\documentstyle[longtable]{l-aa}
\begin{document}
\onecolumn
\setlength{\LTcapwidth}{0.9\textwidth}
\begin{longtable}[l]{rllrllllccc}
\caption*{\raggedright{\bf Table\,5a. New redshifts for Centaurus
cluster members.} Coordinates (1950.0) are given in columns 2 and 3,
column 4 gives the Centaurus Cluster Catalogue (Jerjen \& Dressler
1996a) reference number. The galaxy morphological type (5), the total blue
magnitude (6) and effective surface brightness (7) are taken from this
same source, while the probability of being Cen45 cluster member (8)
has been derived in Section\,5. Please note that if prob$_{45}$=0.00 this 
automatically implies that the galaxy is a 100\% Cen30 member. Column 11 
contains the heliocentric radial velocity (cz) and its estimated 
uncertainty, which results from a weighted average of columns 9 
(cross-correlation redshift) and column 10 (emission line redshift).}\\
\hline
\multicolumn{1}{c}{Seq} & 
\multicolumn{1}{c}{RA} & 
\multicolumn{1}{c}{Dec} & 
\multicolumn{1}{c}{CCC} & 
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{$B_{\rm T}$} & 
\multicolumn{1}{c}{{\it SB}$_{\rm eff}$}&
\multicolumn{1}{c}{prob$_{45}$}&
\multicolumn{1}{c}{V$_{\rm ccf}$} & 
\multicolumn{1}{c}{V$_{\rm emi}$} & 
\multicolumn{1}{c}{V}  \\
\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               
\endfirsthead

\caption*{(cont.)}\\
\hline                    
\multicolumn{1}{c}{Seq} & 
\multicolumn{1}{c}{RA} & 
\multicolumn{1}{c}{Dec} & 
\multicolumn{1}{c}{CCC} & 
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{$B_{\rm T}$} & 
\multicolumn{1}{c}{{\it SB}$_{\rm eff}$}&
\multicolumn{1}{c}{prob$_{45}$}&
\multicolumn{1}{c}{V$_{\rm ccf}$} & 
\multicolumn{1}{c}{V$_{\rm emi}$} & 
\multicolumn{1}{c}{V}  \\
\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                    
\endhead
  1&12~44~44.68&$-$41~22~39.0&  1&dE,N  &17.09&22.7&0.00 & 3527$\pm$59&         & 3527$\pm$59\\
  3&12~44~47.86&$-$40~51~33.0&  6&Im    &16.65&23.2&0.00 &         & 3848$\pm$50& 3848$\pm$50\\
  5&12~44~59.61&$-$40~52~59.0& 11&dS0:N &17.75&23.3&0.00 & 2750$\pm$43&         & 2750$\pm$43\\
  7&12~45~03.75&$-$40~43~33.9& 13&dS0,N &16.83&22.5&0.00 & 3026$\pm$29&         & 3026$\pm$29\\
 13&12~45~22.85&$-$41~35~26.0& 32&Im    &16.98&23.5&0.00 & 2737$\pm$28&         & 2737$\pm$28\\
 15&12~45~29.58&$-$41~26~36.0& 38&dE,N  &18.10&23.9&0.00 & 3925$\pm$45&         & 3925$\pm$45\\
 16&12~45~30.24&$-$41~02~35.0& 41&Im    &18.75&23.9&0.00 &         & 4278$\pm$58& 4278$\pm$58\\
 22&12~45~50.31&$-$41~10~02.9& 58&dE    &17.94&24.1&0.00 & 3304$\pm$60&         & 3304$\pm$60\\
