% Version of 16.03.2001 
\documentstyle{l-aa} 
%\onecolumn 
\begin{document} 
% HI observations of nearby galaxies 
%  IV. More dwarf galaxies in the southern sky 
\tiny 
\onecolumn
%\scriptsize 
\begin{table} 
\caption{\bf{a.} \rm List of new dwarf galaxy candidates found in the 
SERC EJ zone}
\begin{tabular}{|rcclllllrcl|} \hline 
\multicolumn{1}{|r}{kksg}& 
\multicolumn{2}{c}{R.A. (1950.0) Dec.}& 
\multicolumn{1}{c}{$a$}& 
\multicolumn{1}{c}{$b$}& 
\multicolumn{1}{l}{Type}& 
\multicolumn{1}{c}{S.B.}& 
\multicolumn{1}{c}{B$_{t}$}& 
\multicolumn{1}{c}{Ref.(B)}& 
\multicolumn{1}{c}{A$_{b}$}& 
\multicolumn{1}{c|}{Notes}  
\\ \hline  
\multicolumn{1}{|c}{ }&  
\multicolumn{1}{c}{ h m s }& 
\multicolumn{1}{c}{\ \ $\degr\ \ \ $\arcmin$ \ \ \ \arcsec$ }& 
\multicolumn{1}{c}{arc }& 
\multicolumn{1}{c}{min }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}& 
\multicolumn{1}{c}{2}&  
\multicolumn{1}{c}{3}&  
\multicolumn{1}{c}{4}&  
\multicolumn{1}{c}{5}&  
\multicolumn{1}{c}{6}&  
\multicolumn{1}{c}{7}&  
\multicolumn{1}{c}{8}&  
\multicolumn{1}{c}{9}&  
\multicolumn{1}{c}{10}&  
\multicolumn{1}{c|}{11} 
\\ \hline 
&&&&& &&&&& \\ 

  1&  00 23 38.5& $-$11 19 50& 5.0& 4.3& Sph& VL&&& 0.12& Cetus dw, LG member \\
  2&  00 37 44.6& $-$18 06 04& 0.9& 0.6& Sph/Ir& L&&& 0.08& \\
  3&  01 32 16.7& $-$07 36 38& 0.6& 0.4& Ir &L& 17.4&IK&0.14&  NGC 615
  5' NE \\
  4&  02 39 19.2& $-$08 36 54& 1.2& 1.1& Sph & L&&& 0.10&  in NGC 1052 gr.? \\
  5&  02 47 03.0& $-$13 25 06& 1.0& 0.5& Ir & L &&& 0.12&  \\
&&&&& &&&&& \\    
  6&  04 27 59.2& $-$14 18 56& 0.9& 0.4& Ir & L& 17.7&IK& 0.64&  \\
  7&  05 57 02.8& $-$13 05 28& 0.8& 0.2& Ir & L& 17.7&IK& 2.20& \\
  8&  06 42 15.2& $-$17 52 51& 1.8& 0.3& Ir & H& 15.13&NED& 1.79& \\
  9&  06 44 44.3& $-$17 53 10& 0.5& 0.35& Epec& H& 17.2&IK& 1.91&NGC2283
  22'S\\
 10&  07 10 28.9& $-$07 44 12& 1.0& 0.25& Ir& L& 18.5&IK& 3.38& \\
&&&&& &&&&& \\  
 11&  07 28 41.0& $-$00 52 04& 0.7& 0.4& Ir & L&&&0.47&  \\
 12&  08 51 05.8& $-$17 47 42& 0.5& 0.4& Ir & L& 17.4&IK& 0.80& \\
 13&  09 33 05.4& $-$16 06 34& 1.2& 0.2& Ir & VL& 18.2&IK& 0.24& \\
 14&  09 37 55.0& $-$03 39 30& 1.1& 1.0& Ir & L& 16.6&IK& 0.23& \\
 15&  09 52 40.9& $-$06 02 00& 1.3& 0.3& Ir?& H& 15.14&NED& 0.18& comp.
 N 3115 ? \\  
&&&&& &&&&& \\  
 16&  09 57 18.2& $-$09 06 39& 0.9& 0.7& Ir?& VL&&&0.31&  comp. N 3115 ? \\
 17&  09 59 09.4& $-$08 00 27& 1.4& 0.25& Ir& H& 15.5&NED& 0.26&
 comp. N 3115 ? \\  
 18&  10 03 12.3& $-$07 44 16& 1.7& 1.4& S0pec & H& 13.84&NED& 0.23& \\
 19&  10 22 00.5& $-$12 10 43& 0.7& 0.6& Ir& L& 17.9&IK& 0.30& \\
 20&  11 02 06.3& $+$00 19 40& 0.4& 0.4& Ir/Sph& L&&&0.16&  comp. N 3521?\\
&&&&& &&&&& \\   
 21&  11 03 01.7& $-$01 35 36& 1.7& 0.8& Ir & L& 17.3&IK& 0.24&
 UGC6145, comp. N3521? \\
 22&  11 03 34.5& $-$01 10 36& 0.5& 0.4& Ir?& L&&&0.20&  comp. N 3521 ?\\
 23&  11 03 42.2& $-$14 08 04& 3.5& 1.2& Ir & L& 15.8&IK& 0.23&  \\
 24&  11 11 20.3& $-$03 15 31& 0.5& 0.4& Ir & L& 17.4&IK& 0.25& \\
 25&  11 42 45.5& $-$16 59 46& 1.2& 0.7& Ir & VL& 18.2&IK& 0.17& \\
&&&&& &&&&& \\  
 26&  11 51 18.3& $-$14 44 51& 1.8& 1.1& Ir& VL& 17.8&IK& 0.17& \\
 27&  12 19 30.9& $-$09 31 23& 0.8& 0.3& Ir& L& 17.7&IK& 0.19& \\
 28&  12 21 22.0& $-$14 40 34& 1.2& 1.0& Ir& EL& 18.6&IK& 0.25& \\
 29&  12 34 38.4& $-$10 13 21& 1.4& 0.6& Ir& L&&&0.12&  comp. N 4594? \\
 30&  12 35 00.5& $-$08 35 32& 1.0& 0.5& Ir& L& 17.3&IK& 0.14& comp. N 4594?\\
&&&&& &&&&& \\   
 31&  12 35 58.0& $-$10 12 56& 0.8& 0.7& Sph& VL&&&0.13&comp. N 4594 ?\\
 32&  12 37 18.3& $-$11 28 35& 0.6& 0.5& Sph& EL&&&0.21&  comp. N 4594 ?\\
 33&  12 37 32.7& $-$12 05 25& 0.4& 0.4& Sph& VL&&&0.20&  comp. N 4594 ?\\
 34&  12 38 42.7& $-$11 39 12& 0.8& 0.7& Sph& VL&&&0.23&  comp. N 4594 ?\\
 35&  12 39 58.6& $-$14 40 02& 0.4& 0.4& Ir & EL&&&0.22& \\
&&&&& &&&&& \\  
 36&  12 44 02.8& $-$03 48 10& 0.9& 0.65& Ir& L& 17.4&IK& 0.10& \\
 37&  12 45 24.2& $-$12 23 00& 0.6& 0.5& Sph?& VL& 18.7&IK& 0.22& \\
 38&  12 50 56.6& $-$05 39 25& 1.2& 0.5& Ir & L& 17.0&IK& 0.15& \\
 39&  12 51 06.5& $-$05 48 46& 0.8& 0.6& Sph& EL& 18.5&IK& 0.17& \\
 40&  12 57 15.7& $-$13 51 04& 1.0& 0.6& Ir & VL&&&0.20& \\
&&&&& &&&&& \\  
 41&  13 03 07.6& $-$07 29 29& 1.4& 1.1& Ir & L &&&0.20&  comp. N 4948?\\
 42&  13 03 42.7& $-$07 49 31& 1.2& 0.9& Ir & VL&&&0.20& comp. N 4948 ?\\
 43&  13 06 39.6& $-$17 05 55& 0.7& 0.5& Ir?& EL&&&0.31& \\
 44&  13 30 23.5& $-$12 00 20& 0.5& 0.3& Ir & L &&&0.26& \\
 45&  14 11 06.0& $-$01 57 12& 0.6& 0.4& Sph?& L&17.5&IK& 0.29& \\
&&&&& &&&&& \\ 
\hline 
\end{tabular} 
\end{table} 
\begin{table}
\begin{tabular}{|rcclllllrcl|} \hline 
\multicolumn{1}{|r}{kksg}& 
\multicolumn{2}{c}{R.A. (1950.0) Dec.}& 
\multicolumn{1}{c}{$a$}& 
\multicolumn{1}{c}{$b$}& 
\multicolumn{1}{l}{Type}& 
\multicolumn{1}{c}{S.B.}& 
\multicolumn{1}{c}{B$_{t}$}& 
\multicolumn{1}{c}{Ref.(B)}& 
\multicolumn{1}{c}{A$_{b}$}& 
\multicolumn{1}{c|}{Notes}  
\\ \hline  
\multicolumn{1}{|c}{ }&  
\multicolumn{1}{c}{ h m s }& 
\multicolumn{1}{c}{\ \ $\degr\ \ \ $\arcmin$ \ \ \ \arcsec$ }& 
\multicolumn{1}{c}{arc }& 
\multicolumn{1}{c}{min }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}& 
\multicolumn{1}{c}{2}&  
\multicolumn{1}{c}{3}&  
\multicolumn{1}{c}{4}&  
\multicolumn{1}{c}{5}&  
\multicolumn{1}{c}{6}&  
\multicolumn{1}{c}{7}&  
\multicolumn{1}{c}{8}&  
\multicolumn{1}{c}{9}&  
\multicolumn{1}{c}{10}&  
\multicolumn{1}{c|}{11} 
\\ \hline 
&&&&& &&&&& \\ 
 46&  14 25 47.0& $-$08 41 55& 0.5& 0.5& Ir& L&&&0.25& \\
 47&  14 32 38.5& $-$16 56 43& 1.8& 0.9& Ir& L& 17.7&IK& 0.33& \\
 48&  16 03 02.4& $-$04 26 16& 1.3& 1.0& Ir& L& 18.2&IK& 1.19& \\
 49&  16 40 45.7& $-$07 58 00& 1.1& 0.4& Ir& L&&&1.72& \\
 50&  17 39 00.1& $-$04 35 59& 1.3& 0.5& Ir& L&&&3.08& \\
&&&&& &&&&& \\  
 
