\begin{table}%ta2
      \caption{\label{table.xmmnewton}Optical/near-infrared counterparts of EPIC/{\em XMM-Newton} 
      sources in Franciosini et~al. (2006) not listed in 
      Tables~\ref{table.beyond} or~\ref{table.xraydetections}.}   
 %%\centerline
\par
{\small
 \begin{tabular}{l cc c ll}
            \hline
            \hline
            \noalign{\smallskip}
NX		& $\alpha$ 	& $\delta$ 	& {\it CR}	    	& Name  		& Class			\\
(Fr06)		& (J2000)	& (J2000)	& [ks$^{-1}$]   & 			& 			\\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
4		& 05 38 00.56	& --02 45 09.7	&  $9.7\pm1.0$  & Mayrit 861230		& Possible young star	\\ % 
6		& 05 38 06.50	& --02 28 49.4	& $0.67\pm0.18$ & Mayrit 717307		& Young star		\\ % 
7		& 05 38 06.74 	& --02 30 22.8 	& $19.0\pm0.9$  & Mayrit 662301		& Young star		\\ % Bright X-ray stars absent in our work: NX~7 (Mayrit~662301, Kiso A-0904~67).
11		& 05 38 13.20	& --02 26 08.8	&  $1.6\pm0.3$  & Mayrit 757321		& Young star		\\ % 
14		& 05 38 15.53	& --02 42 05.1	&  $2.7\pm0.4$  & [FPS2006] NX 14	& Possible galaxy	\\ % NX 41 in LC2008, blue i-Ks, unknown
17		& 05 38 17.78	& --02 40 50.1	& $0.97\pm0.17$ & Mayrit 498234		& Young star		\\ % 
25		& 05 38 23.32	& --02 44 14.2	& $0.85\pm0.17$ & Mayrit 589213		& Young star		\\ % 
26		& 05 38 23.55	& --02 41 31.8	& $0.96\pm0.19$ & Mayrit 459224		& Young star		\\ % 
33		& 05 38 27.51	& --02 35 04.2 	&  $1.5\pm0.4$  & Mayrit 265282		& Young star		\\ % In the innermost 5~arcmin: NX~33 (Kiso A-0976 329, S~Ori~J053827.5--023504).
42		& 05 38 30.98	& --02 34 03.8	& $0.64\pm0.13$ & [FPS2006] NX 42	& Possible field star	\\ % Prob. fore. star?
47		& 05 38 32.68	& --02 31 15.6	& $0.57\pm0.13$ & [KJN2005] 3.01 325	& Field star		\\ % Non-member in Sacco et~al. 2008
50		& 05 38 33.02	& --02 39 27.9	& $0.53\pm0.11$ & [FPS2006] NX 50	& Possible field star?	\\ % New candidate member?
67		& 05 38 39.13	& --02 28 00.4	&  $1.3\pm0.2$  & Mayrit 487350		& Young brown dwarf	\\ % Interesting: [SE2004]~70 + S~Ori~68.
82		& 05 38 45.98	& --02 45 23.2	& $0.73\pm0.18$ & Mayrit 563178		& Possible young star	\\ % 
89		& 05 38 47.66	& --02 30 37.4	&  $2.2\pm0.5$  & Mayrit 326008		& Young star		\\ % 
97$^{a}$	& 05 38 49.93	& --02 41 22.8	& $1.08\pm0.15$ & Mayrit 332167		& Young star		\\ % 
100		& 05 38 50.39	& --02 26 47.7	&  $1.0\pm0.2$  & Mayrit 559009		& Young star		\\ % 
101		& 05 38 51.01	& --02 27 45.7	& $0.70\pm0.17$ & [KJN2005] 1.02 156 AB	& Field star		\\ % SB, non-member in Sacco et~al. 2008 
111		& 05 38 54.92	& --02 28 58.3	& $0.69\pm0.16$ & Mayrit 449020		& Young star		\\ % 
114		& 05 38 56.99	& --02 31 25.6	& $0.65\pm0.13$ & SO110979		& Field star		\\ % 
116		& 05 38 58.84	& --02 34 13.2	& $0.63\pm0.13$ & [D90] 3		& Radiogalaxy		\\ % 
118		& 05 38 59.23	& --02 33 51.4	& $0.25\pm0.07$ & Mayrit 252059		& Young star		\\ % In the innermost 5~arcmin: NX~118 (Haro 5-18, SWW~227).
147		& 05 39 12.32	& --02 30 06.4	&  $2.1\pm0.4$  & Mayrit 544049 	& Possible young star	\\ % 
149		& 05 39 14.47	& --02 28 33.4 	& $10.9\pm0.6$  & Mayrit 631045		& Possible young star	\\ % Bright X-ray stars absent in our work: NX~149 (Mayrit~631045, S~Ori~J053914.5--022834).
157		& 05 39 18.97	& --02 30 55.6	&  $3.0\pm0.4$  & Mayrit 596059 	& Young star?		\\ % 
160		& 05 39 20.97	& --02 30 33.5	&  $5.8\pm0.5$  & Mayrit 633059		& Young star		\\ % Moderately bright: NX~160 (Mayrit~633059, S~Ori~3).
167		& 05 39 26.73	& --02 26 17.4	&  $2.9\pm0.6$  & Mayrit 856047 	& Young star		\\ % 
169		& 05 39 50.56	& --02 38 27.0	&  $1.8\pm0.3$  & [SWW2004] 222 AB	& Field star		\\ % % NX 169; SB and no member in Sa08; [SWW2004] J053930.567-023826.96
174		& 05 39 39.83	& --02 33 16.0	& $19.8\pm1.0$  & Mayrit 841079		& Young star		\\ % Bright X-ray stars absent in our work: NX~174 (Mayrit~841079, V603~Ori, source of Herbig-Haro object HH~445).
175		& 05 39 39.99 	& --02 43 09.7	&  $1.9\pm0.5$  & Mayrit 931117		& Young star		\\ % 
         \noalign{\smallskip}
            \hline
         \end{tabular}}
\tablefoot{\tablefoottext{a}{Star NX~97 (\object{Mayrit~332167}, [SWW2004]~200) has colours,
lithium, radial velocity, and H$\alpha$ emission consistent with membership in
cluster (Sacco et~al. 2008). Its Mayrit number is first given here.}}
   \end{table}