 23&12~45~53.96&$-$40~59~44.0& 61&dE,N  &17.43&23.8&0.00 & 2910$\pm$67&         & 2910$\pm$67\\
 28&12~46~14.60&$-$40~42~02.0& 73&SBm   &16.90&23.6&0.88 &         & 4823$\pm$50& 4823$\pm$50\\
 30&12~46~16.08&$-$40~59~14.0& 75&dE,N  &18.06&23.2&0.00 & 1958$\pm$71&         & 1958$\pm$71\\
 34&12~46~23.88&$-$40~55~14.0& 84&dS0   &17.73&23.7&0.00 & 3122$\pm$29&         & 3122$\pm$29\\
 36&12~46~28.05&$-$41~27~32.9& 88&dE,N  &18.06&    &0.00 & 2848$\pm$26&         & 2848$\pm$26\\
 38&12~46~36.81&$-$40~58~58.0& 91&dE    &19.40&24.8&0.00 & 3652$\pm$61&         & 3652$\pm$61\\
 42&12~46~44.21&$-$41~08~55.0& 97&dE,N  &18.70&23.7&0.00 & 2818$\pm$30&         & 2818$\pm$30\\
 47&12~46~53.03&$-$41~32~14.0&109&Im    &19.48&24.8&0.00 & 3545$\pm$60&         & 3545$\pm$60\\
 48&12~46~54.00&$-$41~05~38.9&111&dE,N  &16.94&23.8&0.00 & 2880$\pm$40&         & 2880$\pm$40\\
 49&12~46~56.04&$-$40~57~23.9&113&E     &17.33&22.6&0.00 & 3715$\pm$26&         & 3715$\pm$26\\
 52&12~47~06.75&$-$40~34~29.0&120&dS0   &17.00&23.3&0.00 & 3106$\pm$28&         & 3106$\pm$28\\
 53&12~47~08.06&$-$41~04~03.0&121&Im    &18.36&24.3&0.88 & 4739$\pm$70&         & 4739$\pm$70\\
 55&12~47~10.02&$-$41~07~43.9&123&dS0   &18.45&24.0&0.82 & 4661$\pm$69&         & 4661$\pm$69\\
 56&12~47~10.38&$-$40~59~16.9&125&dE,N  &17.14&23.8&0.00 & 2880$\pm$35&         & 2880$\pm$35\\
 64&12~47~34.73&$-$41~23~31.0&146&dE    &17.77&23.7&0.00 & 2675$\pm$53&         & 2675$\pm$53\\
 65&12~47~37.96&$-$41~01~28.9&150&dE,N  &18.23&24.5&0.13 & 4426$\pm$46&         & 4426$\pm$46\\
 71&12~48~12.00&$-$41~06~26.0&172&dE,N  &18.21&24.6&0.86 & 4844$\pm$45&         & 4844$\pm$45\\
 72&12~48~12.65&$-$41~13~22.9&173&Im    &18.30&24.1&0.00 & 2139$\pm$36&         & 2139$\pm$36\\
 82&12~48~51.43&$-$40~53~59.0&193&Sc    &17.51&23.4&0.76 & 4924$\pm$56&         & 4924$\pm$56\\
 83&12~48~53.30&$-$41~12~39.0&196&Im    &18.10&24.3&0.83 &         & 4879$\pm$58& 4879$\pm$58\\
 88&12~49~06.16&$-$41~26~10.0&209&dE    &18.32&24.2&0.00 & 3535$\pm$76&         & 3535$\pm$76\\
 91&12~49~14.16&$-$40~52~15.0&212&Im    &19.06&    &0.00 & 2085$\pm$39&         & 2085$\pm$39\\
 94&12~49~15.44&$-$41~08~49.9&215&dE    &19.50&24.6&0.00 & 3329$\pm$76&         & 3329$\pm$76\\
 96&12~49~18.24&$-$40~38~05.9&219&Im    &17.10&23.5&0.00 &         & 3284$\pm$71& 3284$\pm$71\\
103&12~49~34.13&$-$41~28~48.0&228&dE,N  &18.09&24.1&0.00 & 3212$\pm$62&         & 3212$\pm$62\\
104&12~49~35.37&$-$40~53~47.0&230&Im    &17.94&24.4&0.83 &         & 4881$\pm$45& 4881$\pm$45\\
106&12~49~48.10&$-$40~57~16.0&239&Im    &18.00&24.4&0.64 &         & 4971$\pm$71& 4971$\pm$71\\