 51&  02 31 28.0& $-$06 34 44& 0.8& 0.4& Ir    & L& 15.4&IK&0.11& \\
 52&  02 46 50.9& $-$02 51 43& 0.9& 0.5& Ir/SB & L& 16.9&IK&0.22& \\
 53&  04 06 39.3& $-$08 45 28& 1.0& 0.6& Ir/S  & L& 17.3&IK&0.23& \\
 54&  05 39 36.7& $-$12 35 09& 1.0& 0.4& Ir/Sm & L& 15.4&IK&0.73& \\
 55&  05 47 55.8& $-$10 18 45& 2.0& 0.9& SB/Ir & L& 17.4&IK&3.57& \\
&&&&& &&&&& \\  
 56&  05 49 44.0& $-$11 09 05& 0.9& 0.8& Sph/Ir& VL& 15.5&NED&2.90&
 pair w.No55\\
 57&  08 41 04.4& $-$17 12 15& 1.8& 0.5& Ir& L& 16.1&IK&0.32& \\
 58&  10 50 29.1& $+$02 45 33& 1.5& 0.5& Ir& L& 17.4&NED&0.16&CGCG08-043
 at 8.8' \\   
 59&  11 10 13.9& $-$00 17 39& 0.5& 0.4& Ir& L& 17.8&NED&0.17& \\
 60&  12 20 35.1& $-$13 40 05& 1.4& 0.9& Ir& L& 16.2&IK&0.21& \\
&&&&& &&&&& \\  
 61&  12 42 18.7& $-$08 51 15& 4.0& 1.8& Sm& L& 15.1&IK&0.16& UGCA295 \\
 62&  12 56 29.6& $-$11 57 31& 1.2& 0.8& Ir& L& 16.6&IK&0.18& \\
 63&  13 23 43.5& $+$02 43 06& 0.8& 0.4& Ir& L& 16.8&NED&0.10& \\
 64&  13 25 39.4& $+$02 32 20& 0.8& 0.45& Ir& L& 16.3&NED&0.12& \\
 65&  14 11 47.0& $-$02 47 59& 0.8& 0.25& Ir& L& 15.8&NED&0.30& \\
&&&&& &&&&& \\   
 66&  14 31 20.7& $+$01 42 14& 1.0& 0.2& Ir& L& 17.4&NED&0.20& \\
 67&  20 06 41.4& $-$06 26 05& 2.2& 1.4& S& L& 15.3&IK&0.34& \\
\hline 

