 &10& o &  20 &  19.7 &  4.4 && E & \nd  & \nd &    $>$22.5  &   \nl
1815.2+6619 & 18 15 10.2 & 66 19 48.4 &   2.2 &  0.1 
    &&RXS J181508.9+661930 &20& i &   7 &   9.1 &  4.1 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{11} \nl
1815.3+6507 & 18 15 20.1 & 65  \phn7 13.5 &  52.4 &  1.7 
    &&RXS J181519.3+650712 & 5& i &  12 &  28.8 &  8.5 && S & -1   & 1   &\phg 19.0 b  &   \nl
1817.7+6824 & 18 17 44.2 & 68 24 25.2 &  12.1 &  0.5
    &&RXS J181744.5+682432 & 7& o & 134 &  92.5 &  8.1 && G &  1   & 0   &\phg 20.0 b  & \tablenotemark{12} \nl
1820.0+6636 & 18 19 57.2 & 66 36 14.8 &   5.0 &  0.2 
    &&RXS J181955.2+663619 &13& o &  36 &  18.1 &  3.4 && S & -3   & 0   &\phg 16.0 b  & \tablenotemark{13} \nl
1820.3+6825 & 18 20 17.7 & 68 25 10.7 &   2.2 &  0.2 
    &&RXS J182014.7+682525 &22& o &   7 &   7.4 &  3.0 && E & \nd  & \nd &    $>$22.5  &   \nl
1823.9+6719 & 18 23 56.8 & 67 19 29.9 &   4.3 &  0.5 
    &&RXS J182355.0+671937 &12& o &  16 &  13.0 &  3.4 && E & \nd  & \nd &    $>$22.5  &   \nl
\enddata
\tablenotetext{1}{1732.9+6533  = 8C 1732+655 = 4C +65.21. Optical: 17.6 mag quasar with z = 0.856 (NED).
      As this radio source is off-axis with degraded VLA position, we accept the published quasar identification. }  
\tablenotetext{2}{1747.2+6813 Optical: B = 20 mag stellar object lies 8\arcsec N of the radio source.}
\tablenotetext{3}{1747.2+6532  = 8C 1747+655 = 4C 65.22. Optical: $R = 21.2$ mag galaxy with $z = 1.516$ (Kollgaard \etal 1995).
      Lacy \etal (1993) initially listed 4C 65.22 as a possible quasar at $z \simeq 1.5$, but
      Kollgaard \etal (1995) argue it is a radio galaxy.  Its X-ray
      luminosity of $\sim 5 \times 10^{45}$ erg s$^{-1}$ would then be extraordinarily
      high for either a broad-line radio galactic nucleus or an intracluster medium.}
\tablenotetext{4}{1748.5+7005 = S5 1749+70.  Optical: Well-studied $V = 17.0$ mag (Rusk \& Seaquist 1985) BL Lac object with z = 0.77 (NED).}
\tablenotetext{5}{1748.6+6842  = Mkn 507 = IRAS 17489+6843. Optical: B = 16.3 mag Seyfert 1 galaxy with z = 0.053 (Veron).}
\tablenotetext{6}{1755.1+6519  = IRAS F17549+6520. Optical: Seyfert 1 galaxy with z = 0.0803 (NED). 
      The stated magnitude from the APM is probably too bright, COSMOS gives B = 17.5 (no published magnitude).}
\tablenotetext{7}{1759.3+6902  Optical: 19 mag galaxy lies 9\arcsec SE of the radio source.}
\tablenotetext{8}{1800.1+6636  = NGC 6552 (CGCG 1800.1+6636). Optical: $V = 14.6$ Seyfert 2 galaxy 
      with z = 0.026 (NED); $IRAS$ source (2.5 Jy at 60$\mu$m and 3.1 Jy at 100 $\mu$m; Ashby \etal 1996).}
\tablenotetext{9}{1800.5+6705 X-ray: Steep X-ray spectrum.  Optical: Approximately 17 mag stellar object 
      lies 10\arcsec S of the radio source.} 
\tablenotetext{10}{1807.9+6509 Optical: detected on red plates ($R = 19.9a$) but not on blue.}
\tablenotetext{11}{1815.2+6619 Optical: B = 18 mag stellar object 12\arcsec SW of the radio source.}
\tablenotetext{12}{1817.7+6824 Broad-band properties (log\lbrack{\it f}$_x$/{\it f}$_r$ \rbrack ~ {\it vs.}
      log\lbrack{\it f}$_o$/{\it f}$_r$ \rbrack, see Fig. 10) suggest this object may have a hidden AGN.}
\tablenotetext{13}{1820.0+6636 Optical: unusually bright but radio faint object, possibly a new AGN.   