112&12~51~15.00&$-$41~07~31.0&277&Sc    &16.54&22.1&0.17 & 4441$\pm$73&         & 4441$\pm$73\\
\hline
\end{longtable}

\clearpage
% NEW REDSHIFTS FOR NON-MEMBERS

\begin{longtable}[l]{rllrllccc}
\caption*{\raggedright{\bf Table\,5b. New redshifts of background
galaxies.} Coordinates (1950.0) are given in columns 2 and 3,
column 4 gives the Centaurus Cluster Catalogue (Jerjen \& Dressler
1996a) reference number. The galaxy morphological type (5), the total blue
magnitude (6) and effective surface brightness (7) are taken from this
same source. Column 10 contains the
heliocentric radial velocity (cz) and its estimated uncertainty, which
results from a weighted average of columns 8 (cross-correlation
redshift) and column 9 (emission line redshift).}\\
\hline
\multicolumn{1}{c}{Seq} & 
\multicolumn{1}{c}{RA} & 
\multicolumn{1}{c}{Dec} & 
\multicolumn{1}{c}{CCC} & 
\multicolumn{1}{c}{$B_{\rm T}$} & 
\multicolumn{1}{c}{{\it SB}$_{\rm eff}$}&
\multicolumn{1}{c}{V$_{\rm ccf}$} & 
\multicolumn{1}{c}{V$_{\rm emi}$} & 
\multicolumn{1}{c}{V}  \\
\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)} \\
\hline          
\endfirsthead

 6&12~45~00.98&$-$40~56~44.0& 12&18.82&24.4&38469$\pm$66&         &38469$\pm$66\\
14&12~45~26.04&$-$40~16~07.9& 33&17.49&23.1&14702$\pm$81&14706$\pm$58&14705$\pm$47\\
18&12~45~36.96&$-$41~25~31.0& 44&19.76&24.3&         &21123$\pm$50&21123$\pm$50\\
21&12~45~49.10&$-$41~27~29.9& 56&18.90&24.8&13792$\pm$84&         &13792$\pm$84\\
29&12~46~15.02&$-$41~09~21.0& 74&18.76&23.7&16514$\pm$64&         &16514$\pm$64\\
39&12~46~38.54&$-$40~21~50.0& 92&17.70&23.5&         &10746$\pm$58&10746$\pm$58\\
57&12~47~14.58&$-$41~27~06.0&127&17.85&23.6&16362$\pm$45&         &16362$\pm$45\\
58&12~47~15.19&$-$41~10~30.0&128&19.28&24.2&46615$\pm$85&         &46615$\pm$85\\
63&12~47~31.28&$-$41~01~54.9&142&18.40&24.0&20843$\pm$56&         &20843$\pm$56\\
74&12~48~27.17&$-$40~32~34.9&179&17.27&22.6&14863$\pm$61&14878$\pm$58&14871$\pm$42\\
76&12~48~31.57&$-$41~00~13.0&182&18.01&23.3&         &10679$\pm$38&10679$\pm$38\\
77&12~48~41.55&$-$40~27~12.9&186&17.98&22.6&27387$\pm$91&27371$\pm$58&27376$\pm$49\\
92&12~49~14.18&$-$40~18~54.0&213&17.23&23.5&15916$\pm$44&         &15916$\pm$44\\
97&12~49~18.44&$-$41~22~21.0&220&17.93&23.1&         &19439$\pm$50&19439$\pm$50\\
\hline
\end{longtable}

\clearpage 
%OLD REDSHIFTS FOR CLUSTER MEMBERS

\begin{longtable}[l]{rllrllllccc}
\caption*{\raggedright{\bf Table\,5c. Reobserved redshifts for
Centaurus cluster members.} Coordinates (1950.0) are given in columns 2