\end{tabular} 
\end{table} 
%\end{document} 
\addtocounter{table}{-1} 

 % Version of 18.04.2001
% \documentstyle{aa}
 %\onecolumn
% \begin{document}
 % HI observations of nearby galaxies
 %  IV. More dwarf galaxies in the southern sky
 \tiny
 \onecolumn
 %\scriptsize
 \begin{table}
 \caption{\bf{b.} \rm List of new dwarf galaxy candidates found in the 
 southern sky}
 \begin{tabular}{|rcclllllrcl|} \hline
 \multicolumn{1}{|r}{kks}&
 \multicolumn{2}{c}{R.A. (1950.0) Dec.}&
 \multicolumn{1}{c}{$a$}&
 \multicolumn{1}{c}{$b$}&
 \multicolumn{1}{l}{Type}&
 \multicolumn{1}{c}{S.B.}&
 \multicolumn{1}{c}{B$_{t}$}&
 \multicolumn{1}{c}{Ref.(B)}&
 \multicolumn{1}{c}{A$_{b}$}&
 \multicolumn{1}{c|}{Notes}
 \\ \hline
 \multicolumn{1}{|c}{ }&
 \multicolumn{1}{c}{ h m s }&
 \multicolumn{1}{c}{\ \ $\degr\ \ \ $\arcmin$ \ \ \ \arcsec$ }&
 \multicolumn{1}{c}{arc }&
 \multicolumn{1}{c}{min }&
 \multicolumn{1}{c}{ }&
 \multicolumn{1}{c}{ }&
 \multicolumn{1}{c}{ }&
\multicolumn{1}{c}{ }&
\multicolumn{1}{c}{ }&
\multicolumn{1}{c|}{ }
\\ \hline
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c}{10}&
\multicolumn{1}{c|}{11}
\\ \hline
&&&&& &&&&& \\
%	       List of 81 southern dwarf galaxy candidates
%		  found in AIP/SAO (1999) and SAO (2000)
%============================================================================
% #     R.A. (1950) Dec    (a x b)_b  Type  SB    B_t    NED       Notes
%			  (a x b)_r              A_b  identif.
%----------------------------------------------------------------------------
% (1)    (2)       (3)       (4)  (5)   (6)  (7)        (8)
%----------------------------------------------------------------------------
 1&  02 12 45.1&$-$32 26 31& 0.80& 0.70& Ir&   LV&18.0:&IK&0.09&  \\
 2&  02 23 38.7&$-$19 55 07& 1.30& 0.60& Ir& L& 16.23&NED&0.14& \\
 3&  02 24 23.1&$-$73 44 16& 2.50& 1.00& Sph?& VL&16.0:&IK&0.22& \\
 4&  03 12 06.1&$-$66 27 22& 2.0:& 1.0:& Ir& EL&17.8: &IK&0.14&   comp. to NGC 1313\\
 5& 03 12 12.4 &$-$38 10 42& 1.20& 0.70& Sph& L& 17.18&NED&0.07& \\
&&&&& &&&&& \\  
 6&  03 13 47.5&$-$66 34 32& 3.2:& 1.4:& Ir& EL&17.0: &IK&0.24&  comp. to NGC 1313\\
 7&  03 15 28.0&$-$25 05 30& 1.20& 0.60& Ir& L&17.2&IK& 0.05&  \\
 8&  03 19 37.2&$-$42 10 40& 1.10& 0.90& Ir& L& 16.37&NED&0.05& \\
 9&  03 33 36.1&$-$51 37 11& 1.3:& 1.0:& Ir& VL& 16.24&NED&0.06& \\
10&  03 37 33.1&$-$31 57 12& 1.20& 0.70& Ir& L& 16.9&IK&0.04& \\
&&&&& &&&&& \\ 
11&  03 40 08.9&$-$22 54 54& 1.90& 1.40& S& VL& 14.92&NED&0.08&  projected on E482-36\\
12&  03 41 49.2&$-$25 04 48& 1.0:& 0.7:& Ir& L& 17.49&NED&0.06& \\
13&  03 47 12.8&$-$48 34 18& 1.10& 0.80& Ir& L& 16.39&NED&0.04& \\
14&  05 26 23.6&$-$63 36 16& 0.70& 0.55& Ir& EL&17.8 &IK&0.22&   near NGC 1947\\
15&  05 26 45.5&$-$63 16 41& 1.70& 0.80& Ir?& VL& 16.81&NED&0.24& near NGC 1947\\
&&&&& &&&&& \\ 
16&  05 30 10.8&$-$17 43 54& 0.70& 0.40& Ir&  L&17.8&IK& 0.32&  \\
17&  05 32 13.0&$-$61 57 49& 0.95& 0.65& Ir& VL&17.4 &IK&0.26&  \\
18&  06 03 55.2&$-$33 04 33& 3.5:& 2.5:& Ir?& L& 13.58&NED&0.19& \\
19&  06 15 06.3&$-$57 42 27& 1.40& 1.00& Ir& L& 15.85&NED&0.17&ESO\,121-G020 \\
20&  07 01 21.5&$-$44 59 30& 1.10& 0.50& Ir& L& 16.19&NED&0.41& \\
&&&&& &&&&& \\ 
21&  07 14 52.7&$-$40 00 21& 1.30& 0.40& Ir& L& 16.32&NED&1.17& \\
22&  07 31 04.6&$-$35 22 50& 1.20& 0.80& Ir& VL& 16.7&IK&1.94&  \\
23&  07 42 13.9&$-$45 01 45& 0.90& 0.90& Sph?& EL& 17.5&IK&1.49& \\
24&  07 50 14.8&$-$55 19 22& 1.10& 0.90& Ir&L&17.3&IK&0.89&  \\
25&  07 54 33.4&$-$26 07 03& 0.50& 0.40& Ir& VL&17.7&IK&1.45& \\
&&&&& &&&&& \\  
26&  07 55 43.5&$-$26 44 00& 0.80& 0.35& Ir& VL&18.0&IK&2.67&  \\
27&  08 44 39.8&$-$21 36 43& 0.80& 0.60& Ir& L&17.4&IK& 0.74&  \\
28&  08 52 39.5&$-$32 37 34& 1.20& 0.50& Ir& VL& 17.42&NED&1.36& \\
29&  09 08 51.2&$-$63 41 27& 0.75& 0.45& Ir&   VL&17.5&IK&0.89&  \\
30&  09 20 51.7&$-$19 57 10& 0.60& 0.40& Im& H& 15.53&NED&0.27& \\
&&&&& &&&&& \\  
31&  09 30 38.2&$-$33 01 20& 1.3:& 0.7:& Ir& L& 16.4&IK&0.58& \\
32&  09 32 24.3&$-$74 01 55& 0.80& 0.60& Ir& VL& 16.69&NED&0.48& \\
33&  09 53 30.2&$-$67 50 06& 0.70& 0.50& Sph?& L&17.2&IK&0.80& \\
34&  10 03 11.4&$-$31 47 17& 0.80& 0.40& Ir& L& 17.5&IK&0.45& \\
35&  10 05 32.0&$-$64 07 16& 1.00& 0.90& Ir?& VL& 14.3&NED&0.93& \\
&&&&& &&&&& \\  
36&  10 28 25.0&$-$46 00 51& 1.60& 1.20& Sph?& L& 14.86&NED&0.77& \\
37&  10 29 18.9&$-$21 59 33& 1.20& 0.60& Ir& L& 16.44&NED&0.28& \\
38&  10 43 38.3&$-$44 25 04& 0.80& 0.40& Ir&    L&16.8&IK&0.77&  \\
39&  10 53 00.6&$-$47 26 12& 1.10& 0.80& Ir&   VL&17.5&IK&0.93&  \\
40&  10 55 16.8&$-$47 54 40& 2.00& 1.20& Ir?& VL& 16.03&NED&0.95& \\
&&&&& &&&&& \\ 
41&  11 17 39.2&$-$68 48 49& 0.90& 0.60& Ir& VL& 18.0&IK&1.20& \\
42&  11 24 11.0&$-$72 20 19& 1.00& 0.60& Ir?& VL&17.8&IK&1.46& \\
43&  11 32 51.7&$-$41 16 14& 0.70& 0.50& Ir?& VL&17.9 &IK&0.35& \\
44&  11 35 25.2&$-$38 56 37& 1.40& 0.90& Ir& H& 15.85&NED&0.61& \\
45&  11 37 59.9&$-$46 55 44& 0.60& 0.50& Ir &  VL&18.2&IK&0.71&  \\
&&&&& &&&&& \\ 
\hline