      It has not been studied. }
\end{deluxetable}


\begin{deluxetable}{lrrrrrrrrrrrrlrrlc}
\tablecolumns{18}
\tablewidth{0pt}
\tablenum{2}
\tablecaption{Extended X-ray/Radio Sources in the NEP}
\tablehead{
\multicolumn{5}{c}{Radio Data} & \colhead{} & \multicolumn{6}{c}{X-ray Data} &\colhead{} &  \multicolumn{4}{c}{Optical Data} & \colhead{Notes} \\
\cline{1-5} \cline{7-12} \cline{14-17} & \\
\multicolumn{1}{c}{VLA Source} & \multicolumn{1}{c}{$\alpha_{2000}$} & \multicolumn{1}{c}{$\delta_{2000}$} & 
\multicolumn{1}{c}{S$_{1.5}$} & \multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{ROSAT source} &
\multicolumn{1}{c}{$\Delta$} & \multicolumn{1}{c}{Loc} & \multicolumn{1}{c}{MaxL} & \multicolumn{1}{c}{F$_x$} & 
\multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{$\Delta\alpha$} & 
\multicolumn{1}{c}{$\Delta\delta$} & \multicolumn{1}{c}{B} & 
}
\startdata
1741.3+6508 & 17 41 16.0 & 65  \phn8 \phn6.0 &   2.8 &  0.3
    &&RXS J174114.3+650748 &21& o &  20 &  16.4 &  4.0 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{1} \nl
1743.1+6732 & 17 43 \phn7.8 & 67 32 32.5 &  17.8 &  0.6
    &&RXS J174312.1+673220 &27& i &   7 &  11.5 &  4.8 && G & 6    & -1  &\phg 16.0 c  & \tablenotemark{2} \nl
1743.4+6342 & 17 43 23.5 & 63 42 57.8  & 214.4 &  9.5 
    &&RXS J174328.0+634145 &78& o &  69 &  59.8 &  7.0 && Gp& \nd  & \nd &\phg 21.5    & \tablenotemark{3} \nl
1744.7+6750 & 17 44 42.9 & 67 50 47.1 &  38.1 &  1.5
    &&RXS J174444.3+675035 &14& i &   5 &  10.0 &  4.9 && S & -4   & -1  &\phg 21.0 a  & \tablenotemark{4} \nl
1746.1+6421 & 17 46 \phn6.4 & 64 21 49.5 & 237.4 &  7.4 
    &&RXS J174605.0+642150 & 9& o &  10 &   9.5 &  3.1 && S &  1   &  0  &\phg 21.0 b  & \tablenotemark{5} \nl
1747.3+6701 & 17 47 20.7 & 67 \phn1 23.5  &  48.4 &  1.5 
    &&RXS J174721.6+670211 &48& i &  28 &  18.5 &  4.7 && S &  5   & 40  &\phg 20.5 c & \tablenotemark{6} \nl
1747.4+6702 & 17 47 22.8 & 67 \phn2 31.0  &  \nd  &  \nd
    &&RXS J174721.6+670211 &21& i &  28 &  18.5 &  4.7 &&\nd& \nd  & \nd &    \nd      & \tablenotemark{6} \nl
1747.5+6345 & 17 47 30.9 & 63 45 28.1 &  77.3 &  3.2 
    &&RXS J174734.0+634511 &27& o &  10 &  20.0 &  5.1 && G & -3   & -3  &\phg 20.0 b  & \tablenotemark{7} \nl
1748.4+6404 & 17 48 23.0 & 64 \phn4 \phn5.6 &   1.4 &  0.1 
    &&RXS J174822.8+640340 &25& o &  17 &  15.7 &  3.8 && S &  1   &  2  &\phg 17.5 b  & \tablenotemark{8} \nl
1748.5+6404 & 17 48 27.6 & 64 \phn4 \phn5.8 &  \nd  & \nd  
    &&RXS J174822.8+640340 &40& o &  17 &  15.7 &  3.8 &&\nd&  \nd & \nd &    \nd  & \tablenotemark{8} \nl
1749.4+6631 & 17 49 21.5 & 66 31 52.4  &   6.7 &  0.2 
    &&RXS J174918.3+663146 &20& i &  16 &  11.2 &  3.4 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{9} \nl
1749.8+6824 & 17 49 48.1 & 68 24 \phn1.4  &  \nd  & \nd  
    &&RXS J174948.1+682325 &36& o &   8 &   7.8 &  2.8 &&\nd& \nd  & \nd &    \nd      & \tablenotemark{10} \nl
1749.8+6823 & 17 49 50.5 & 68 23 11.0  &   7.7 &  0.3 
    &&RXS J174948.1+682325 &19& o &   8 &   7.8 &  2.8 && Gp& \nd  & \nd &\phg 16.     & \tablenotemark{10} \nl
1751.1+6531 & 17 51 \phn6.6 & 65 31 52.5 &   0.6 &  0.1 
    &&RXS J175107.7+653204 &13& i &   7 &   8.6 &  1.7 && Gp& \nd  & \nd &\phg 15.4    & \tablenotemark{11} \nl
1751.4+6719 & 17 51 25.9 & 67 19 27.8 &   2.4 &  0.2 
    &&RXS J175130.2+671910 &31& i &  13 &  38.4 &  7.7 && Gp&  9   &  5  &\phg 17.7 c  & \tablenotemark{12} \nl
1751.6+6719 & 17 51 35.2 & 67 19 43.7 & \nd   & \nd  
    &&RXS J175130.2+671910 &45& i &  13 &  38.4 &  7.7 &&\nd& \nd  & \nd &    \nd      & \tablenotemark{12} \nl
1751.9+6454A& 17 51 51.8 & 64 54 50.4  & \nd   & \nd  
    &&RXS J175151.3+645511 &21& i &   5 &   9.6 &  7.2 &&\nd& \nd  & \nd &    \nd      & \tablenotemark{13} \nl
1751.9+6454B& 17 51 53.6 & 64 54 18.5  & 129.7 &  4.1 
    &&RXS J175151.3+645511 &55& i &   5 &   9.6 &  7.2 && S &  4   &  0  &\phg 19.0 a  & \tablenotemark{13} \nl
1752.0+6551 & 17 51 58.8 & 65 51 23.4 &  36.9 &  1.2 
    &&RXS J175157.3+655128 &10& i &  57 &  34.9 &  6.5 && G & \nd  & \nd &\phg 17.0    & \tablenotemark{14} \nl
\enddata
\tablenotetext{1}{1741.3+6508  Radio: possible triple, 24\arcsec separation.}
\tablenotetext{2}{1743.1+6732  Radio: extended about 30\arcsec, possibly with strong core.  Optical: Uncatalogued
             16 mag galaxy, possibly elliptical with companion; $\sim$ dozen galaxies $>$18 mag within 10\arcmin.} 
\tablenotetext{3}{1743.4+6342 = 8C 1743+637.  X-ray: extended ($ML_{ext}=16.8$). Radio: extended, 30\arcsec; 
             located in the outer region of the extended X-ray structure. 
