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\markboth{Southern Hemisphere catalogue of Bordeaux}{Southern Hemisphere catalogue of Bordeaux}
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\begin{titlepage}
\vspace*{20.mm}
\begin{center}
\Huge {SOUTHERN HEMISPHERE } \\[20.mm]
\Huge {CATALOGUE of BORDEAUX} \\[50.mm]
\Large{\sf{Stars of the southern hemisphere proposed for the HIPPARCOS mission.}} \\ [15.mm]
\Large{\sf{J.M. Rousseau} \hspace{15.mm} \sf{J.P. P\'{e}ri\'{e} }} \\ [3.mm]
\hspace*{5.mm} \Large{\sf{M.T. Gachard }} \\ [5.mm]
\large{\sf{Observatoire de Bordeaux, INSU/CNRS-Universit\'{e} Bordeaux I }} \\ [3.mm]
\large{\sf{B.P. 89, F-33270 Floirac, France }} \\ [35.mm]
\large 1995
\end{center}
\end{titlepage}

\newpage
\begin{titlepage}
\vspace*{60.mm}
\begin{center}
\bf{Summary} \\
\end{center}
As part of the preparation for the Hipparcos mission, we determined the positions of 96800 already listed stars and 21265
previously unlisted companions, using information gathered by the ESO Quick Blue Survey. B1950 and J2000 system coordinates
are given for each star. The magnitudes and spectral types are given in addition to the exact date of the observation
(approximately 1976). PPM, HIC, SAO, HD, CoD, CPD, CPC, ADS, IDS, BD, LHS and V* identifiers are given systematically whenever
they exist as well as two supplementary identifiers selected from 43 other catalogues. Comments where necessary complete the
information. This catalogue is available from the Centre for Astronomic Data at Strasbourg.
\end{titlepage}

\newpage
\section{Introduction}

\subsection{Origin of the catalogue}
	In 1983, we were asked by C. Turon, acting on behalf of the INCA CONSORTIUM, to participate in the compilation of the
INPUT CATALOGUE for the HIPPARCOS mission.

	This catalogue includes all the objects observed by the satellite (Turon et al. 1992). One of the conditions required
for the correct running of this project was knowing, in advance, the position of each object in the programme with an accuracy
of 1.5" for each coordinate; 0.5" being unofficially desired. Although this requirement was satisfied for stars included in
more recent astrometric catalogues, (FK5, AGK3 and PERTH 70), it was not the case for those described exclusively in older
catalogues
or in personal lists of certain proposers. The only reliable solution, for a certain number of cases, was to redetermine the
positions, in a uniform manner, based on recent photographic observations or new meridian observations. The complete programme
of compilation and observation carried out for this project was described by Jahrei{\ss} et al. 1992. The work was performed by
a specialised team from the Bordeaux Observatory, using the appropriate equipment.

	We have presented below all the measurements taken at Bordeaux, from photographic plates, for stars in the southern
hemisphere. This was, in fact, the region of the sky in which the greatest number of problems and the least accuracy was
encountered, since the high density catalogues were either old (CoD, CPD) or approximate (HD).

\subsection{Observations}
	The time available was relatively short. The only way in which an entire hemisphere could be rapidly observed was by
using an instrument with a wide field of view. We initially studied the solution offered by cameras previously used for the
observation of artificial satellites (Baker-Nunn and Antares cameras). Considerable and costly hardware problems were
encountered in implementing these instruments and the results were disappointing; the accuracy obtained did not reach 1.5" and
the magnitude limit was insufficient. It soon became apparent that we would have to use copies of the ESO Quick Blue Survey
available from the Paris-Meudon Observatory. This recent collection is made up of 606 plates, in 30 x 30 cm format, i.e. 29
square degrees, with a scale of 0.0148 mm per arcsecond and an exposure time of 1 hour. The magnitude limit was approximately
20, well above our requirements. All these characteristics have been published (West \& Schuster 1982).

	However, the coverage of this collection is only for declinations from -17.5 to -90 degrees. We were thus limited to
observations within this zone, equivalent to approximately one third of the sky. The reference catalogue used was Perth 70,
which offers very recent observations, and which was the only reasonably dense astrometric list (approximately 1 star per
square degree) covering the zone in question in 1985 (H{\o}g \& von der Heide 1976).

	We checked that the use of glass copies instead of the original plates did not affect the accuracy. Comparative
measurements performed at Garching (where the originals are stored) using the Optronics measuring instrument, showed that the
results would not
be degraded. Indeed, for star-rich plates, the contrast quality is better on the copies, thus improving the ease and precision
of sightings.

\subsection{Catalogue composition and choice of objects}
Based on the proposals for the Hipparcos observation programme, the INCA CONSORTIUM team provided us with a list of 84323
objects, with no repetitions; many more than the 46785 stars of the Hipparcos Input Catalogue in our zone of 14225
square degrees. In order to avoid having to repeat measurements as a result of any subsequent programme revisions and also in
order to satisfy the requests not selected in the final choice for the programme, we decided not to take into account the
priorities and to treat all the proposed stars equally. This list was very close to the total number of proposals for the zone
under consideration. Each object was designated by an identifier, its magnitude, its 1950 coordinates (with variable precision)
and occasionally its proper motion.