\end{tabular}
\end{table}
%\end{document}

 \begin{table}
 %\caption{List of new dwarf galaxy candidates found in the southern sky}
 \begin{tabular}{|rcclllllrcl|} \hline
 \multicolumn{1}{|r}{kks}&
 \multicolumn{2}{c}{R.A. (1950.0) Dec.}&
 \multicolumn{1}{c}{$a$}&
 \multicolumn{1}{c}{$b$}&
 \multicolumn{1}{l}{Type}&
 \multicolumn{1}{c}{S.B.}&
 \multicolumn{1}{c}{B$_{t}$}&
 \multicolumn{1}{c}{Ref.(B)}&
 \multicolumn{1}{c}{A$_{b}$}&
 \multicolumn{1}{c|}{Notes}
 \\ \hline
 \multicolumn{1}{|c}{ }&
 \multicolumn{1}{c}{ h m s }&
 \multicolumn{1}{c}{\ \ $\degr\ \ \ $\arcmin$ \ \ \ \arcsec$ }&
 \multicolumn{1}{c}{arc }&
 \multicolumn{1}{c}{min }&
 \multicolumn{1}{c}{ }&
 \multicolumn{1}{c}{ }&
 \multicolumn{1}{c}{ }&
\multicolumn{1}{c}{ }&
\multicolumn{1}{c}{ }&
\multicolumn{1}{c|}{ }
\\ \hline
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c}{10}&
\multicolumn{1}{c|}{11}
\\ \hline
&&&&& &&&&& \\ 
46&  11 40 02.3&$-$25 38 08& 0.80& 0.70& Ir& L& 16.60&NED&0.20& \\
47&  11 54 57.6&$-$27 50 45& 1.30& 1.10& Ir/Sph& VL&17.5&IK&0.32&conf. E440-35  \\
48&  12 03 01.0&$-$43 29 30& 1.30& 0.90& Ir& L& 17.20&NED&0.53& \\
49&  12 05 02.6&$-$30 54 58& 0.80& 0.60& Ir/Sph& L& 17.25&NED&0.28& \\
50&  12 06 55.1&$-$30 05 07& 0.60& 0.45& Sph?& L&18.0&IK&0.25& \\
&&&&& &&&&& \\
51&  12 41 36.2&$-$42 39 58& 0.90& 0.40& E/Sph& L&16.7 &IK&0.38& \\
52&  12 55 13.5&$-$45 32 31& 1.60& 1.10& Ir/Sm&  VL&16.4&IK&0.38& \\
53&  13 08 24.3&$-$38 38 26& 0.80& 0.70& Sph& VL&17.3 &IK&0.38& \\
54&  13 18 44.5&$-$31 37 29& 1.10& 0.75& Ir?& EL&17.6 &IK&0.29& \\
55&  13 19 17.8&$-$42 28 00& 0.80& 0.70& Sph& EL&18.5 &IK&0.63& Centaurus. gr. \\
&&&&& &&&&& \\ 
56&  13 32 56.1&$-$56 16 46& 1.10& 0.95& Ir?& L& 16.7&IK&3.02& \\
57&  13 38 38.5&$-$42 19 47& 0.80& 0.70& Sph& EL&18.1 &IK&0.39& Centaurus gr.? \\
58&  13 43 05.7&$-$36 04 41& 1.00& 0.70& Sph?& VL&17.1 &IK&0.27& \\
59&  13 44 43.9&$-$53 06 08& 3.00& 1.30& Ir& L& 14.2&NED&2.13& \\
60&  13 50 42.2&$-$61 59 18& 1.70& 1.20& RN? &   L&17.1&IK&77.92&  \\
&&&&& &&&&& \\ 
61&  15 05 56.6&$-$67 45 15& 1.50& 0.60& Ir& L&18.0 &IK&0.79& \\
62&  15 40 49.7&$-$27 55 07& 1.00& 0.50& Ir  &   L&18.1&IK&0.90&  \\
63&  15 56 42.3&$-$31 08 45& 2.5:& 1.5:& Ir?& EL&16.0 &IK&0.94& \\
64&  16 06 01.7&$-$65 37 14& 0.90& 0.75& Ir?& L& 16.9&IK&0.56& \\
65&  16 44 08.9&$-$27 05 17& 0.80& 0.60& S?& L&17.5 &IK&1.24&  \\
&&&&& &&&&& \\  
66&  16 49 29.1&$-$59 00 29& 1.50& 0.70& Ir& VL&16.7 &IK&0.58& comp. to NGC 6221?\\
67&  17 00 38.2&$-$18 48 14& 0.70& 0.70& Ir  &  VL&17.7&IK&1.40&  \\
68&  18 18 05.8&$-$62 17 42& 1.00& 0.55& Ir& L& 16.59&NED&0.34& \\
69&  18 46 22.8&$-$64 04 02& 0.40& 0.30& Ir& L& 18.09&NED&0.37& comp. to NGC 6744?\\
70&  19 02 12.3&$-$64 02 28& 0.55& 0.50& Ir?& L&17.7 &IK&0.20& comp. to NGC 6744?\\
&&&&& &&&&& \\  
71&  19 04 00.6&$-$63 48 41& 2.70& 0.70& Ir& L& 15.10&NED&0.19& comp. to NGC 6744\\
72&  19 07 40.0&$-$63 56 21& 0.60& 0.45& Ir& VL&17.9 &IK&0.17& comp. to NGC 6744?\\
73&  19 17 20.4&$-$60 46 41& 1.20& 1.00& Ir  &   L&16.9&IK&0.23&  \\
74&  19 23 16.9&$-$61 06 43& 0.90& 0.45& Ir  &  VL&17.6&IK&0.34&  \\
75&  20 17 21.2&$-$22 03 48& 0.50& 0.45& Ir& L& 18.2&IK&0.34& \\
&&&&& &&&&& \\  
76&  20 39 57.8&$-$61 26 52& 0.80& 0.70& Ir& L& 17.11&NED&0.23& \\
77&  20 49 44.9&$-$39 06 43& 0.80& 0.30& Ir& L&17.8 &IK&0.24& \\
78&  21 50 30.9&$-$26 48 54& 1.10& 0.50& Ir& L& 16.25&NED&0.15& \\
79&  22 04 02.0&$-$46 39 31& 0.9:& 0.7:& Sph?& L&17.5 &IK&0.06&   \\
80&  22 12 51.8&$-$59 46 48& 0.90& 0.70& Ir& L&17.4 &IK&0.11&  \\
81&  22 44 29.4&$-$19 06 33& 1.10& 0.60& Ir& L& 16.47&NED&0.14& \\
&&&&& &&&&& \\ 
\hline

\end{tabular}
\end{table}
%\end{document}

\addtocounter{table}{-1} 

% Version of 16.03.2001 
%\documentstyle{aa} 
%\onecolumn 
%\begin{document} 
% HI observations of nearby galaxies 
%  IV. More dwarf galaxies in the southern sky 
\tiny 
\onecolumn
%\scriptsize 
\begin{table} 
\caption{\bf{c.} \rm List of new dwarf galaxy candidates from the kk list}
\begin{tabular}{|rcclllllrcl|} \hline 
\multicolumn{1}{|r}{kk}& 
\multicolumn{2}{c}{R.A. (1950.0) Dec.}& 
\multicolumn{1}{c}{$a$}& 
\multicolumn{1}{c}{$b$}& 
\multicolumn{1}{l}{Type}& 
\multicolumn{1}{c}{S.B.}& 
\multicolumn{1}{c}{B$_{t}$}& 
\multicolumn{1}{c}{Ref.(B)}& 
\multicolumn{1}{c}{A$_{b}$}& 
\multicolumn{1}{c|}{Notes}  
\\ \hline  
\multicolumn{1}{|c}{ }&  
\multicolumn{1}{c}{ h m s }& 
\multicolumn{1}{c}{\ \ $\degr\ \ \ $\arcmin$ \ \ \ \arcsec$ }& 
\multicolumn{1}{c}{arc }& 
\multicolumn{1}{c}{min }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c}{ }& 
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}& 
\multicolumn{1}{c}{2}&  
\multicolumn{1}{c}{3}&  
\multicolumn{1}{c}{4}&  
\multicolumn{1}{c}{5}&  
\multicolumn{1}{c}{6}&  
\multicolumn{1}{c}{7}&  
\multicolumn{1}{c}{8}&  
\multicolumn{1}{c}{9}&  
\multicolumn{1}{c}{10}&  
\multicolumn{1}{c|}{11} 
\\ \hline 
&&&&& &&&&& \\ 