and 3, column 4 gives the Centaurus Cluster Catalogue (Jerjen \&
Dressler 1996a) reference number. The galaxy morphological type (5),
the total blue magnitude (6) and effective surface brightness (7) are
taken from this same source, while the probability of being Cen45
cluster member (8) has been derived in Section\,5. Please note that if
prob$_{45}$=0.00 this automatically implies that the galaxy is a 100\%
Cen30 member. Column 11 contains the heliocentric radial velocity (cz)
and its estimated uncertainty, which results from a weighted average of
columns 9 (cross-correlation redshift) and column 10 (emission line
redshift).}\\ \hline 
\multicolumn{1}{c}{Seq} & \multicolumn{1}{c}{RA} &
\multicolumn{1}{c}{Dec} & \multicolumn{1}{c}{CCC} &
\multicolumn{1}{c}{Type} & \multicolumn{1}{c}{$B_{\rm T}$} &
\multicolumn{1}{c}{{\it SB}$_{\rm eff}$}&
\multicolumn{1}{c}{prob$_{45}$}& \multicolumn{1}{c}{V$_{\rm ccf}$} &
\multicolumn{1}{c}{V$_{\rm emi}$} & \multicolumn{1}{c}{V} \\
\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 \endfirsthead

\caption*{(cont.)}\\
\hline               
\multicolumn{1}{c}{Seq} & 
\multicolumn{1}{c}{RA} & 
\multicolumn{1}{c}{Dec} & 
\multicolumn{1}{c}{CCC} & 
\multicolumn{1}{c}{Type} &
\multicolumn{1}{c}{$B_{\rm T}$} & 
\multicolumn{1}{c}{{\it SB}$_{\rm eff}$}&
\multicolumn{1}{c}{prob$_{45}$}&
\multicolumn{1}{c}{V$_{\rm ccf}$} & 
\multicolumn{1}{c}{V$_{\rm emi}$} & 
\multicolumn{1}{c}{V}  \\
\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                 
\endhead
 
  2&12~44~46.32&$-$40~59~22.0&  4&S0    &16.93&22.1&0.00& 2704$\pm$61& 2714$\pm$58& 2709$\pm$42\\
  4&12~44~56.98&$-$41~15~21.9&  8&SB0   &14.03&21.5&0.00& 3531$\pm$25&         & 3531$\pm$25\\
  8&12~45~10.56&$-$40~38~53.0& 17&S0    &15.95&22.4&0.00& 3874$\pm$70&         & 3874$\pm$70\\
  9&12~45~14.22&$-$40~56~49.2& 19&d:S0  &15.82&22.1&0.00& 4059$\pm$19&         & 4059$\pm$19\\
 10&12~45~16.54&$-$41~01~57.5& 22&dE    &17.94&23.5&0.00& 2433$\pm$33&         & 2433$\pm$33\\
 11&12~45~16.76&$-$40~19~19.0& 24&SBd   &15.21&22.5&0.00&         & 4017$\pm$58& 4017$\pm$58\\
 12&12~45~19.01&$-$40~56~29.9& 26&SBc   &16.06&22.4&0.00& 1414$\pm$77&         & 1414$\pm$77\\
 17&12~45~35.56&$-$41~26~28.9& 43&S0    &14.05&20.6&0.00& 2647$\pm$25&         & 2647$\pm$25\\
 19&12~45~37.24&$-$40~51~03.2& 45&E     &14.93&20.8&0.00& 3681$\pm$49&         & 3681$\pm$49\\
 20&12~45~45.33&$-$41~02~02.8& 54&E     &15.90&20.3&0.00& 2958$\pm$44&         & 2958$\pm$44\\
 24&12~45~57.41&$-$41~22~15.9& 62&S0    &15.37&21.8&0.00& 2193$\pm$19&         & 2193$\pm$19\\