	After measuring, and for various reasons, 389 objects were missing, including :

\begin{itemize}
\item[ ] - 72 variable stars with incorrect coordinates. \\
         - 13 stars ignored since they were too bright to be measured (noted in the table in Annex II).
However, certain bright stars, such as Antares, could be retained since their maximum radiation is in red and their image does
not have an excessively large diameter. \\
	 -  40 anonymous stars with insufficient data. \\
         -  17 high speed and faint stars, whose initial coordinates were inaccurate (L, LP, BPM, etc.). \\
         -  150 companions very close to a bright main object and obscured by its halo. \\
         -  41 stars whose identification was too uncertain.
\end{itemize}

To this initial list we added :

- Unexpected companions of stars included in the programme, that might induce errors when the star's position and magnitude was
measured by the satellite (as a function of their distance from the main object and their brightness). We determined their
position with the same accuracy as for the main objects and estimated the magnitude of most of them. The visible companions in
question are less than approximately 30" from the main object and have an estimated magnitude of up to 15. They were assigned
lower case letters
"b, c, d, etc." (with the main star identified by the letter "a"). Systems detected in this way do not appear in the ADS and
IDS catalogues. No indication of a dynamic link exists. Only the apparent proximity is indicated.

- Objects selected in regions not covered by any of the proposals that constitute the programme (the primary list is the sum of
the individual proposals, which do not cover the sky uniformly). When regions having a low stellar density were detected in this
list, we looked for identifiable objects and added them to the catalogue. Amongst these are 27 galaxies from the EQ, ESQ and MCQ
catalogues, distinctive for their well-defined nucleus which is easy to sight accurately.

- Companions not requested, but already known and included in the ADS and IDS catalogues.

\subsection{Measurements}
	The plates were measured using one of the observatory's Zeiss comparators. The instrument had been slightly modified
before the start of the work by mounting Heidenhain rules in order to automate the reading of the X and Y coordinates and to
eliminate human error. Furthermore, this device, which is commonly used, enabled readings to be directly transmitted to the
computer, thus avoiding transferral error. The construction of the rules enables a display to be obtained to the nearest
0.1$\mu$, however the average measurement scatter is 2$\mu$. As a result of the relatively long exposure time for these plates,
bright stars are shown as large images and are affected by diffraction, since the strips supporting the plate holder generate
a parasitic image of 4 to 8 branches. Up to approximately mag 10, the only measurement possible is to sight this cross. This was
the case for all the reference stars included in the Perth 70 catalogue. Whilst this procedure is not without flaws, the
diameter of the images prohibits any other solution. In order for this work to have been carried out with greater precision, for
a programme such as this which includes stars with magnitudes from 2 to 14, it would have been necessary to have several plates
for each field with increasing exposure times; which was not the case. Images fainter than B = 10 were circular without spikes.

	All the measurements for any one plate were carried out by one operator, as quickly as possible. Each reference star
was measured 4 times, and objects twice (since the plate was observed first in its normal position, and then after the optical
system was rotated through 90 degrees). A safety feature included in the acquisition programme immediately warned of any
erroneous sightings. Two operators performed all the measurements, over a period of 25 months.

\subsection{Reductions}
	The equatorial coordinates for the centre of each plate are known approximately (West \& Schuster 1982).
	On average, there were 32 reference stars per plate (varying from 20 to 43 depending on the region).

	A file was created for each plate, which after measuring included :
\begin{itemize}
\item[ ]
      - equatorial coordinates for each reference star, on the day of the observation. \\
      - rectangular coordinates for the same stars. \\
      - rectangular coordinates for the objects. \\
\end{itemize}

Using a traditional method (Barlier \& Muller 1964, Dodd 1972), this data enabled the determination of the value of the 10
coefficients (or plate constants) of the third order polynomials relating each equatorial coordinate to rectangular
coordinates.

The analysis and evaluation of all the coefficients resulting from the reduction of the 606 plates was performed separately
(Ducourant, Thesis 1989).

For each plate, the root-mean-square error is given by :
\begin{equation}
   \sqrt{\frac{\Sigma{(o-c)^{2}}}{(n-10)}}
\end{equation}

Any reference star whose (o - c) term was greater than 2.5 times the root-mean-square error of the plate, in right ascension
or in declination, was rejected and the reduction performed again.

For all the 18653 reference stars used, the root-mean-square deviation was 0.25" in right ascension and 0.29" in declination.

In the catalogue, the root-mean-square deviation of the plate for each coordinate is given for each star.

\subsection{Identifiers}
	Particular attention was paid to finding all the principal identifiers for each object. The search covered 55
different catalogues in addition to maps and lists of galactic open clusters. The procedure followed was :
\begin{itemize}
\item[ ] - Consultation of the Hipparcos Input Catalogue \\
         - Consultation at the Centre for Astronomic Data in Strasbourg (CDS) \\
         - Direct search in original works.
\end{itemize}

584 stars did not have an identifier. These stars were faint objects, with magnitudes fainter than 10, proposed to the
Hipparcos mission without being included in any catalogue.

\subsection{Comparison with the Carlsberg Automatic Meridian Catalogue}
	The Carlsberg Automatic Meridian Catalogue, (Vol. 4-6, 1989-1992) was selected as a reference since it had been
compiled using recent and impersonal meridian observations. Comparisons were not made for all the stars but by random local
samplings, and for the zone from - 17.5 degrees to - 45 degrees which was common to the two catalogues. For each common star,
the position was calculated, according to the CAMC at the ESO plate epoch (using the proper motion components given by this
catalogue). The Bordeaux-CAMC differences for each coordinate were also calculated. The mean value, or systematic error is
0.001s in right ascension and -0.055" in declination.

