\begin{table}%ta1c
%\caption{continued.} 
%\centerline
{\small
\begin{tabular}{cccccccccccccc}
\hline\hline
CMaX &	Err&Cnt/ks	&			$S/N$&		log$L_{\rm x}$ &	RA  	&	Dec  	&	$R$	&	$A_V$	&	$J$	  &	$H$	     &	$K$	       &	Age	&	Mass	\\
         &    ($''$)      &         &               &             & J2000  &  J2000    & (mag) &  (mag)  &   (mag) &    (mag) &  (mag)   &  (Myr)    &   ($M_{\odot}$)  \\
%\noalign{\smallskip}
\hline
60	&	30	&	1.5	$\pm$	0.9	&	1.6	&	30.20	&	7 03 30.4	&
	$-11$ 48 07	&	13.7	&	2.4	&	13.5	&	13.0	&	12.8	&	20--50	&	1.0--1.5	 \\
61$^x$	&	30	&	1.7	$\pm$	0.9	&	1.9	&	30.27	&	7 03 33.5	&	$-11$ 34 27	&	15.2	&	2.6	&	13.5	&	12.8	&	12.5	&	05--10	&	1.0--1.5	 \\	
62$^x$	&	30	&	1.5	$\pm$	0.9	&	1.7	&	30.20	&	7 03 42.1	&	$-11$ 35 14	&	15.5	&	2.5	&	13.4	&	12.6	&	12.4	&	02--05	&	1.5--2.0	 \\
63$^{*,g,x}$	&	30	&	2.5	$\pm$	1.0	&	2.5	&	30.43	&	7 03 43.2	&	$-11$ 33 06	&	9.1	&	3.4	&	6.5	&	5.2	&	3.8	&	??	&	??	 \\
64$^x$	&	30	&	2.9	$\pm$	1.1	&	2.7	&	30.49	&	7 03 47.5	&	$-11$ 31 49	&	13.8	&	1.3	&	13.5	&	12.8	&	12.6	&	01--02	&	0.5--1.0	 \\
65	&	30	&	1.2	$\pm$	0.8	&	1.5	&	30.11	&	7 03 48.2	&	$-11$ 41 46	&	14.0	&	0.3	&	13.6	&	12.8	&	12.6	&	??	&	??	 \\
66$^{j,x}$	&	30	&	6.2	$\pm$	1.4	&	4.3	&	30.82	&	7 03 51.5	&	$-11$ 34 56	&	--	&	--	&	11.0	&	10.8	&	10.7	&	01--02	&	3.0--5.0	 \\
67$^x$	&	30	&	2.1	$\pm$	1.0	&	2.2	&	30.35	&	7 03 52.5	&	$-11$ 26 17	&	16.0	&	1.4	&	13.7	&	12.9	&	12.6	&	??	&	??	 \\
68$^j$	&	30	&	2.0	$\pm$	1.0	&	2.1	&	30.34	&	7 03 54.0	&	$-11$ 32 37	&	14.1	&	2.3	&	14.6	&	13.7	&	13.3	&	2--5	&	0.5--1.0	 \\
69$^h$	&	30	&	7.9	$\pm$	1.6	&	4.9	&	30.93	&	7 03 54.4	&	$-11$ 28 29	&	9.4	&	1.5	&	9.4	&	9.4	&	9.4	&	$<$1?	&	$>$5	 \\
70	&	30	&	2.2	$\pm$	1.0	&	2.2	&	30.37	&	7 03 54.8	&	$-11$ 42 37	&	15.1	&	0.3	&	12.0	&	11.5	&	11.3	&	01--02	&	1.5--2.0	 \\
71$^x$	&	30	&	4.9	$\pm$	1.3	&	3.7	&	30.72	&	7 03 55.7	&	$-11$ 29 32	&	14.9	&	2.5	&	12.9	&	12.2	&	12.0	&	02--05	&	1.5--2.0	 \\