             Optical: 21.5 mag galaxy in the region of Abell 2280 (z = 0.326, Gioia \etal 1995).  
             However, Lacy \etal (1993) suggest this galaxy is at much higher redshift.  
             Abell 2280 has Richness Class 0, Bautz-Morgan Class II-III, and Distance Class 6 (Abell \etal 1989).  
             Cluster of very faint galaxies seen on POSS I (Fig. 5a).}
\tablenotetext{4}{1744.7+6750  Radio: extended, 30\arcsec.}
\tablenotetext{5}{1746.1+6421 = 8C 1745+644. Radio: extended, 24\arcsec. Optical: stellar object B = 21.5a (-4.0, -0.7). 
             21.9 mag quasar with z = 1.228 (NED).}
\tablenotetext{6}{1747.3+6701 and 1747.4+6702  Radio: double, 66\arcsec separation. Optical: B = 20.5 stellar object 
             coincides with the X-ray position; both lie midway between the radio components. }
\tablenotetext{7}{1747.5+6345  Radio: possibly extended, 24\arcsec. }
\tablenotetext{8}{1748.4+6404 and 1748.5+6404  Radio: probably double, 28\arcsec.  Optical: possibly merged stellar objects.
             COSMOS magnitude is B = 18.9. }
\tablenotetext{9}{1749.4+6631  Radio: double, 36\arcsec separation, or core of a core-dominated triple, 95 arcsecond extent 
             oriented SE-NW.  Optical: B$\sim$19 optical objects 24\arcsec away from the core to the south and west.}
\tablenotetext{10}{1749.8+6824 and 1749.8+6823  Radio: possible double, 54\arcsec separation, and 13 mJy
             compact radio source (1749.9+6824) to the NE. Optical: Galaxy group.  The NE radio source is associated with 
             CGCG 1750.1+6825, 15.2 mag with z = 0.05122 (NED). 1749.8+6824 is associated with MCG +11-22-005, 17 mag.  
             1749.8+6823 is associated with KUG 1750+683A, 16 mag (NED).  The RASS source is from the outer region where 
             extent measurements are not accurate. (Fig. 5b).}
\tablenotetext{11}{1751.1+6531  = NGC 6505 (CGCG 1751.1+6533).  X-ray: extended($ML_{ext}=16.3$).  Optical: 
             E/SO galaxy with B = 15.4, z = 0.0389 (NED) with galaxy group (Henry \etal 1995; Fig. 5c).}
\tablenotetext{12}{1751.4+6719 and 1751.6+6719  X-ray: extended ($ML_{ext}=15.1$).  Radio: triple structure; 1751.4+6719 
             is the apparent core, with lobes 1751.6+6719 and 1751.2+6719 (Kollgaard \etal 1994). 
             Optical: Galaxy group.  The central radio source is associated with two B = 17.7 c galaxies.  COSMOS classifies 
             the nearby 18 mag objects as stellar, but locates many objects near the plate limit. (Fig. 5d).} 
\tablenotetext{13}{1751.9+6454A and 1751.9+6454B = 8C 1751+649.  Radio: double, 36\arcsec separation.