%  1&  00 23 38.5& $-$11 19 50& 5.0& 4.3& Sph& VL&&&& Cetus dw, LG member[1]\\ 
11& 01 06 03.4&$-$38 28 35& 0.9& 0.4& Im& H& &&& K3,AM0106-382  distant?\\
47& 05 27 49.0& $-$87 37 36& 1.0& 0.45& Im& L&17.78& NED& 0.652& AM
0528-873 \\  
63& 07 37 20.0&$-69$ 13 38& 1.5& 0.9& Sph& VL&&&& FG219,AM0737-691 \\  
87 & 10 12 37.6& $-$44 36 08& 1.2& 1.0& Sm?& H& 13.49&NED& 0.902& AM
1012-443 \\  
88 & 10 13 57.4& $-$39 44 23& 0.9& 0.5& Ir& VL& 16.7& IK& 0.592& AM
1013-394 \\ 
&&&&& &&&&& \\    
179&13 00 40.5&$-$46 19 07& 1.2:&0.9:&Sph& L&&&& FG367,AM1300-461 \\  
272& 13 03 33.1& $-$49 33 38& 1.6& 0.6&Ir &L & 17.83&NED& 0.822&ESO\,219-G027
\\ 
184&13 06 15.0&$-$50 44 46& 1.9& 0.4& Ir & H&&&& AM1305-501 distant? \\
189&13 09 53.2&$-$41 34 01& 1.0& 0.6& Sph?& VL&&&&  EL in R \\  
190&13 10 14.6&$-$44 37 28& 2.7& 1.7& Sph& L&&&& FG373,AM1310-443 \\  
&&&&& &&&&& \\  
197&13 19 06.8&$-$42 16 20& 1.5& 1.1& Sph& VL&&&&  near NGC5128 \\  
203&13 24 29.6&$-$45 05 36& 0.5& 0.5& Ir/Sph&L&&&& AM1324-450  \\  
211&13 39 03.4&$-$44 57 11& 1.2& 1.1& Sph?& L&&&& AM1339-445 \\  
213&13 40 34.6&$-$43 31 04& 0.6& 0.3& Sph?& VL&&&& EL in R \\  
214&13 40 44.0&$-$45 29 41& 0.75&0.4& Ir & L&&&& AM1340-453  
distant? \\ 
&&&&& &&&&&  \\ 
217&13 43 13.4&$-$45 26 06& 1.0& 0.9& Sph& L&&&& AM1343-452 \\  
221&13 45 40.5&$-$46 44 54& 1.5:&1.0:&Sph & EL&&&& near br.star \\  
222&13 46 04.9&$-$47 57 21& 0.5& 0.4& Ir/Sph&L&&&& AM1346-475 \\  
226& 13 53 01.2& $-$45 24 47& 1.1& 0.7& Ir& L& 15.73&NED& 0.311& \\
235&15 03 11.2&$-$39 42 36& 0.8& 0.6& Ir & L&&&& FG438 distant? \\  
&&&&& &&&&& \\ 
239& 15 25 33.2& $-$42 36 36& 1.9& 0.7& Ir& L& 15.06&NED& 0.621& FG444
\\  
244&19 09 20.3&$-$61 59 57& 0.45&0.45&Sph?& L&17.0:&IK&0.239& AM1909-615 \\  
248&20 22 46.0&$-$71 34 23& 0.8& 0.4& Ir & L&15.87&NED&0.208& FG499  distant? \\  
256& 22 09 04.6& $-$43 25 29& 0.6& 0.5&Im&L& 16.89&NED& 0.053& AM
2209-432 \\ 
260& 23 11 46.9& $-$43 52 39& 4.5& 1.8& Ir& VL& 15.0:& IK& 0.049& \\ 
\hline 

\end{tabular} 
\end{table} 
%\end{document} 
%-------------------------------------------------------------------------------


%\documentstyle{aa}
\onecolumn 
%\begin{document} 
\tiny  
%\scriptsize   
\begin{table*}
\caption{\bf{a.} \rm The HI line data for new dwarf galaxies found in 
the SERC EJ zone}
\begin{tabular}{|rcrrrrrcrl|}\\ \hline
\multicolumn{1}{|r}{kksg}&
\multicolumn{1}{c}{HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{$V_h$}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{$V_{LG}$}&
\multicolumn{1}{c}{$M_{Bt}^{0}$}&
\multicolumn{1}{c}{$M_{HI}/L_B$}&
\multicolumn{1}{c}{$M_{dyn}/L_B$}&
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No.}&
\multicolumn{1}{c}{Jy km s$^{-1}$}&
\multicolumn{1}{c}{mJy}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c|}{ }
\\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
 \\ \hline  
&&&&&& & & & \\
% 1  & 2.2& 98$\pm$7 &$-104\pm2$ & 25 28 29& & & & & local HI \\
 1& & $\pm$10& & & & & & & \\ 
 2  & & $\pm$6& & & & & & &   \\ 
 3  & 14.1& 61$\pm$11& 1841$\pm$3& 371 380 383 & 1922 & $-$14.78& 17.1:& 99.6:& 
 conf. by NGC615\\
 4  & & $\pm$4& & & & & & &   \\  
 5  & & $\pm$4& & & & & & &  \\
&&&&& &&&& \\  
6  & 1.2& 35$\pm$8& 2236$\pm$2& 44 \  55 \  62& 2135& $-$15.21& 1.21&1.6 & \\
 7  & 3.8& 72$\pm$7& 960$\pm$3 & 49 \  67 \  76& 790& $-$14.61& 0.91& 1.1&  \\ 
 8  & 12.5& 108$\pm$8& 785$\pm$2& 118 152 155&568 & $-$16.06& 0.41& 2.8&  \\
 9  & 25.9& 161$\pm$6& 696$\pm$1& 187 205 207& 477& $-$13.73& 5.13:& 13.8:& conf.  by NGC2283\\ 
10 & 3.9& 48$\pm$6& 2445$\pm$2& 93 143 154& 2245&$-$17.26 & 0.66& 1.2&  \\
&&&&& &&&& \\   
 11 & & $\pm$4& &  & &$-$ & & &  \\
 12 & 2.6& 44$\pm$7& 1830$\pm$3& 51 \  78 \  96& 1560&$-$14.99 & 1.72& 1.1& \\
 13 & 6.9& 36$\pm$6& 90$\pm$1& 18 \  25 \  27&$-$180 & & & & \\
 14 & 3.5& 75$\pm$7& 1454$\pm$2& 52 \  65 \  68& 1225&$-$14.70 & 1.87& 2.5&  \\
15 & 2.7& 52$\pm$5& 791$\pm$3& 54 \  76 \  77& 554& $-$14.38& 0.39& 1.9&  \\
&&&&& &&&& \\   
16 & & $\pm$5& & & & & & & \\
 17 & 1.5& 59$\pm$7&446$\pm$3 &35 \  51 \  54 & 202& $-$11.91& 0.28& 3.1&  \\ 
 18 & 0.6& 39$\pm$7& 134$\pm$3& 36 \  39 \  40& $-$108& & & &  \\
 19 & 3.5& 112$\pm$6 & 628$\pm$2 & 31 \  44 \  46& 373&$-$10.88 & 5.82& 5.7& \\
20 & & $\pm$6& & & & & & & \\
&&&&& &&&& \\  
21 & 2.8& 52$\pm$8& 744$\pm$2& 56 \  60 \  61& 537& $-$12.21& 2.83& 19.1& \\  
 22 & & $\pm$6& & & & & & & \\ 
 23 & 11.9& 157$\pm$5& 1041$\pm$1& 78 \  92 \  95& 790& $-$14.51& 3.05& 13.2& \\ 
 24 & 3.6& 38$\pm$7& 3833$\pm$2& 77 115 116& 3623&$-$16.27 & 3.96& 1.7&  \\
25 & 1.0& 48$\pm$5& 1226$\pm$2& 25 \  33 \  35& 982& $-$12.56&2.47 & 3.6&  \\
&&&&& &&&& \\  
26 & 1.5& 65$\pm$7& 1732$\pm$2& 20 \  34 \  37& 1499& $-$13.87& 2.56& 1.6& \\
27 & 2.2& 104$\pm$4& 1328$\pm$1& 20 \  28 \  30& 1128& $-$13.38& 3.37& 0.8& \\ 
 28 & 2.7& 67$\pm$7& 1416$\pm$3& 37 \  52 \  56& 1199&$-$12.67 & 8.96& 8.7& \\
 29 & & $\pm$0& & & & & & & \\ 
30 & 1.0& 36$\pm$6& 1105$\pm$2& 36 \  43 \  45 & 917& $-$13.28& 1.11& 3.0& \\ 
&&&&& &&&& \\  
31 & & $\pm$6& & & & & & & \\ 
 32 & & $\pm$9& & & & & & & \\ 
 33 & & $\pm$6& & & & & & & \\ 
 34 & & $\pm$8& & & & & & & \\
35 & & $\pm$6& & & & & & & \\ 
&&&&& &&&&  \\  
36 & 1.2& 37$\pm$5& 1275$\pm$2& 43 \  50 \  52& 1111& $-$13.55& 1.51& 3.6& \\
 37 & 1.3& 53$\pm$7& 84$\pm$2& 22 \  30 \  32& $-$110& & & & \\
 38 & 0.9& 35$\pm$7& 1071$\pm$4& 44 \  50 \  52& 905&$-$13.56 & 0.75& 4.1& \\
 39 & 1.1& 60$\pm$6& 1470$\pm$3& 16 \  31 \  37& 1303&$-$12.87 &3.58 & 1.0& \\
40 & & $\pm$8& & & & & & & \\
&&&&& &&&& \\  
41 & & $\pm$6& & & & & & &  \\  
 42 & & $\pm$9& & & & & & & \\
 43 & & $\pm$10& & & & & & & \\
 44 & & $\pm$6& & & & & & & \\
 45 & 0.8& 25$\pm$8& 1446$\pm$4& 40 \  55 \  56& 1357& $-$1408& 0.93& 1.6& \\
&&&&& &&&& \\ 
\hline 
\end{tabular}
\end{table*}