 25&12~46~03.51&$-$41~02~18.9& 65&E/S0  &11.32&22.6&0.00& 2985$\pm$31&         & 2985$\pm$31\\
 26&12~46~08.09&$-$41~02~48.0& 70&E     &15.64&18.3&0.00& 2317$\pm$20&         & 2317$\pm$20\\
 27&12~46~09.66&$-$40~18~33.0& 71&S0    &14.76&21.3&0.00& 3541$\pm$25&         & 3541$\pm$25\\
 31&12~46~17.22&$-$41~07~10.7& 76&dS0   &16.41&21.8&0.00& 5298$\pm$28&         & 5298$\pm$28\\
 32&12~46~18.34&$-$41~03~59.9& 77&Sc    &15.99&23.2&0.00& 3513$\pm$34&         & 3513$\pm$34\\
 33&12~46~20.34&$-$41~33~35.9& 80&S0    &14.78&21.8&0.13& 4422$\pm$23&         & 4422$\pm$23\\
 35&12~46~26.03&$-$41~16~21.5& 85&SBa   &15.07&22.5&0.00& 2839$\pm$20&         & 2839$\pm$20\\
 37&12~46~32.63&$-$41~03~48.0& 89&E     &15.77&20.0&0.00& 3104$\pm$19&         & 3104$\pm$19\\
 40&12~46~39.53&$-$41~09~25.0& 94&dS0,N &16.67&23.2&0.00& 4076$\pm$29&         & 4076$\pm$29\\
 41&12~46~40.18&$-$41~13~03.0& 95&SB0   &14.56&21.7&0.00& 4222$\pm$21&         & 4222$\pm$21\\
 43&12~46~46.81&$-$41~37~43.0&102&S0    &14.65&22.4&0.00& 3347$\pm$23&         & 3347$\pm$23\\
 44&12~46~48.55&$-$40~46~59.0&103&S0    &14.41&20.4&0.00& 1990$\pm$24&         & 1990$\pm$24\\
 45&12~46~51.82&$-$41~06~57.1&106&SB0/a &14.62&21.7&0.00& 3677$\pm$19&         & 3677$\pm$19\\
 46&12~46~52.56&$-$40~48~58.7&108&E     &16.11&19.9&0.00& 3263$\pm$36&         & 3263$\pm$36\\
 50&12~46~56.15&$-$40~24~51.9&114&SBb   &15.78&23.0&0.00& 2242$\pm$24&         & 2242$\pm$24\\
 51&12~47~05.57&$-$40~57~14.0&119&E     &14.64&20.3&0.00& 2101$\pm$23&         & 2101$\pm$23\\
 54&12~47~08.12&$-$41~00~26.3&122&S0/a  &14.18&21.6&0.00& 3845$\pm$23&         & 3845$\pm$23\\
 59&12~47~17.90&$-$41~06~35.9&130&E     &12.43&22.6&0.76& 4624$\pm$25&         & 4624$\pm$25\\
 60&12~47~21.59&$-$41~07~32.9&134&E     &15.04&20.6&0.66& 4966$\pm$31&         & 4966$\pm$31\\
 61&12~47~25.40&$-$40~56~57.2&135&E     &15.35&20.6&0.00& 2908$\pm$26&         & 2908$\pm$26\\
 62&12~47~26.12&$-$41~14~36.0&137&S0    &14.03&20.4&0.00& 2384$\pm$24&         & 2384$\pm$24\\
 66&12~47~38.33&$-$40~34~26.9&151&Sa    &14.27&22.2&0.79& 4640$\pm$20&         & 4640$\pm$20\\
 67&12~47~48.05&$-$41~11~58.0&158&S0    &14.77&21.3&0.01& 5249$\pm$24&         & 5249$\pm$24\\
 68&12~48~00.14&$-$41~37~20.9&165&S0    &14.87&20.7&0.89& 4758$\pm$25&         & 4758$\pm$25\\
 69&12~48~11.13&$-$41~07~28.9&170&S0    &15.24&20.4&0.25& 4466$\pm$19&         & 4466$\pm$19\\
 70&12~48~11.30&$-$40~36~53.0&171&BCD   &16.76&22.3&0.60& 4562$\pm$22&         & 4562$\pm$22\\
 73&12~48~14.65&$-$41~27~01.9&175&E     &14.65&21.7&0.00& 2469$\pm$23&         & 2469$\pm$23\\