             Optical: The 19.0 a mag stellar object lies between the radio sources.}
\tablenotetext{14}{1752.0+6551  = 7C 1751+6551 Radio: double, 30\arcsec separation. Optical: 17.0 mag galaxy (NED).}
\end{deluxetable}


\begin{deluxetable}{lrrrrrrrrrrrrlrrlc}
\tablecolumns{18}
\tablewidth{0pt}
\tablenum{2}
\tablecaption{(continued)}
\tablehead{
\multicolumn{5}{c}{Radio Data} & \colhead{} & \multicolumn{6}{c}{X-ray Data} &\colhead{} &  \multicolumn{4}{c}{Optical Data} & \colhead{Notes} \\
\cline{1-5} \cline{7-12} \cline{14-17} & \\
\multicolumn{1}{c}{VLA Source} & \multicolumn{1}{c}{$\alpha_{2000}$} & \multicolumn{1}{c}{$\delta_{2000}$} & 
\multicolumn{1}{c}{S$_{1.5}$} & \multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{ROSAT source} &
\multicolumn{1}{c}{$\Delta$} & \multicolumn{1}{c}{Loc} & \multicolumn{1}{c}{MaxL} & \multicolumn{1}{c}{F$_x$} & 
\multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{$\Delta\alpha$} & 
\multicolumn{1}{c}{$\Delta\delta$} & \multicolumn{1}{c}{B} & 
}
\startdata
1753.6+6634 & 17 53 36.4 & 66 34 37.1 & 357.2 & 15.6 
    &&RXS J175334.9+663440 & 9& i &   7 &   4.8 &  1.9 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{15} \nl
1753.6+6542 & 17 53 38.5 & 65 42 18.7  & 453.4 & 17.9 
    &&RXS J175341.7+654251 &38& i &  38 &  10.6 &  5.2 && G & \nd  & \nd &\phg 19.7 b  & \tablenotemark{16} \nl
1753.8+6542 & 17 53 45.2 & 65 42 57.8  & \nd   & \nd  
    &&RXS J175341.7+654251 &23& i &  38 &  10.6 &  5.2 &&\nd& \nd  & \nd &    \nd      & \tablenotemark{16} \nl
1754.1+6452 & 17 54 \phn7.3 & 64 52 \phn3.1 & 147.8 &  4.9 
    &&RXS J175405.6+645201 &11& i &   6 &   8.7 &  3.9 && G &   2  &  0  &\phg 20.0 b  & \tablenotemark{17} \nl
1755.4+6803 & 17 55 24.9 & 68 \phn3 12.9 &   6.3 &  0.3 
    &&RXS J175514.7+680324 &58& i &   8 &  87.7 & 13.3 && Gp& \nd  & \nd &    $>$22.5  & \tablenotemark{18} \nl 
1755.7+6754 & 17 55 43.5 & 67 54 10.8 &   1.8 &  0.1 
    &&RXS J175546.7+675421 &21& i &   8 &  98.8 & 14.6 && Gp&  -4  &  -2 &$\sim$16. c  & \tablenotemark{19} \nl
1756.5+6512 & 17 56 29.2 & 65 12 50.1 &   7.6 &  0.4 
    &&RXS J175632.2+651233 &25& i &  14 &  13.2 &  4.3 && Gp& \nd  & \nd &\phg 15.6    & \tablenotemark{20} \nl
1758.6+6637 & 17 58 33.5 & 66 37 58.9  & 939.4 & 31.8 
    &&RXS J175833.4+663758 & 1& i & 169 &  19.6 &  1.8 && PN& \nd  & \nd &\phg  8.9    & \tablenotemark{21} \nl 
1801.2+6902 & 18  \phn1 14.5 & 69  \phn2 40.4 & 202.7 &  6.3 
    &&RXS J180115.3+690244 & 6& o &   8 &   7.5 &  2.7 && S &  0   &  3  &\phg 19.4    & \tablenotemark{22} \nl
1802.0+6657 & 18 \phn1 57.8 & 66 57 14.7 &  23.0 &  0.7 
    &&RXS J180155.5+665540 &95& i &  11 &   2.9 &  0.9 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{23} \nl 
1803.9+6548 & 18  \phn3 54.0 & 65 48 25.0 &  43.1 &  1.7 
    &&RXS J180353.9+654827 & 3& i & 152 &  57.5 &  6.6 && G &  1   &  0  &\phg 20.5 b  & \tablenotemark{24} \nl
1805.3+6621 & 18  \phn5 16.3 & 66 21  \phn9.8 &   7.0 &  0.3 
    &&RXS J180515.8+662053 &16& i &   6 &   5.9 &  2.2 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{25} \nl
1805.5+6535 & 18  \phn5 30.5 & 65 35 22.7 &   3.4 &  0.1 
    &&RXS J180532.5+653521 &13& i &   7 &  13.8 &  4.8 && S &  5   & -3  &\phg 20.0 c  & \tablenotemark{26} \nl
1806.8+6536 & 18  \phn6 46.4 & 65 36 37.1  &  11.1 &  0.4 
    &&RXS J180651.6+653740 &71& i &  34 &  47.5 &  8.3 && Gp&  5   &  2  &\phg 20.0 c  & \tablenotemark{27} \nl 
1808.1+6605 & 18  \phn8  \phn3.8 & 66  \phn5 33.3 &  17.7 &  0.6 
    &&RXS J180803.4+660531 & 3& i &  17 &  11.1 &  3.2 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{28} \nl
\enddata
\tablenotetext{15}{1753.6+6634  = 7C 1753+6635  Radio: possible double with 1753.6+6635, 72\arcsec separation. 
             Optical: Two B = 18.0 c stellar objects lie within the radio structure, but identification is unclear.}
\tablenotetext{16}{1753.6+6542 and 1753.8+6542 = 8C 1753+657. Radio: double, 54\arcsec separation. Optical: 
             $B = 19.9$, $R = 17.4$ mag quasar with z = 0.148 (Lacy \etal 1995, Kock \etal 1996). Quasar and RASS source lie between the radio peaks.}
\tablenotetext{17}{1754.1+6452  Radio: possibly extended, 36\arcsec.}
\tablenotetext{18}{1755.4+6803  X-ray: Gioia \& Luppino (1994) note slightly extended X-ray emission from the EMSS cluster 
              MS1754.9+6803 (z = 0.077), but it is uncertain whether the RASS-VLA source is physically related to the 
              EMSS cluster.  Radio: double, 18\arcsec separation. Optical: Galaxy group. (Fig. 5e).}
\tablenotetext{19}{1755.7+6754  X-ray: extended ($ML_{ext}=31.0$). Radio: faint.  Optical: Erroneously classified by COSMOS 
              as a 16.4 mag star surrounded by a cluster of 21 mag objects.  POSS I image indicates an elliptical galaxy 
              with a diffuse halo $\simeq$40\arcsec in extent.  Possible cD galaxy in cluster. (Fig. 5f).}
\tablenotetext{20}{1756.5+6512  = CGCG 1756.3+6513. X-ray: extended ($ML_{ext}=26.5$).  