	It should be noted that the Bordeaux catalogue is referred to the Perth 70 catalogue (and thus to the FK4 system)
whilst the Carlsberg Meridian Catalogue uses the FK5 system.

	Isolated cases of differences of up to 0.5" were observed. They often correspond to stars located on the edges of the
ESO plates, or to double stars that we measured separately in contrast to the Carlsberg Meridian who sighted the combination.

\newpage
\section{Catalogue description}
The description follows the same order as the catalogue columns.

\subsection{Number (N$^{o}$)  }
	Numbers are given, from 1 to 118065, irrespective of the hierarchy of the object. The object's rank is recognised :
\begin{itemize}
\item[ ] - for systems that are already known, by the suffix (A, B, C, etc.) to the ADS or IDS identifier. \\
         - for previously unlisted systems, that we detected, by the letter "a" after the main object, and letters b, c, d,
            etc. after the companions.
\end{itemize}

The star entries follow the order of the object's right ascension (J2000), except for previously unlisted companions (with b,
c, d, etc.) which immediately follow the associated main object. In other words, it is the right ascension of the main object
"a" which places the system in the catalogue. This should avoid annoying "mix-ups" with other objects or other systems.

In accordance with the Centre for Astronomic Data at Strasbourg, we suggest to use the acronym SHB (Southern Hemisphere
Bordeaux).

    In order to simplify the consultation of the right-hand page, the column "$N^{o}$" is repeated.

\subsection{Magnitude (Mag) }
	It was not possible to add the measurement of photographic magnitude to our work. We have therefore drawn this data
from various sources, hence their lack of homogeneity. For the same reasons, the magnitudes are either in B or V. If the
source is incomplete in this respect, no colour is indicated. Our sources were :
\begin{itemize}
  \item[ ] - the HIC catalogue \\
           - the Centre for Astronomic Data at Strasbourg. \\
           - original catalogues (HD, CoD, CPD). \\
           - ADS and IDS catalogues for companions not included in the programme. \\
           - the list of the sum of proposals. \\
           - our personal estimations, made by rapid comparison with nearby stars. \\

           This process may lead to errors, depending on the colour of the object, of up to 1.5 magnitudes. It was used in
           cases where data was not present in other catalogues. The values given should only be used as an indication.
\end{itemize}

\subsection{Spectral type (Sp) }
	The same reservations apply, to an even greater degree, to the indications of the spectral type. Since this parameter
is only given by way of an indication, we have kept only 2 characters corresponding to the principal types.

\subsection{J2000 and B1950 positions}
We have continued with the B1950 positions, which are still widely used today. They refer to the FK4 system, as does the
Perth 70 catalogue which provided our reference stars.

We just precessed the B1950 coordinates originally measured to 2000 (Lieske et al. 1977 and 1979). We did not apply the
regional systematic differences between the FK5 and FK4 system given e.g., with the FK5.

\subsection{Precision, epoch and number of observations ($\sigma_{\alpha},\sigma_{\delta}$,\normalsize{Ep,N}) }

\begin{itemize}
	\item[ ] - $\sigma_{\alpha},\sigma_{\delta}$ : In principle, each star should only have been examined once. However,
the plates from the ESO Quick Blue Survey overlap, to a
greater or lesser extent. Stars located on the edges may therefore have been measured 2 or even 4 times (in a corner).
Furthermore, and for various reasons, certain plates were measured several times. Occasionally both cases occurred for the
same plate. The following solutions have been adopted :

\begin{itemize}
    \item[ ]  - Several positions of an object for the same plate :
    \begin{itemize}
        \item[]   The mean position of the object is used, on the plate epoch.
    \end{itemize}
             - One or more positions of an object on more than one plate. We give :
    \begin{itemize}
       \item[]             the average of the positions \\
                           the average of the plate epochs \\
                           the resulting deviation for each coordinate :
       \begin{itemize}
       \item[ ]
             \begin{equation}
                  \sqrt{\frac{\Sigma{(\sigma)^{2}}}{n}}   \\
             \end{equation}
        \end{itemize}
     \end{itemize}
                  where $\sigma$  is the deviation resulting from each reduction, as has already been defined, for reference
                  stars only.
\end{itemize}

	\item[ ] - \normalsize{Ep} : The relatively small time period separating two plates allowed us to use mean positions
(the plates were exposed between 30/03/1973
and 22/02/1979). In many cases, neighbouring plates correspond to very similar epochs.

	The epoch of each plate is known to the nearest second (West \& Schuster, 1982). This precision is not required for
this type of catalogue. We therefore only give the epoch (Ep) to the nearest 0.01 year.