 75&12~48~31.55&$-$40~32~50.0&181&SB0   &14.76&21.8&0.00& 3391$\pm$23&         & 3391$\pm$23\\
 78&12~48~42.69&$-$41~34~20.9&187&d:S0  &15.99&22.3&0.00& 1826$\pm$19&         & 1826$\pm$19\\
 79&12~48~46.40&$-$40~57~21.5&189&Sc    &15.02&21.3&0.89& 4771$\pm$24&         & 4771$\pm$24\\
 80&12~48~49.76&$-$41~13~14.4&190&dS0,N &16.11&21.7&0.00& 4048$\pm$23&         & 4048$\pm$23\\
 81&12~48~50.78&$-$41~01~54.7&191&S0    &15.32&21.1&0.00& 3467$\pm$22&         & 3467$\pm$22\\
 84&12~48~59.52&$-$40~59~42.7&203&dS0   &16.72&21.7&0.08& 4400$\pm$20&         & 4400$\pm$20\\
 85&12~49~01.57&$-$40~43~19.9&205&S0    &15.95&22.1&0.00& 2563$\pm$47&         & 2563$\pm$47\\
 86&12~49~04.27&$-$40~54~52.8&207&E     &16.01&21.0&0.87& 4712$\pm$18&         & 4712$\pm$18\\
 87&12~49~04.70&$-$41~09~38.3&208&dE,N  &17.44&23.3&0.00& 3624$\pm$22&         & 3624$\pm$22\\
 89&12~49~09.74&$-$41~16~02.8&210&SB0   &15.16&21.7&0.00& 3675$\pm$19&         & 3675$\pm$19\\
 90&12~49~13.97&$-$40~52~32.2&211&S0    &14.09&22.1&0.00& 2025$\pm$26&         & 2025$\pm$26\\
 93&12~49~14.56&$-$41~00~28.0&214&Sc    &14.73&22.6&0.89& 4806$\pm$32& 4757$\pm$50& 4792$\pm$27\\
 95&12~49~16.48&$-$41~11~17.6&217&SB0   &14.04&21.1&0.00& 3950$\pm$22&         & 3950$\pm$22\\
 98&12~49~26.21&$-$41~04~02.8&222&Sc    &14.74&23.2&0.17& 5107$\pm$31&         & 5107$\pm$31\\
 99&12~49~28.70&$-$41~12~19.0&224&dS0   &16.49&23.5&0.00& 3037$\pm$26&         & 3037$\pm$26\\
100&12~49~29.06&$-$40~59~15.5&225&S0    &15.71&22.5&0.00& 3459$\pm$23&         & 3459$\pm$23\\
101&12~49~29.31&$-$41~07~08.6&226&S0/a  &14.08&21.7&0.00& 2968$\pm$23&         & 2968$\pm$23\\
102&12~49~33.02&$-$40~47~22.0&227&SBa   &13.60&22.2&0.00& 3389$\pm$26&         & 3389$\pm$26\\
105&12~49~39.54&$-$40~26~13.0&236&SB0   &14.32&22.0&0.18& 4445$\pm$21&         & 4445$\pm$21\\
107&12~49~54.27&$-$40~57~31.0&242&S0    &15.46&19.3&0.85& 4858$\pm$23&         & 4858$\pm$23\\
108&12~50~18.65&$-$40~33~13.9&255&S0    &15.92&20.6&0.87& 4831$\pm$22&         & 4831$\pm$22\\
109&12~50~27.27&$-$40~52~10.6&260&dE,N  &17.59&23.9&0.00& 2766$\pm$43&         & 2766$\pm$43\\
110&12~50~39.31&$-$40~55~59.9&266&E     &13.08&21.4&0.01& 4314$\pm$23&         & 4314$\pm$23\\
111&12~50~55.53&$-$40~45~32.0&272&Im/BCD&16.51&23.0&0.00& 4215$\pm$48&         & 4215$\pm$48\\
113&12~51~19.19&$-$40~37~47.9&279&S0    &15.67&20.7&0.00& 3024$\pm$17&         & 3024$\pm$17\\
114&12~51~41.30&$-$40~53~12.0&284&Sd    &15.86&21.7&0.02& 4367$\pm$41& 4319$\pm$58& 4351$\pm$34\\
115&12~52~10.47&$-$40~42~48.9&290&E     &16.31&21.7&0.02& 4344$\pm$19&         & 4344$\pm$19\\
\hline
\end{longtable}
\end{document}