             Radio: coincides with bright spot in complex X-ray structure.
             Optical: B = 15.6 E/S0 galaxy with z = 0.0263 (NED) in group (Henry \etal 1995).  (Fig. 5g).}
\tablenotetext{21}{1758.6+6637  = NGC 6543 = IRAS 17584+6638.  X-ray: Kreysing \etal 1992 found extended X-ray emission.
             Radio: extended, 36\arcsec.  Optical: Galactic planetary nebula.}
\tablenotetext{22}{1801.2+6902  = 8C 1801+690.  Radio: extended, 24\arcsec. Optical: 19.4 mag quasar with z = 1.271 (NED).}
\tablenotetext{23}{1802.0+6657  Radio: double with 1802.1+6657, separation 54\arcsec with marginally resolved core.
             Optical: No object found near core. Contour map in Kollgaard \etal (1994).}
\tablenotetext{24}{1803.9+6548  X-ray: possibly extended ($ML_{ext}=6.8$). Radio: possibly extended, 36\arcsec.  
             The low likelihood of X-ray extension and precisely coincident radio and X-ray centroids suggest it is an 
             unresolved active nucleus rather than a group candidate.}
\tablenotetext{25}{1805.3+6621  Radio: possibly extended, 30\arcsec. Optical: 17.5 c mag stellar object located 
             12\arcsec NW of the radio source.}
\tablenotetext{26}{1805.5+6535  Radio: double or triple, 30\arcsec separation. Contour map in Kollgaard \etal (1994).
             Optical: B = 20.0 c stellar object coincident with brightest radio component.  Several other faint
             objects lie within 1\arcmin.}
\tablenotetext{27}{1806.8+6536  X-ray: extended ($ML_{ext}=10.8$). Radio: unresolved. Optical: Several 19-20 mag objects lie 
             within 1\arcmin.  Possible distant galaxy group. (Fig. 5i).}
\tablenotetext{28}{1808.1+6605  = 7C 1807+6604. Radio: double, 24\arcsec separation. Optical: No optical object lies 
             coincident with, or between, the radio components.  An extremely red star lies $\simeq$20\arcsec S of the radio 
             source, and is associated with a stellar $IRAS$ source (0.42 Jy at 12$\mu$m, 0.12 Jy at 25$\mu$m; Hacking \& Houck
             1987).  The star, listed in the  HST Guide Star Catalog (GSC 4213 596, $V = 9.4$,
             18 08 03.3, +66 05 10), has recently been classified as a K star by Kuemmel \etal (1998, private communication) using the 2.5m Guillermo Haro telescope of INAOE, Mexico.} 
\end{deluxetable}


\begin{deluxetable}{lrrrrrrrrrrrrlrrlc}
\tablecolumns{18}
\tablewidth{0pt}
\tablenum{2}
\tablecaption{(continued)}
\tablehead{
\multicolumn{5}{c}{Radio Data} & \colhead{} & \multicolumn{6}{c}{X-ray Data} &\colhead{} &  \multicolumn{4}{c}{Optical Data} & \colhead{Notes} \\
\cline{1-5} \cline{7-12} \cline{14-17} & \\
\multicolumn{1}{c}{VLA Source} & \multicolumn{1}{c}{$\alpha_{2000}$} & \multicolumn{1}{c}{$\delta_{2000}$} & 
\multicolumn{1}{c}{S$_{1.5}$} & \multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{ROSAT source} &
\multicolumn{1}{c}{$\Delta$} & \multicolumn{1}{c}{Loc} & \multicolumn{1}{c}{MaxL} & \multicolumn{1}{c}{F$_x$} & 
\multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{$\Delta\alpha$} & 
\multicolumn{1}{c}{$\Delta\delta$} & \multicolumn{1}{c}{B} & 
}
\startdata
1808.8+6634 & 18  \phn8 49.7 & 66 34 30.4 &  26.2 &  0.8 
    &&RXS J180850.2+663426 & 5& i & 134 &  50.6 &  6.4 && S & -1   & -1  &\phg 17.5 b  & \tablenotemark{29} \nl
1809.0+6704 & 18  \phn9  \phn0.6 & 67  \phn4 25.4 &  17.7 &  0.6 
    &&RXS J180859.7+670427 & 5& i &  20 &  19.3 &  5.3 && S &  1   &  0  &\phg 20.5 b  & \tablenotemark{30} \nl
1815.4+6806 & 18 15 24.0 & 68 \phn6 26.6  & 381.4 & 12.2 
    &&RXS J181521.5+680639 &19& i &  54 &  62.2 & 12.6 && G &  5   &  5  &\phg 17.8    & \tablenotemark{31} \nl 
1816.2+6627 & 18 16 11.6 & 66 27 \phn3.7 &   3.1 &  0.1 
    &&RXS J181611.2+662713 &10& i &   6 &  10.1 &  4.8 && G & 26   & 33  &\phg 18.5 c  & \tablenotemark{32} \nl 