72$^{i,j}$	&	30	&	1.6	$\pm$	0.9	&	1.9	&	30.25	&	7 03 56.8	&	$-11$ 34 42	&	11.0	&	7.0	&	10.5	&	10.2	&	10.1	&	??	&	??	 \\
73$^{j,x}$	&	30	&	2.9	$\pm$	1.1	&	2.7	&	30.50	&	7 04 00.4	&	$-11$ 34 00	&	12.7	&	7.0	&	12.1	&	10.9	&	10.2	&	$<$1	&	2.0--3.0	 \\
74$^{*,k}$	&	30	&	9.2	$\pm$	1.8	&	5.3	&	31.00	&	7 04 01.4	&	$-11$ 23 35	&	12.6	&	2.5	&	11.5	&	10.8	&	10.3	&	02--05	&	2.0--3.0	 \\
75$^{k,l,x}$	&	30	&	6.4	$\pm$	1.5	&	4.3	&	30.84	&	7 04 02.3	&	$-11$ 25 39	&	10.8	&	1.3	&	10.4	&	10.3	&	10.3	&	1--2	&	3.0--5.0	 \\
76$^m$	&	30	&	3.8	$\pm$	1.3	&	3.0	&	30.61	&	7 04 06.6	&	$-11$ 18 35	&	10.9	&	6.0	&	13.1	&	12.2	&	11.6	&	02--05	&	2.0--3.0	 \\
77$^m$	&	30	&	3.0	$\pm$	1.1	&	2.7	&	30.51	&	7 04 09.2	&	$-11$ 30 08	&	14.2	&	0.8	&	13.7	&	13.0	&	12.9	&	01--02	&	1.0--1.5	 \\
78	&	30	&	2.2	$\pm$	1.2	&	1.9	&	30.38	&	7 04 11.3	&	$-11$ 16 48	&	13.4	&	3.5	&	12.0	&	11.4	&	11.1	&	05--10	&	2.0--3.0	 \\
79	&	30	&	4.1	$\pm$	1.3	&	3.2	&	30.64	&	7 04 12.1	&	$-11$ 21 10	&	13.8	&	2.9	&	14.4	&	13.4	&	13.1	&	??	&	??	 \\
80	&	30	&	2.1	$\pm$	1.0	&	2.1	&	30.36	&	7 04 12.3	&	$-11$ 39 23	&	12.0	&	1.2	&	11.3	&	11.0	&	11.0	&	05--10	&	2.0--3.0	 \\
81$^{m,n}$	&	30	&	3.2	$\pm$	1.2	&	2.7	&	30.54	&	7 04 13.2	&	$-11$ 19 01	&	7.8	&	3.5	&	10.9	&	10.6	&	10.5	&	01--02	&	3.0--5.0	 \\
82$^{o,x}$	&	30	&	3.8	$\pm$	1.2	&	3.0	&	30.61	&	7 04 15.9	&	$-11$ 24 06	&	9.4	&	1.4	&	9.0	&	8.9	&	8.9	&	$<$1?	&	$>$5	 \\
83$^p$	&	30	&	3.5	$\pm$	0.8	&	4.3	&	30.58	&	7 04 17.4	&	$-11$ 43 10	&	10.9	&	0.6	&	10.2	&	10.1	&	10.0	&	02--05	&	3.0--5.0	 \\
84$^x$	&	30	&	3.5	$\pm$	0.8	&	4.3	&	30.58	&	7 04 18.3	&	$-11$ 42 36	&	13.8	&	0.0	&	12.0	&	11.5	&	11.3	&	02--05	&	1.5--2.0	 \\
85	&	30	&	4.2	$\pm$	1.3	&	3.3	&	30.66	&	7 04 18.8	&	$-11$ 24 47	&	14.7	&	0.8	&	14.6	&	13.9	&	13.7	&	05--10	&	0.5--1.0	 \\
86$^x$	&	30	&	2.9	$\pm$	1.1	&	2.6	&	30.50	&	7 04 19.1	&	$-11$ 33 48	&	13.4	&	0.4	&	13.1	&	12.4	&	12.2	&	02--05	&	0.5--1.0	 \\