	\item[ ] - \normalsize{N} : Indicates the number of measurements carried out for this star.
\end{itemize}

\subsection{Comment (Com) }
This column contains a wide range of information :

\begin{tabular}{lp{138.mm}}
m..         & The estimated magnitude of previously unlisted companions, to the nearest 1 mag, given by way of an indication
only (varying from 10 to 16). The magnitude of a certain number of these companions was not estimated when work began on the
plates.\\
2 to 39     & Indicates that the star forms part of a group of n stars, in which each star is less than 50" from another. The
most frequent numbers are 2 and 3 and are often observed in relation to systems cited by the ADS and IDS catalogues. The other
numbers relate in general to members of galactic open clusters. This number should be primarily considered as a signal
indicating the proximity of other objects and thus the risk of confusion or identification error. \\
a = b	    & Components a and b appear to be equal in magnitude. \\
D	    & The star in question may be a double star (69 cases). \\
S	    & The star in question is part of a pair that is too close together to enable the measurement of the two
              components.\\
?           & A doubt exists as to the identification of the components. The allocation of the letters a and b is arbitrary. \\
\verb|*|    & See notes (listed in Annex V) \\
\end{tabular}

\subsection{LHS/V*  }
	This is the first column relating to identifiers. It gives both the stars included in the Luyten Half-Second Catalogue
(Luyten 1979) (stars with proper motion larger than 0.5" annually) and variable stars taken from the General Catalogue of
Variable Stars (GCVS, Kholopov, 1990). These categories may be combined in the same field since no star is included in both
catalogues. Variable stars designated uniquely by a Greek letter and the constellation are mentioned in the notes (* in the
Com. column and notes in Annex V).
\begin{itemize}
\item[ ] Format of LHS identifiers : nnnn : (running number)
\item[ ] Format of identifiers for variable stars : LL ccc :
     \begin{itemize}
     \item[ ] (LL = Upper case letters) \\
              (ccc = Abbreviation of the constellation)
    \end{itemize}
\end{itemize}

\subsection{PPM, HIC, SAO  }
	Gives the numbers taken from the following catalogues :
\begin{itemize}
\item[] - Positions and Proper Motions (Bastian U. et al., 1992). \\
	- HIC (Turon C. et al., 1992).
\begin{itemize}
\item[ ]\it{\bf{Attention : Replace each "INCA" occurence by "HIC". This type mismatch was discovered too late to be modified
before printing. \\}}
\end{itemize}
\normalsize
	- Smithsonian Astrophysical Observatory Star Catalogue (1966).
\end{itemize}

\begin{itemize}
\item[ ] Format of PPM, HIC, SAO identifiers : nnnnnn : (running number)
\end{itemize}

\subsection{HD }
	Gives numbers taken from the :
\begin{itemize}
\item[ ]
- Henry Draper Catalogue (Cannon \& Pickering 1918-1949) \\
- Henry Draper Extensions (Cannon 1925-1936, Cannon \& Mayall 1949)
\end{itemize}

	When a star belonging to the HD catalogue is double or multiple (according to ADS or IDS) the letter A is never placed
after the HD number of the main object. However, the companions are assigned the same HD number followed by the same suffix B,
C, etc. as in the ADS or IDS identifier.

	The character + following an HD identifier indicates that the entry relates to two neighbouring stars in our catalogue
(one or the other or the sum of both) for which the doubt has not been resolved (inaccuracy of the positions in the HD catalogue
and absence of comments). It does not form part of the identifier.

\begin{itemize}
\item[ ] Format of HD identifiers : nnnnnn : (running number)
\end{itemize}

\subsection{CD and CPD }
	Respectively give the numbers from the Cordoba Durchmusterung (Thome 1892, 1894, 1900, 1914 and Perrine 1932),
and those from the Cape Photographic Durchmusterung (Gill 1903).

	The HD Convention has not been taken into consideration. The two CD and CPD identifiers are given regardless of the
declination of the star under consideration.

	When a star belonging to one of these catalogues is double or multiple, according to ADS or IDS, the identifier is
given for each component, accompanied by the same suffix A, B, C, etc. as the ADS or IDS identifier.

	The character + following an CD or CPD identifier indicates that the entry relates to two neighbouring stars in our
catalogue (one or the other or the sum of both) for which the doubt has not been resolved (inaccuracies in the CD or CPD
catalogue and absence of comment). It does not form part of the identifier.

	Certain CD or CPD identifiers are followed by a "p" or an "s". Should two stars be close together, correspond to a
single CD or CPD identifier, and not be included in the ADS and IDS catalogues, this notation enables the components to be
more clearly designated. This system has been adopted by the Centre for Astronomic Data in Strasbourg.
\begin{itemize}
\item[ ] Format of CD and CPD identifiers : -dd nnnnn :
      \begin{itemize}
       \item[ ] (dd = Declination degree for the 1875 equinox) \\
		(nnnnn = running number)
       \end{itemize}
\end{itemize}

\subsection{CPC   }
	Gives the numbers from the Cape Photographic Catalogue for 1950.0 (Jackson \& Stoy 1954-1968).

	In 4 cases, the character + following a CPC identifier indicates that this entry relates to two neighbouring stars in
our catalogue. It does not form part of the identifier. This fusion is indicated in a note in the actual CPC catalogue.
\begin{itemize}
\item[ ] Format of CPC identifiers : vv nnnnn :
      \begin{itemize}
      \item[ ] (vv = volume number of the Cape Photographic Catalogue for 1950.0 \\
	       (nnnnn = running number)
      \end{itemize}
Note that volume 20 is broken down into 20 and 20.1.

Stars designated by CPC 0 nnnnn are included in the "Catalogue of the positions and proper motions of stars between
declinations $-40^{o}$ and $-50^{o}$" (Hoffleit 1970).
\end{itemize}

\subsection{ADS/IDS }
	Contains the identifiers from the New General Catalogue of Double Stars (Aitken 1932) and the Index of Double Stars
(Jeffers 1963).