1818.1+6349 & 18 18  \phn7.8 & 63 49 51.6 &  20.9 &  1.0 
    &&RXS J181805.8+634948 &14& o &   6 &   6.5 &  2.9 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{33} \nl
1819.6+6857 & 18 19 37.6 & 68 57 25.1  &  \nd  & \nd  
    &&RXS J181951.4+685704 &77& o &  24 &  93.2 & 11.2 &&\nd& \nd  & \nd &      \nd    & \tablenotemark{34} \nl 
1819.6+6856 & 18 19 38.4 & 68 56 30.8  &  \nd  & \nd  
    &&RXS J181951.4+685704 &78& o &  24 &  93.2 & 11.2 &&\nd& \nd  & \nd &      \nd    & \tablenotemark{34} \nl 
1819.7+6856 & 18 19 42.4 & 68 56 52.6  & 735.3 & 22.1 
    &&RXS J181951.4+685704 &50& o &  24 &  93.2 & 11.2 && Gp& \nd  & \nd &\phg 15.0    & \tablenotemark{34} \nl 
1821.8+6818 & 18 21 49.0 & 68 18 48.7 &  \nd  & \nd  
    &&RXS J182155.7+681852 &38& o &  15 &  14.9 &  4.3 &&\nd& \nd  & \nd &      \nd    & \tablenotemark{35} \nl
1822.0+6818 & 18 21 59.3 & 68 18 43.4 & 185.9 &  6.2 
    &&RXS J182155.7+681852 &22& o &  15 &  14.9 &  4.3 && S &   1  & -1  &\phg 21.0 c  & \tablenotemark{35} \nl
1822.1+6637 & 18 22  \phn3.5 & 66 37 14.8 &  10.7 &  0.5 
    &&RXS J182203.6+663713 & 1& o &   6 &   4.9 &  2.2 && G & \nd  & \nd &\phg 14.0    & \tablenotemark{36} \nl
1826.6+6706 & 18 26 37.4 & 67  \phn6 44.4 & 107.6 &  3.6 
    &&RXS J182636.9+670645 & 3& o &  38 &  34.0 &  5.5 && G &  0   &  0  &\phg 17.7    & \tablenotemark{37} \nl
\enddata
\tablenotetext{29}{1808.8+6634  Radio: possibly extended, 36\arcsec.} 
\tablenotetext{30}{1809.0+6704  Radio: may be northern component of triple source with 1808.9+6703 and 1809.0+6702, extent 
             54\arcsec. Contour map in Kollgaard \etal (1994).}
\tablenotetext{31}{1815.4+6806  = 8C 1815+680 = 4C 68.20.  Radio: extended, 48\arcsec. Optical: R = 17.8 mag 
             broad line radio galaxy at z = 0.23 (Veron).  Numerous B$\sim$20 stars or galaxies nearby; radio galaxy may be 
             a member of a group, but X-ray source unlikely to be group emission.}
\tablenotetext{32}{1816.2+6627  Radio: extended 36\arcsec SE-NW. Contour map in Kollgaard \etal (1994). Optical: The NW 
             portion coincides with the V = 10.5 K0 star BD +66$^\circ$1092 (SIMBAD).  The SE portion coincides with 
             a B = 18.5 c galaxy.  The table refers to the latter identification.}
\tablenotetext{33}{1818.1+6349  Radio: This source appears to be the SE lobe of a multiple-component source 3-4\arcmin
             in extent.  Contour map in Kollgaard \etal (1994). Optical: Several B = 17-18 stars or galaxies lie around 
             the radio sources, one of which coincides with radio component 1817.8+6351.  Given these uncertainties, we 
             classify this as an empty field. }
\tablenotetext{34}{1819.6+6857, 1819.6+6856 and 1819.7+6856  = 4C 68.21.  X-ray: extended ($ML_{ext}=28.9$). 
             Radio: triple source with 54\arcsec extent, head-tail with core morphology; located in the outer region 
             of the extended X-ray structure.  Optical: 15.0 mag galaxy in Abell 2304 with z = 0.0881 (NED) is coincident 
             with easternmost radio component (radio core).  
             Abell 2304 has Richness Class 0, Bautz-Morgan Class II, and Distance Class 5 (Abell \etal 1989).  (Fig. 5j).}
\tablenotetext{35}{1821.8+6818  and 1822.0+6818  Radio: probable double, 60\arcsec separation. Optical: a B = 21.0
             stellar object coincides with the brighter component.}
\tablenotetext{36}{1822.1+6637  = NGC 6636 = VV 679 = IRAS 18220+6635.  Radio: extended 24\arcsec, brightest at center 
             and located between the optical galaxies.  Optical: 14 mag SBc Seyfert 2 galaxy with z = 0.0133 with 16 mag 
             compact galaxy companion (NED).}
\tablenotetext{37}{1826.6+6706  = 7C 1826+6704. Radio: possibly extended, 48\arcsec. 