\begin{table*}

\begin{tabular}{|rcrrrrrcrl|}\\ \hline
\multicolumn{1}{|r}{kksg}&
\multicolumn{1}{c}{HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{$V_h$}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{$V_{LG}$}&
\multicolumn{1}{c}{$M_{BT}^{0}$}&
\multicolumn{1}{c}{$M_{HI}/L_B$}&
\multicolumn{1}{c}{$M_{dyn}/L_B$}&
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No.}&
\multicolumn{1}{c}{Jy km s$^{-1}$}&
\multicolumn{1}{c}{mJy}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
 \\ \hline  
&&&&& &&&& \\ 
46 & & $\pm$9& & & & & & & \\
 47 & 9.8& 114$\pm$13& 1574$\pm$2& 100 114 116& 1447& $-$14.06& 13.19& 31.9&\\ 
 48 & 6.5& 95$\pm$8& 1611$\pm$1& 82 \  87 \  89& 1615&$-$14.66 & 6.28& 10.0& \\ 
 49 & & $\pm$7& & & & & & & \\ 
 50 & & $\pm$9& & & & & & & \\
&&&&& &&&& \\  
51 & 3.0& 75$\pm$7& 1410$\pm$2& 33 \  64 \  66& 1446&$-$16.14 & 0.59& 0.2& \\
 52 & 12.6& 146$\pm$5& 1090$\pm$1& 88 \  101 104& 1127& $-$14.20& 8.98& 8.4& \\
 53 & 4.9& 86$\pm$8& 894$\pm$2& 63 \  71 \  79& 834& $-$13.16& 5.0& 9.3& \\ 
 54 & 3.2& 42$\pm$5& 2243$\pm$2& 85 135 136& 2088&$-$17.58 & 0.36& 0.7& \\
55 & 51.7& 386$\pm$8& 900$\pm$1 & 172 185 188& 746& $-$16.16& 2.67 & 7.8&
 \\ 
&&&&& &&&& \\  
56 & 5.1& 82$\pm$8& 906$\pm$3& 70 \  87 \  91& 748& $-$13.39& 0.08& 0.2& \\  
 57 & 9.1& 95$\pm$9& 2021$\pm$2& 85 142 144& 1754& $-$16.06& 2.83& 4.2&  \\
 58 & 6.6& 121$\pm$8& 1052$\pm$2& 77 \  88 \  91 & 859&$-$13.05 & 7.88:& 23.6:&conf. \\
 59 & 1.1 & 14$\pm$4& 8517$\pm$6 & 90 102 104& 8318& $-$17.59& 1.88& 1.6& \\
60 & 4.3& 66$\pm$6& 1156$\pm$3& 69 \  86 \  90& 942& $-$14.50& 1.62& 5.1& \\ 
&&&&& &&&& \\ 
61 & 12.9& 147$\pm$5& 1381$\pm$2& 106 118 121& 1197& $-$16.08& 1.85& 10.3& \\  
 62 & 18.2& 277$\pm$12& 1309$\pm$1& 62 \  99 108& 1124&$-$14.46 & 10.21& 4.4& \\
 63 & 2.0& 39$\pm$8& 1028$\pm$3& 51 \  67 \  72& 919& $-$13.74& 1.45& 3.1& \\ 
 64 & 3.2& 83$\pm$7& 1021$\pm$2& 37 \  52 \  54& 913&$-$14.25 & 1.44& 1.0& \\
65 & 4.6& 39$\pm$10& 1902$\pm$3& 60 150 162& 1811& $-$16.41& 1.11& 0.7& \\ 
&&&&& &&&& \\  
66 & 3.0& 45$\pm$6& 1832$\pm$3& 71 \  82 \  84& 1776& $-$14.67& 3.45& 6.2& \\ 
 67 & 22.1& 338$\pm$9& 1424$\pm$1& 77 \  87 \  90& 1594& $-$16.68& 3.23& 2.3& \\ 
&&&&& &&&& \\  
\hline 
\end{tabular}
\end{table*}