	It was possible to group the identifiers since their formats are very different. The presence of a 2-letter suffix (AB,
BC, etc.)
indicates that we were unable to separate the two components from fused or very close images.
\begin{itemize}
\item[ ] Format of ADS identifiers : nnnnnL :
         \begin{itemize}
         \item[ ] (nnnnn = running number) \\
		  (L = component rank)
         \end{itemize}
\item[ ] Format of IDS identifiers : hhhhh-ddddL :
         \begin{itemize}
         \item[ ] (hhhhh = Right ascension 1900 in Hours minutes and tenths) \\
		  (dddd = Declination 1900 in degrees and arcminutes) \\
		  (L = Suffix giving the component rank)
         \end{itemize}
\end{itemize}

\subsection{Others}
	The identifiers described in the previous 9 columns correspond to the major catalogues in common use. However it was
necessary to mention others, in a less systematic way, depending on the space available. These are often local or smaller
catalogues. Priority was given to the BD (Sch\"{o}nfeld 1886), L, LP, LTT (Luyten 1957,1979,1980) identifiers and the numbers
designating the members of galactic open clusters (see Annexes I and IV). The presence in this column of BD identifiers is
justified by the zone of less than 6 degrees included in the Bonner Durchmusterung.

We have occasionally given additional identifiers in the notes (Annex V), indicated by a * in the Com. column.

\begin{itemize}
\item[ ] Format of BD identifiers : -dd nnnnn :
         \begin{itemize}
         \item[ ] (dd = Declination degree for the 1855 equinox) \\
		  (nnnnn = running number).
         \end{itemize}
\end{itemize}

\section{Annexes}
Tabulated annexes precede the actual catalogue :

\begin{tabular}{llp{125.mm}}
\\
 ANNEX I     & : & Identifiers used : Abbreviations, names and references of the catalogues used. \\
 ANNEX II    & : & Stars ignored for being too bright in blue. \\
 ANNEX III   & : & Bibliography. \\
 ANNEX IV    & : & List of the galactic open clusters whose members are included in the catalogue. \\
 ANNEX V     & : & Specific notes concerning certain objects (comment *).
\end{tabular}

\section{Conclusion}
	This catalogue has not been compiled simply for astrometric purposes, but primarily to prepare for the HIPPARCOS
satellite mission.
Having fulfilled this role, it has been adapted to meet the requirements of observers and those who would like to identify
objects with varied names, hence the care taken in terms of cross-referencing identifications from 55 catalogues. Numerous
ambiguous cases have been individually dealt with, in particular in the galactic open clusters and multiple systems through
referring to original articles and reference works. The catalogue's principal characteristic is its homogeneity, since it has
been compiled from plates taken by one instrument, measured using one machine, in a short time, by just two operators, and
reduced by one method, the results of which were submitted to identical criteria.

This catalogue has been filed at the Centre for Astronomic Data in Strasbourg and is also available in printed form.

\section{Acknowledgements}
	This work was carried out following checks performed at Garching using the Optronics measuring instrument on the
original plates. We would like to thank R. M. West for giving us permission to use these plates in these exceptional
circumstances. The library of the Paris-Meudon Observatory successively lent us the 606 plates taken by the ESO Quick Blue
Survey in spite of the risks involved in the many transfers between Meudon and Bordeaux. Without these documents and the
guarantee of their high quality, this work would not have been possible. The workshop at the Bordeaux Observatory carried out
a great deal of essential work in modifying and maintaining our Zeiss instrument. The Computing Department designed the
acquisition and measurement data transfer systems. Many people assisted, in various roles, with the demanding work involved
in taking the measurements. Their help is gratefully acknowledged.

	Our particular thanks go to C. Turon, who, together with her team, advised us and provided documentation over several
years. Without her, this catalogue would not have been compiled.

\newpage
\vspace{20.mm}
\begin{center}
\Large{\underline{\bf{ANNEX I}}} \\[40.mm]
\large{\framebox(120,10){\bf{Identifiers used in the catalogue}}} \\[40.mm]
\end{center}

\begin{tabular}{lp{125.mm}}
\\
ADS  &     New General Catalogue of Double Stars within $120^{o}$  of the North Pole  (Aitken 1932)\\
ARDB &    Spectrographic and Photometric Observations of Supergiants and Foreground  Stars in the
direction of the LMC (Ardeberg; Brunet; Maurice \& Pr\'{e}vot 1972)\\
BD   &    Bonner Durchmusterung  (Sch\"{o}nfeld 1886) \\
BPM  &     Bruce Proper Motion Survey  (Luyten 1963)\\
BRAN &     Catalogue of Nebulous Objects  (Brand; Blitz \& Wouterloot 1986)\\
CD   &     Cordoba Durchmusterung (Thome 1892, 1894, 1900, 1914 and Perrine 1932)\\
CEL  &     Celescope Catalogue of UV Stellar Observations  (Davis et al. 1973)\\
CF   &     Cape Catalogue of Faint Stars  (Spencer-Jones \& Jackson 1939)\\
CPC  &     The Cape Photographic Catalogue for 1950.0  (Jackson \& Stoy 1954...1968 and Hoffleit 1970)\\
CPD  &     Cape Photographic Durchmusterung  (Gill 1903)\\
Ci   &     Catalogue of Proper motions  (Porter et al. Cincinatti 1918)\\
C*   &     Cool Carbon Stars Catalogue  (Stephensen 1973)\\
EM*  &     Lick H Alpha Catalogue\\
ESO  &     ESO/Uppsala Survey of the ESO B (Holmberg et al. 1974...1981)\\
FK4  &     Fourth Fundamental Catalogue  (Fricke et al. 1963)\\
G    &     Lowell Proper Motion Survey  (Giclas et al. 1959...1978)\\
GCRV &     General Catalogue of Radial Velocities  (Wilson 1953)\\
GJ   &     Extension of the Catalogue of Nearby Stars  (Gliese \& Jahrei{\ss} 1979)\\
HD   &     Henry Draper Catalogue  (Cannon \& Pickering 1918...1949) and\\
     &     Henry Draper Extensions (Cannon 1925...1936 and Cannon \& Mayall 1949)\\
He   &     Southern Emission-Line Stars  (Henize 1976) \\
HIC  &     Hipparcos Input Catalogue, (Turon et al. 1992)\\
\end{tabular}