             Optical: 17.7 mag galaxy with z = 0.287 (NED).}
\end{deluxetable}


\begin{deluxetable}{lrrrrrrrrrrrrlrrlc}
\tablecolumns{18}
\tablewidth{0pt}
\tablenum{3}
\tablecaption{Possible Additional X-ray/Radio Sources in the NEP}
\tablehead{
\multicolumn{5}{c}{Radio Data} & \colhead{} & \multicolumn{6}{c}{X-ray Data} &\colhead{} &  \multicolumn{4}{c}{Optical Data} & \colhead{Notes} \\
\cline{1-5} \cline{7-12} \cline{14-17} & \\
\multicolumn{1}{c}{VLA Source} & \multicolumn{1}{c}{$\alpha_{2000}$} & \multicolumn{1}{c}{$\delta_{2000}$} & 
\multicolumn{1}{c}{S$_{1.5}$} & \multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{ROSAT source} &
\multicolumn{1}{c}{$\Delta$} & \multicolumn{1}{c}{Loc} & \multicolumn{1}{c}{MaxL} & \multicolumn{1}{c}{F$_x$} & 
\multicolumn{1}{c}{$\pm$} && \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{$\Delta\alpha$} & 
\multicolumn{1}{c}{$\Delta\delta$} & \multicolumn{1}{c}{B} & 
}
\startdata
1739.2+6907 & 17 39 14.1 & 69  \phn7 43.3 &   2.7 &  0.2 
    &&RXS J173917.3+690828 &48& o &   5 &   8.0 &  3.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1744.9+6642 & 17 44 53.5 & 66 42 53.7 &  29.8 &  1.1 
    &&RXS J174458.3+664339 &54& i &   6 &   7.9 &  3.8 && E & \nd  & \nd &    $>$22.5  &   \nl
1745.7+6620 & 17 45 44.0 & 66 20 14.6 &   2.5 &  0.2 
    &&RXS J174546.7+662056 &44& i &   6 &   7.5 &  3.4 && E & \nd  & \nd &    $>$22.5  &   \nl
1747.7+6345 & 17 47 42.4 & 63 45 \phn5.9 &   1.2 &  0.2 
    &&iRXS J174734.0+634511 &56& o &  10 &  20.0 &  5.1 && G &  -3  & -2  &\phg 21.5 b  &   \nl
1749.2+6632 & 17 49 12.2 & 66 32 \phn8.6 &   1.5 &  0.1 
    &&RXS J174918.3+663146 &42& i &  16 &  11.2 &  3.4 && E & \nd  & \nd &    $>$22.5  &   \nl
1749.5+6726 & 17 49 27.0 & 67 26 25.3 &   1.8 &  0.1 
    &&RXS J174934.5+672554 &53& i &   6 &   8.1 &  3.6 && E & \nd  & \nd &    $>$22.5  &   \nl
1751.0+6535 & 17 51 \phn0.9 & 65 35 54.2 &   1.1 &  0.1 
    &&RXS J175106.6+653559 &35& i &   6 &   9.5 &  4.1 && E & \nd  & \nd &    $>$22.5  &   \nl
1753.2+6619 & 17 53 13.7 & 66 19 49.8 &   8.0 &  1.0 
    &&RXS J175313.0+662020 &31& i &  10 &   6.7 &  2.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1755.2+6505 & 17 55 \phn9.6 & 65 \phn5 22.2  &  15.7 &  0.7 
    &&RXS J175519.8+650451 &71& i &  34 &  30.4 &  6.6 && S &   6  &  -1 &    $>$22.5  & \tablenotemark{1} \nl  
1756.2+6807 & 17 56 11.7 & 68 \phn7 59.1 &  2.8  &  0.1 
    &&RXS J175614.4+680712 &49& o & 336 &  77.5 &  5.0 && E & \nd  & \nd &    $>$22.5  &   \nl
1756.7+6531 & 17 56 40.1 & 65 31 46.2 &  56.5 &  1.8 
    &&RXS J175641.9+653123 &26& i &   7 &   7.4 &  2.9 && S &   2  &  0  &\phg 22.0 c  &   \nl
1756.8+6546 & 17 56 45.6 & 65 46 22.3 &  14.7 &  0.6 
    &&RXS J175651.7+654601 &43& i &   7 &   5.9 &  2.4 && E & \nd  & \nd &    $>$22.5  &   \nl
1757.1+6353 & 17 57 \phn7.3 & 63 53 15.4 &   1.0 &  0.1 
    &&RXS J175710.1+635235 &44& o &  43 &  21.6 &  3.6 && E & \nd  & \nd &    $>$22.5  &   \nl
1757.4+6536 & 17 57 23.3 & 65 36 10.4 &  45.6 &  1.8 
    &&RXS J175728.8+653539 &46& i &   8 &   6.7 &  2.6 && S &   4  &  0  &\phg 22.0 a  &   \nl
1758.1+6408 & 17 58 \phn6.6 & 64 \phn8 54.6 &   1.5 &  0.1 
    &&RXS J175801.2+640932 &52& o & 538 & 127.0 &  6.4 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{2}  \nl
1758.2+6729 & 17 58 12.1 & 67 29 27.3 &  13.7 &  0.5 
    &&RXS J175813.8+673006 &41& i &   6 &   6.1 &  2.5 && E & \nd  & \nd &    $>$22.5  &   \nl
1758.8+6607 & 17 58 50.5 & 66 \phn7 15.6 &   1.4 &  0.1 