%\end{document}

\addtocounter{table}{-1} 

%\documentstyle{aa}
\onecolumn 
%\begin{document} 
\tiny  
%\scriptsize   
\begin{table*}
\caption{\bf{b.} \rm The HI line data for new dwarf galaxies in the southern sky}
\begin{tabular}{|rcrrrrrcrl|}\\ \hline
\multicolumn{1}{|r}{kks}&
\multicolumn{1}{c}{HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{$V_h$}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{$V_{LG}$}&
\multicolumn{1}{c}{$M_{BT}^{0}$}&
\multicolumn{1}{c}{$M_{HI}/L_B$}&
\multicolumn{1}{c}{$M_{dyn}/L_B$}&
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No.}&
\multicolumn{1}{c}{Jy km s$^{-1}$}&
\multicolumn{1}{c}{mJy}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
 \\ \hline  
&&&&&& & & & \\
 1& & $\pm$10& & & & & & & \\ 
 2  & 5.09& 92$\pm$6& 2286$\pm$2& 67 \  79 \  83& 2272& $-$16.32& 2.11& 2.0&100-m RT   \\ 
    & 3.9& 60& 2293& 65 \ \ \ \ \ \ \ \ \  &&&&&  \\  
 3  & & & &  &  & & & & \\
 4  & & $\pm$4& & & & & & &   \\  
 5  & & $\pm$4& & & & & & &  \\
&&&&& &&&& \\  
 6  & & & & & & & & & \\
 7  & 1.9& 68$\pm$8& 1949$\pm$2 & 33 \  45 \  48& 1871& $-$14.84& 2.09& 1.5&100-m RT  \\ 
   & 1.5& 40& 1945& 39 \ \ \ \ \ \ \ \ \ &&&&&  \\ 
 8  & & & & & & & & &  \\
 9  & 2.6& 68$\pm$6& 1031& 39 \ \ \ \ \ \ \ \ \ & 852& $-$14.09& 1.17& 2.0&  \\ 
 10 & & $\pm$6& & & & & & &  \\
&&&&& &&&& \\   
 11 & 3.6& 39$\pm$5& 1567$\pm$5&  122 133 136& 1476&$-$16.64 & 0.47& 4.8&100-m RT  \\
    & 2.6& 45      & 1538& 65 \ \ \ \ \ \ \ \ \ &&&&&  \\ 
 12 & 0.9& 31$\pm$6& 1381$\pm$3& 30 \  38 \  39& 1281&$-$13.73 & 1.28& 1.9&100-m RT \\
 13 & 1.6& 52$\pm$6& 1478$\pm$1& 26 \ \ \ \ \ \ \ \ \  & 1299&$-$14.85 & 0.84& 0.6& \\
 14 & & $\pm$7& & & & & & &  \\
 15 & 2.5& 54$\pm$5& 1164$\pm$3& 51 \ \ \ \ \ \ \ \ \  & 913& $-$13.85& 1.62& 6.0& \\
&&&&& &&&& \\   
 16 & 2.04& 52$\pm$5& 3421$\pm$2& 42 \  51 \  52& 3256& $-$15.71& 3.04& 1.1&100-m RT \\
 17 & & $\pm$7& & & & & & &  \\ 
 18 & 13.7& 222$\pm$7& 787$\pm$3& 65 \ \ \ \ \ \ \ \ \ & 554&$-$15.95 & 0.47& 1.8&  \\
 19 & 9.4& 146$\pm$6 & 575$\pm$2 & 63 \ \ \ \ \ \ \ \ \ & 307&$-$12.38 & 2.66& 9.8&  \\
 20 & 3.1& 79$\pm$6& 1071&52 \ \ \ \ \ \ \ \ \  & 790& $-$14.34& 0.96& 2.2& \\
&&&&& &&&& \\  
 21 & 9.7& 83$\pm$8& 1391$\pm$2& 132 \ \ \ \ \ \ \ \ \ & 1109& $-$15.70& 1.69& 6.8& \\  
 22 & 11.7& 20$\pm$6& 1394& 59 \ \ \ \ \ \ \ \ \ & 1112& $-$16.10& 1.42& 0.9& \\ 
 23 & 3.6& 61$\pm$5& 1052$\pm$1& 65 \ \ \ \ \ \ \ \ \ & 765& $-$14.01& 1.38& 3.7&  \\ 
 24 & 5.8& 124$\pm$7& 1119$\pm$2& 39 \ \ \ \ \ \ \ \ \ & 820&$-$13.78 & 3.22& 2.2&  \\
 25 & 0.7& 67$\pm$5& 241$\pm$2& 26 \  27 \  30& -34& & & &100-m RT  \\
&&&&& &&&& \\  
 26 & 4.4& 68$\pm$10& 967$\pm$2& 62 \  82 \  84& 690& $-$14.49& 0.90& 1.7&100-m RT \\
 27 & 4.4& 49$\pm$4& 4641$\pm$1& 92 \ \ \ \ \ \ \ \ \ & 4362& $-$17.16& 3.08& 2.1& \\ 
 28 & 3.2& 48$\pm$7& 1310$\pm$3& 79 \ \ \ \ \ \ \ \ \ & 1008&$-$14.59 & 1.28& 5.7& \\
 29 & & $\pm$0& & & & & & & \\ 
30 & 1.8& 54$\pm$9& 829$\pm$3& 31 \  51 \  53 & 549& $-$14.06& 0.35& 0.4&100-m RT \\ 
   & 1.6& 37&  827&  35 \ \ \ \ \ \ \ \ \ &&&&&  \\ 
&&&&& &&&& \\  
31 & 4.1& 63$\pm$6& 853& 65 \ \ \ \ \ \ \ \ \ & 547& $-$13.49& 1.32& 6.2& \\ 
 32 & & $\pm$9& & & & & & & \\ 
 33 & & $\pm$6& & & & & & & \\ 
 34 & 2.1& 74$\pm$8& 1974& 28 \ \ \ \ \ \ \ \ \ & 1670& $-$14.69& 2.10& 0.7&  \\
35 & & $\pm$6& & & & & & & \\ 
&&&&& &&&&  \\  
36 & & $\pm$5& & & & & & & \\
 37 & 2.5& 56$\pm$7& 990$\pm$3& 44 \  66 \  68& 709&$-$13.71 & 1.11& 2.8&100-m RT \\
    & 2.0& 48& 1006& 30 \ \ \ \ \ \ \ \ \ &&&&&  \\  
38 & & $\pm$7& & & & & & & \\
 39 & & $\pm$6& & & & & & & \\
40 & 72.2& 1270$\pm$8& 594& 51 \ \ \ \ \ \ \ \ \ & 286& $-$12.83& 11.77& 5.7& \\
&&&&& &&&& \\  
\hline 
\end{tabular}
\end{table*}