\newpage
\begin{tabular}{lp{125.mm}}
IC   &     Index Catalogue 1895 et Second Index Catalogue (Dreyer 1908)\\
IDS  &     Index of Double Stars  (Jeffers et al. 1963)\\
IRAS &     Infrared Astronomical Satellite (Persi 1990) \\
IRC  &     Caltech 2 $\mu$  Survey  (Neugebauer et al. 1969)\\
L    &     Luyten Catalogue  (Luyten 1942)\\
LF   &     UBV Photoelectric Photometry in Four Southern Milky Way Fields  (Wooden II 1970 )\\
LHS  &     Luyten Half-Second Catalogue  (Luyten 1979)\\
LP   &     Luyten Palomar Catalogue (Luyten 1963...1987)\\
LS   &     Luminous stars in the Southern Milky Way  (Stephenson \& Sanduleak 1971)\\
LTT  &     Luyten Two-Tenth Catalogue  (Luyten 1957)\\
MCG  &     Morphological Catalogue of Galaxies  (Vorontsov et al. 1968...)\\
NGC  &     New General Catalogue  (Dreyer 1888)\\
OM   &     Non Supergiant Stars Near Magellanic Clouds (Carozzi 1974)\\
PHL  &     Faint Blue Stars in the Region Near the South Galactic Pole (Haro \& Luyten 1962)\\
PK   &     Planetary Nebulae  (Perek \& Kohoutek 1967)\\
PLX  &     Parallaxes  (Jenkins 1952,1963)\\
PMMR &     Catalogue of late-type stars in SMC  (Pr\'{e}vot; Maurice; Martin \& Rebeirot 1983)\\
PPM  &     Positions and Proper Motions  (Bastian U. et al. 1992)\\
RMC  &     The Brightest Stars in the Magellanic Couds  (Feast; Thackeray \& Wesselink 1960)\\
RMMP &     Catalogue of late-type stars in LMC  (Rebeirot; Maurice; Martin \& Pr\'{e}vot 1983)\\
SAO  &     Smithsonian Astrophysical Observatory Star Catalogue 1966\\
SB   &     List of Early-Type Stars near the South Galactic Pole  (Slettebak \& Brundage 1971)\\
SK   &     Stars in the Large \& Small Magellanic Clouds (Sanduleak 1968,1969ab) \\
SRS  &     Southern Reference System Catalogue  (Smith et al. 1990)\\
SZ   &     Survey of Southern Dark Clouds for Herbig-Haro objects and H-Alpha Emission Stars (Schwartz 1977)\\
UBV  &     Photoelectric Catalogue, magnitude and color of stars in UBV (Blanco et al. 1968)\\
UBV M&     UBV Photoelectric Photometry Catalogue (Mermilliod 1987) \\
VDB  &     Reflexion Nebulae (van den Bergh 1966)\\
VDBH &     Catalogue of Southern Stars Embedded in Nebulosity (van den Bergh \& Herbst 1975a,b)\\
V*   &     General Catalogue of Variable Stars GCVS (Kholopov 1990)\\
WD   &     Catalogue of White Dwarfs (Mc Cook \& Sion 1977)\\
WT   &     New proper motions stars south of $-40^{o}$ and Right Acensions between 00h and 04h 30m (Wroblenski \&
           Torres 1989)\\
\\
NOTE : &   Annex IV refers to galactic open clusters identifiers.
\end{tabular}

\newpage
\vspace{20.mm}

\begin{center}
\Large{\underline{\bf{ANNEX II}}} \\[40.mm]
\large{\framebox(120,10){\bf{Excluded stars (too bright)}}} \\[40.mm]
\end{center}

\begin{tabular}{@{\hspace{25.mm}}rlll}
\vspace{1.mm}
No Hic & & &  \\ \vspace{1.mm}
30324  & SAO 151428 & = HD 44743  & = beta CMa   \\ \vspace{1.mm}
30438  & SAO 234480 & = HD 45348  & = alfa Car   \\ \vspace{1.mm}
33579  & SAO 172676 & = HD 52089  & = epsilon CMa   \\ \vspace{1.mm}
39429  & SAO 198752 & = HD 66811  & = zeta Pup   \\ \vspace{1.mm}
42913  & SAO 236232 & = HD 74956  & = delta Vel   \\ \vspace{1.mm}
60718  & SAO 251904 & = HD 108248 & = alfa 01 Cru   \\ \vspace{1.mm}
60718  &            & = HD 108249 & = alfa 02 Cru   \\ \vspace{1.mm}
62434  & SAO 240259 & = HD 111123 & = beta Cru   \\ \vspace{1.mm}
71681  & LHS 51     & = HD 128621 & = alfa 02 Cen   \\ \vspace{1.mm}
71683  & SAO 252838 & = HD 128620 & = alfa 01 Cen   \\ \vspace{1.mm}
85696  & SAO 208896 & = HD 158408 & = upsilon Sco   \\ \vspace{1.mm}
85927  & SAO 208954 & = HD 158926 & = lambda Sco   \\ \vspace{1.mm}
113368  & SAO 191524 & = HD 216956 & = alfa PsA   \\ \vspace{1.mm}
\end{tabular}