87	&	30	&	3.0	$\pm$	1.2	&	2.6	&	30.51	&	7 04 20.0	&	$-11$ 22 22	&	13.2	&	0.9	&	14.4	&	13.3	&	12.7	&	??	&	??	 \\
88	&	30	&	1.8	$\pm$	0.9	&	1.9	&	30.29	&	7 04 20.6	&	$-11$ 36 44	&	16.7	&	0.7	&	14.6	&	13.7	&	13.5	&	??	&	??	 \\
89$^x$	&	30	&	3.5	$\pm$	1.2	&	2.9	&	30.57	&	7 04 26.3	&	$-11$ 31 21	&	13.8	&	0.8	&	12.5	&	11.6	&	11.2	&	??	&	??	 \\
90	&	30	&	4.0	$\pm$	1.3	&	3.1	&	30.63	&	7 04 25.3	&	$-11$ 34 28	&	13.2	&	1.1	&	11.7	&	11.1	&	10.9	&	$<$1	&	1.5--2.0	 \\
91$^x$	&	30	&	5.2	$\pm$	1.7	&	3.1	&	30.75	&	7 04 29.8	&	$-11$ 47 21	&	12.1	&	0.0	&	11.2	&	10.5	&	10.3	&	??	&	??	 \\
92$^x$	&	30	&	2.3	$\pm$	1.1	&	2.2	&	30.39	&	7 04 31.0	&	$-11$ 32 42	&	14.0	&	0.8	&	13.9	&	13.1	&	12.9	&	01--02	&	0.1--0.5	 \\
93	&	30	&	2.8	$\pm$	1.1	&	2.4	&	30.47	&	7 04 37.0	&	$-11$ 30 59	&	14.0	&	0.0	&	14.0	&	13.8	&	13.7	&	??	&	??	 \\
94	&	30	&	1.6	$\pm$	1.0	&	1.5	&	30.23	&	7 04 48.4	&	$-11$ 15 07	&	15.7	&	0.4	&	14.8	&	14.4	&	14.1	&	$>$50	&	1.0--1.5	 \\
95	&	30	&	5.4	$\pm$	1.8	&	3.0	&	30.76	&	7 04 52.5	&	$-11$ 38 21	&	14.7	&	0.2	&	13.2	&	12.4	&	12.1	&	??	&	??	 \\
96$^x$	&	30	&	3.4	$\pm$	1.5	&	2.3	&	30.56	&	7 04 56.3	&	$-11$ 29 33	&	12.5	&	1.2	&	11.5	&	10.9	&	10.2	&	01--02	&	2.0--3.0	 \\
97	&	30	&	0.9	$\pm$	0.6	&	1.7	&	30.00	&	7 05 15.5	&	$-11$ 31 06	&	14.8	&	0.0	&	13.2	&	12.8	&	12.7	&	20--50	&	1.0--1.5	 \\
98	&	30	&	0.9	$\pm$	0.6	&	1.7	&	30.00	&	7 05 15.7	&	$-11$ 32 05	&	14.4	&	0.0	&	12.8	&	12.1	&	12.0	&	01--02	&	1.0--1.5	 \\
\hline
\end{tabular}}
\smallskip
Notes: Stars previously identified (Clari\'a 1974, indicated by ``C'' and Shevchenko et~al. \cite{Shevchenko1999}, indicated by ``SEI''):  (l) SEI~99;  (n) SEI~111; (o)~HD~53339 (B3), C84, SEI114; (p) HD~53396  (B9), SEI~112. Members of clusters: 	(k) BRC~27; (m) NGC~2327. Objects detected by \mbox{\it XMM-Newton} and/or {\it Chandra} are indicated by ``x'' (see list in Table~\ref{taba3}). 
\end{table}