\begin{table*}

\begin{tabular}{|rcrrrrrcrl|}\\ \hline
\multicolumn{1}{|r}{kks}&
\multicolumn{1}{c}{HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{$V_h$}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{$V_{LG}$}&
\multicolumn{1}{c}{$M_B$}&
\multicolumn{1}{c}{$M_{HI}/L_B$}&
\multicolumn{1}{c}{$M/L_B$}&
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No.}&
\multicolumn{1}{c}{Jy km s$^{-1}$}&
\multicolumn{1}{c}{mJy}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
 \\ \hline  
41 & 6.1& 90$\pm$6& 1332& 65 \ \ \ \ \ \ \ \ \ & 1045& $-$13.92& 4.86& 5.5&  \\  
 42 & 10.9& 66$\pm$9& 2030& 23 \ \ \ \ \ \ \ \ \ & 1750& $-$15.50& 5.67& 0.3& \\
 43 & & $\pm$10& & & & & & & \\
 44 & 2.6& 81$\pm$6& 654& 20 \ \ \ \ \ \ \ \ \ & 362& $-$13.18& 0.49& 0.6& \\
 45 & & $\pm$8& & & & & & & \\
 &&&&&& & & & \\
 46 & & $\pm$9& & & & & & & \\
 47 & 1.8& 64$\pm$13& 2125$\pm$2& 18: \ \ \  \ \ \ \ \  & 1859& $-$14.79& 2.03:& 0.5:& conf. E440-35\\ 
 48 & 3.5& 45$\pm$8& 3018$\pm$1& 105: \ \ \ \ \ \ \ \ & 2732& $-$16.14& 2.46& 7.0& \\ 
 49 & & $\pm$7& & & & & & & \\ 
 50 & 5.2& 184$\pm$9& 150$\pm$1.5& 23 \  39 \  42& -115& & & &100-m RT \\
&&&&& &&&& \\  
 51 & & $\pm$7& & & & & & & \\
 52 & 3.9& 59$\pm$5& 2079$\pm$1& 63 \ \ \  \ \ \ \ \ \  & 1814& $-$15.90& 1.51& 2.6& \\
 53 & & $\pm$8& & & & & & & \\ 
 54 & & $\pm$5& & & & & & & \\
55 & & $\pm$8&  & & & &  & &
 \\ 
&&&&& &&&& \\  
56 & 11.6& 61$\pm$8& 4058$\pm$3& 194 \ \ \ \ \ \ \ \ \ & 3802& $-$19.85& 0.52& 0.9& \\  
 57 & & $\pm$9& & & & & & &  \\
 58 & & $\pm$8& &  & & & & & \\
 59 & 48.2 & 68$\pm$4& 694$\pm$6 & 59 \ \ \ \ \ \ \ \ \  & 446& $-$16.80& 0.49& 0.5& \\
60 & & $\pm$6& & & & & & & \\ 
&&&&& &&&& \\ 
61 & & $\pm$5& & & & & & & \\  
 62 & & $\pm$12& & & & & & & \\
 63 & & $\pm$8& & & & & & & \\ 
 64 & 5.8& 66$\pm$7& 3530$\pm$2& 112 \ \ \ \ \  \ \ \ \ & 3329&$-$16.90 & 3.02& 3.4& \\
65 & & $\pm$10& & & & & & & \\ 
&&&&& &&&& \\  
66 & 28.2& 1320$\pm$6& 1559$\pm$3& 218 \ \ \ \ \ \ \ \ \ & 1393& $-$15.30& 
11.21:& 38.8:&conf.
by NGC6221\\ 
 67 & & $\pm$9& & & & & & & \\ 
 68 & 4.6& 84& 951& 46 \ \ \ \ \ \ \ \ \ & 809& $-$13.92& 2.20& 2.4& \\ 
 69 & & & & & & & & & \\ 
 70 & & & & & & & & & conf. by NGC6744\\ 
 &&&&& &&&& \\ 
 71 & & & & & & & & &conf. by NGC6744 \\ 
 72 & & & & & & & & & conf. by NGC6744\\  
 73 & & & & & & & & & \\ 
 74 & & & & & & & & & \\ 
 75 & & & & & & & & & \\
 & & & & & &&&&  \\ 
 76 & & & & & & & & & \\ 
 77 & & & & & & & & & \\ 
 78 & 4.8& 77$\pm$9& 1772$\pm$1.5& 82 107 109& 1858& $-$15.87& 2.01& 3.2&100-m RT \\ 
    & 3.0& 39& 1751& 104: \ \ \ \ \ \ \ \ &&&&&  \\  
 79 & & & & & & & & & \\ 
 80 & & & & & & & & & \\ 
 81 & & & & & & & & & \\
&&&&& &&&& \\  
\hline 
\end{tabular}
\end{table*}

%\end{document}

\addtocounter{table}{-1} 

%\documentstyle{aa}
\onecolumn 
%\begin{document} 
\tiny  
%\scriptsize   
\begin{table*}
\caption{\bf{c.} \rm The HI line data for new dwarf galaxies from the kk list
(HIPASS data)}
\begin{tabular}{|rcrrrrrcrl|}\\ \hline
\multicolumn{1}{|r}{kk}&
\multicolumn{1}{c}{HI-flux}&
\multicolumn{1}{c}{S$_{max}$}&
\multicolumn{1}{c}{$V_h$}&
\multicolumn{1}{l}{line width}&
\multicolumn{1}{c}{$V_{LG}$}&
\multicolumn{1}{c}{$M_B$}&
\multicolumn{1}{c}{$M_{HI}/L_B$}&
\multicolumn{1}{c}{$M/L_B$}&
\multicolumn{1}{c|}{Comments}
\\ \hline   
\multicolumn{1}{|c}{No.}&
\multicolumn{1}{c}{Jy km s$^{-1}$}&
\multicolumn{1}{c}{mJy}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
\multicolumn{1}{c}{km s$^{-1}$}&
&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c}{$M_{\sun}/L_{\sun}$}&
\multicolumn{1}{c|}{ } 
\\ \hline 
\multicolumn{1}{|c}{1}&
\multicolumn{1}{c}{2}&
\multicolumn{1}{c}{3}&
\multicolumn{1}{c}{4}&
\multicolumn{1}{c}{5}&
\multicolumn{1}{c}{6}&
\multicolumn{1}{c}{7}&
\multicolumn{1}{c}{8}&
\multicolumn{1}{c}{9}&
\multicolumn{1}{c|}{10} 
 \\ \hline  
&&&&&& & & & \\
11 & & & & & & & & & \\ 
47 & 2.0& 48$\pm$7& 1774$\pm$8& 33 \ \ \ \ \ \ \ \ \  & 1538& $-$14.43& 2.15& 1.5& \\  
63 & & & & & & & & & \\  
87 & 5.9& 80$\pm$7& 1118$\pm$8& 65 \ \ \ \ \ \ \ \ \  & 804& $-$17.56& 0.10& 0.2& \\  
88 & 4.8& 75$\pm$7& 3004$\pm$8& 61 \ \ \ \ \ \ \ \ \  & 2692& $-$16.67& 2.02& 1.0& \\ 
&&&& &&&&& \\  
179& & & & & & & & & \\ 
272& 7.5& 90$\pm$7& 1281$\pm$8& 85 \ \ \ \ \ \ \ \ \  & 1017& $-$13.65& 7.23& 20.9& \\ 
184& & & & & & & & & \\ 
189& & & & & & & & & \\ 
190& & & & & & & & & \\ 
&&&&& &&&& \\  
197& & & & & & & & & \\ 
203& & & & & & & & & \\ 
211& & & & & & & & & \\ 
213& & & & & & & & & \\ 
214& & & & & & & & & \\  
&&&&& &&&& \\  
217& & & & & & & & & \\ 
221& & & & & & & & & \\  
222& & & & & & & & & \\ 
226& 4.6& 86$\pm$7& 2534$\pm$8& 60 \ \ \ \ \ \ \ \ \  & 2301& $-$17.02& 1.03& 0.7& \\ 
235& & & & & & & & & \\ 
&&&&& &&&& \\ 
239& 18.4& 152$\pm$7& 1331$\pm$8& 146 \ \ \ \ \ \ \ \ \   & 1164& $-$16.52& 1.66& 6.0& \\ 
244& 8.6& 138$\pm$ & 946$\pm$9& 66 \ \ \ \ \ \ \ \ \  & 821& $-$13.44& 6.60:& 
3.5:&confused by IC4831 \\ 
248& 3.8& 66$\pm$  & 4227$\pm$11& 53 \ \ \ \ \ \ \ \ \  & 4070& $-$18.01& 1.06& 0.3& \\ 
256& 2.4& 53$\pm$7& 2199$\pm$8& 40 \ \ \ \ \ \ \ \ \  & 2194& $-$15.49& 1.98& 0.7& \\ 
260& 4.4& 110$\pm$7& 1598$\pm$8& 40 \ \ \ \ \ \ \ \ \  & 1579& $-$16.67& 0.64& 1.3& \\
&&&&& &&&& \\  
\hline 
\end{tabular}
\end{table*}

\end{document}