\newpage
\vspace{20.mm}

\begin{center}
\Large{\underline{\bf{ANNEX III}}} \\[40.mm]
\large{\framebox(120,10){\bf{Bibliography }}} \\[40.mm]
\end{center}

\begin{tabular}{lp{142.mm}}
\\
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   Washington \\
 & Ardeberg et al., 1972, Astron. Astrophys. Suppl., 6, 249 \\
 & Barlier F. \& Muller P., 1964, Bull. Astr. Obs. Paris, XXIV, 29   \\
 & Bastian U. et al., 1992, PPM South Star Catalogue, Astronomisches Rechen-Institut, Heidelberg \\
 & Bergh S. van den, 1966, Astron. J., 71, 990 \\
 & Bergh S. van den, Herbst W., 1975a, Astron. J., 80, 208 and 255 \\
 & Blanco V.M. et al., 1968, Photoelectric Catalogue, Publ. of the U.S. Naval Observatory, Second series, Vol XXI \\
 & Brand J., Blitz L., Wouterloot J.G.A., 1986, Astron. Astrophys. Suppl., 65, 537 \\
 & Cannon A.J. \& Pickering E.C., 1918-1924, Henry Draper Catalogue, Ann. Astron. Obs. Harvard College, Vol 91-99 \\
 & Cannon A.J. 1925, Henry Draper Extension I, Ann. Astron. Obs. Harvard College, Vol 100 \\
 & Cannon A.J. \& Walton Mayall M., 1949, Henry Draper Extension II, Ann. Astron. Obs. Harvard College, Vol 112 \\
 & Carlsberg Meridian Catalogue La Palma, Vol 4 (1989), Vol 5 (1991), Vol 6 (1992)                   \\
 & Carozzi N., 1974, Astron. Astrophys. Suppl., 16, 277 \\
 & Davis et al., 1973, Celescope Catalogue of UV photometrie, SAO Special Report, 350, 1973 \\
 & Dodd R.J., 1972, Astron. J., 77, 306 \\
 & Dreyer J.L.E., 1888, New General Catalogue, Royal Astronomical Society, London \\
 & Dreyer J.L.E., 1895 and 1908, Index Catalogue and Second Index Catalogue, Royal Astronomical Society, London \\
 & Ducourant C., 1989, Th\`{e}se de Doctorat Bordeaux                                      \\
 & Feast M.W., Thackeray A.D. and Wesselink A.J., 1960, Mon. Not. R. Astr. Soc., 121, 4, 337 \\
 & Giclas H.L. et al., 1958-1979, Lowell Proper Motion Survey, Lowell Obs. Bull., 89-165 \\
\end{tabular}

\newpage

\begin{tabular}{lp{142.mm}}
\\
 & Gill D. \& Kapteyn J.C., 1896-1897-1900, The Cape Photographic Durchmusterung, Annals of the Cape Observatory,
   Vol III-V \\
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 & Henize K.G., 1976, Observations of Southern Emission-line Stars, Astrophys. J. Suppl. Series, 30, 491 \\
 & Herbst W., 1975b, Astron. J. 80, 212 \\
 & Hoffleit D., 1970, Catalogue of the positions and proper motions of stars between declinaisons $-40^{o}$ and
   $-50^{o}$, Transactions of the Astronomical Observatory of Yale University, New Haven, Vol 30 \\
 & H{\o}g E. \& von der Heide J., 1976, Abhandlungen aus der Hamburger Sternwarte $n^{o}$9  \\
 & Holmberg et al., 1974a, (Paper I), Astron. Astrophys. Suppl., 18, 463 \\
 & Holmberg et al., 1974b, (Paper II), Astron. Astrophys. Suppl., 18, 491 \\
 & Holmberg et al., 1975, (Paper III), Astron. Astrophys. Suppl., 22, 327 \\
 & Holmberg et al., 1977, (Paper IV), Astron. Astrophys. Suppl., 27, 295 \\
 & Holmberg et al., 1978a, (Paper V), Astron. Astrophys. Suppl., 31, 15 \\
 & Holmberg et al., 1978b, (Paper VI), Astron. Astrophys. Suppl., 34, 285 \\
 & Holmberg et al., 1980, (Paper VII), Astron. Astrophys. Suppl., 39, 173 \\
 & Jackson J. \& Stoy R.H. 1954-1968, Cape Photographic Catalogue for 1950.0, Annals of the Cape Observatory, Vol XVII-XXII \\
 & Jahrei{\ss} H. et al., 1992, Astron. Astrophys., 258, 82                                                \\
 & Jeffers H.M., van den Bos W.H., and Greeby F.M., 1963, Index Catalogue of Visual Double Stars, Univ. California,
Publ. Lick Obs., Vol XXI \\
 & Jenkins L., 1952, General Catalogue of Trigonometric Parallaxes, New Haven, Conn., Yale Univ. Obs. \\
 & Jenkins L., 1963, Supplement to the General Catalogue of Trigonometric Parallaxes, New Haven, Conn., Yale Univ. Obs. \\
 & Kholopov P.N. et al., 1990, General Catalogue of Variable Stars, Fourth Edition, Moscow, Nauka Publ. House \\
 & Lauberts et al., 1981, (Paper VIII), Astron. Astrophys. Suppl., 43, 307 \\
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 & Lieske J.H. et al., 1977, Astron. Astrophys., 58, 1 \\
 & Lieske J.H., 1979, Astron. Astrophys., 73, 282 \\
 & Luyten W.J., 1957, Luyten Two-Tenths Catalogue, Univ. Minesota, Mineapolis \\
 & Luyten W.J., 1963, Bruce Proper Motion Survey, Univ. Minesota, Mineapolis \\
 & Luyten W.J., 1979, Luyten Half-Second Catalogue, Univ. Minesota, Mineapolis \\
 & Luyten W.J., 1980, New Luyten Two-Tenths Catalogue, Univ. Minesota, Mineapolis \\
 & McCook G.P. \& Sion E.M., 1977, Villanova Univ. Obs. Contr., $n^{o}$2 \\
 & Mermilliod J.C., 1987, Astron. Astrophys. Suppl., 71, 413   \\
 & Neugebauer G. et al., 1969, NASA SP-3047 \\
 & Perek L. \& Kohoutek L., 1967, Catalogue of galactic planetary nebulae, Prague, Academia Publ. House Czechoslovak Academy
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\end{tabular}