    &&RXS J175853.3+660637 &41& i &   9 &   4.6 &  1.6 && G & -3   & -1  &\phg 18.0 c  & \tablenotemark{3} \nl
1759.4+6735 & 17 59 23.0 & 67 35 55.1 &  11.9 &  0.4 
    &&RXS J175919.8+673628 &38& i &   7 &   9.4 &  3.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1800.3+6739 & 18  \phn0 16.1 & 67 39 21.9 &   8.9 &  0.3 
    &&RXS J180013.4+673835&49& i &  11 &   8.6 &  3.0 && E & \nd  & \nd &    $>$22.5  &   \nl
1801.5+6645 & 18  \phn1 32.5 & 66 45  \phn8.6 &   3.6 &  0.3 
    &&RXS J180137.7+664526 &36& i &  10 &   3.4 &  1.0 && Gp& \nd  & \nd &    $>$22.5  &  \tablenotemark{4} \nl
1802.9+6450 & 18  \phn2 56.0 & 64 50 59.7 &   1.1 &  0.1 
    &&RXS J180301.6+645028 &47& i &   8 &   7.6 &  3.1 && E & \nd  & \nd &    $>$22.5  &   \nl
1805.2+6737 & 18  \phn5  \phn9.5 & 67 37 46.5 &   3.3 &  0.1 
    &&RXS J180514.9+673738 &32& i &   8 &  10.8 &  401 && E & \nd  & \nd &    $>$22.5  &   \nl
1806.4+6619 & 18  \phn6 25.1 & 66 19 57.4 &   1.3 &  0.2 
    &&RXS J180616.7+662009 &52& i &   5 &   4.7 &  2.0 && E & \nd  & \nd &    $>$22.5  &  \tablenotemark{5} \nl
1807.5+6557 & 18  \phn7 31.1 & 65 57 19.3 &   2.7 &  0.1 
    &&RXS J180723.7+655640 &60& i &  14 &  10.7 &  3.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1807.9+6617 & 18  \phn7 53.0 & 66 17 30.3 &  21.6 &  1.0 
    &&RXS J180747.6+661737 &34& i &  85 &  30.6 &  4.6 && E & \nd  & \nd &    $>$22.5  &   \nl
1808.8+6607 & 18  \phn8 49.8 & 66  \phn7  \phn8.5 &   4.0 &  0.2 
    &&RXS J180844.8+660624 &53& i &   7 &   6.5 &  2.6 && E & \nd  & \nd &    $>$22.5  &   \nl
1810.0+6345 & 18  \phn9 57.2 & 63 45  \phn2.6 &  44.5 &  2.1 
    &&RXS J181003.7+634426 &56& o &  56 &  36.3 &  5.1 && E & \nd  & \nd &    $>$22.5  &   \nl
1810.1+6634 & 18 10  \phn6.1 & 66 34 14.4 &   2.2 &  0.1 
    &&RXS J181006.1+663321 &53& i &   8 &   8.5 &  3.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1811.0+6810 & 18 10 59.2 & 68 10 29.0 &   9.2 &  0.7 
    &&RXS J181106.8+681044 &45& o &   5 &   5.2 &  2.3 && E & \nd  & \nd &    $>$22.5  &   \nl
1812.9+6533 & 18 12 52.6 & 65 33 44.7 &   1.4 &  0.1 
    &&RXS J181246.2+653350 &40& i &  30 &  24.5 &  6.1 && E & \nd  & \nd &    $>$22.5  &   \nl
1813.5+6641 & 18 13 30.0 & 66 41 55.9 &   1.8 &  0.2 
    &&RXS J181339.3+664132 &60& i &   5 &   8.2 &  3.8 && E & \nd  & \nd &    $>$22.5  & \tablenotemark{6} \nl
1819.9+6749 & 18 19 55.5 & 67 49 10.3 &  15.9 &  0.6 
    &&RXS J181952.8+674820 &52& o &   6 &   8.4 &  3.4 && G &  5   & -1  &\phg 19.5 c  &   \nl
\enddata

\tablenotetext{1}{1755.2+6505  Radio: possibly extended, 36\arcsec.}
\tablenotetext{2}{1758.1+6408  Radio/X-ray offset exceeds 40\arcsec.  X-ray: very bright. Radio: faint and unresolved. 
          Optical: X-ray position coincides with unstudied V =  10.6 G star BD 64$^\circ$1235 = SAO 17709 (SIMBAD).}
\tablenotetext{3}{1758.8+6607  Radio/X-ray offset exceeds 40\arcsec.  Radio: faint and unresolved.  Optical: 
          $IRAS$ detected starburst galaxy (0.07 Jy at 60$\mu$m and 0.11 Jy at 100 $\mu$m) with z = 0.0799, member of 
          massive supercluster (Ashby \etal  1996).}
\tablenotetext{4}{1801.5+6645  Optical: associated with NEPX1, an X-ray-selected galaxy cluster with z = 0.09 
          (Burg \etal 1992; Hasinger \etal 1991). (Fig. 5h).}
\tablenotetext{5}{1806.4+6619  Possibly associated with $IRAS$-detected triple galaxy, 0.6\arcmin distant
          (z=0.107; 0.09 Jy at 60$\mu$m and $<$0.1 Jy at 100 $\mu$m; Ashby \etal 1996).}
\tablenotetext{6}{1813.5+6641  = IRAS F18135+6641.}
\end{deluxetable}

\end{document}