\begin{tabular}{lp{142.mm}}
\\
 & Pr\'{e}vot L. et al., 1983, Astron. Astrophys. Suppl., 53, 255 \\
 & Rebeirot E. et al., 1983, Astron. Astrophys. Suppl., 51, 277 \\
 & Sanduleak N., 1968, Astron. J., 73, 246 \\
 & Sanduleak N., 1969a, Cerro Tololo Inter-American Observatory Contr., $n^{o}$89 \\
 & Sanduleak N., 1969b, Astron. J., 74, 877 \\
 & Schonfeld E., 1886, Bonner Sternverzeichniss, Vierte section, A. Marcus, Bonn \\
 & Schwartz R., 1977, Astrophys. J. Suppl., 35, 161 \\
 & Slettebak A. \& Brundage R.K., 1971, Astron. J., 76, 338 \\
 & Smith C. et al., 1990, IAU Symp. 141, Lieske J. \& Abalakin V. (eds), 457 \\
 & Smithsonian Institution, 1966, Smithsonian Astrophysical Observatory Star Catalogue, Washington D.C. \\
 & Spencer-Jones H. \& Jackson J., 1939, Catalogue of 20554 faint stars in the Cape Astrographic Zone
$-40^{o}$ to $-52^{o}$ for the Equinox of 1900.0, Royal Observatory Cape of Good Hope \\
 & Stephensen C.B., 1973, A General Catalogue of Cool Carbon Stars, Publ. Warner and Swasey Obs., 1, $n^{o}$4 \\
 & Stephenson C.B. \& Sanduleak N., 1971, Luminous Stars in the Southern Milky Way, Publ. Warner and Swasey Obs. 1 $n^{o}$1 \\
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 & Vorontsov-Vemyaminov B.A. and Arkhipova V.P., 1968, Morphological Catalogue of Galaxies, IV, Moscow State University,
   Moscow \\
 & West R. M. \& Schuster H. E., 1982, Astron. Astrophys. Suppl., 49, 577 \\
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 & Wroblenski H. \& Torres C., 1989, Astron. Astrophys. Suppl., 78, 231 \\
 & \\
 & \\
 & Articles dealing with galactic open clusters. (listed in Annex IV). \\
\end{tabular}

\newpage
\begin{center}
\vspace{20.mm}
\Large{\underline{\bf{ANNEX IV}}} \\[40.mm]
\large{\framebox(120,10){\bf{List of the galactic open clusters }}} \\[40.mm]
\end{center}

\begin{tabular}{lll}

  Basel 19       & : Fenkart R.P. et al.          & 1977, Astron. Astrophys. Suppl. 30,307 \\

\vspace{0.8mm}

  Blanco 1       & : Westerlund B.E.              & 1988, Astron. Astrophys. Suppl. 76,101 \\

\vspace{0.8mm}

  Bochum 9       & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Bochum 10      & : Feinstein A.                 & 1981, Publ. Astr. Soc. Pacific 93,202 \\

\vspace{0.8mm}

  Bochum 11      & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Bochum 13      & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,155 \\

\vspace{0.8mm}

  Collinder 140  & : Clari\'{a} J.J., Rosenzweig P.      & 1978, Astron. J. 83,278 \\

\vspace{0.8mm}

  Collinder 185  & : Lindoff U.                          & 1968, Arkiv f\"{o}r Astronomi. Bd 5 nr 4,63 \\

\vspace{0.8mm}

  Collinder 197  & : Vogt N., Moffat A.F.J.               & 1972, Astron. Astrophys. Suppl.  9,97 \\

\vspace{0.8mm}

  Collinder 223  & : Clari\'{a} J.J., Lapasset E.         & 1991, Publ. Astr. Soc. Pacific 103,998 \\

\vspace{0.8mm}

  Collinder 228  & : Th\'{e} P.S.  et al.                & 1980, Astron. Astrophys. Suppl. 41,93 \\

\vspace{0.8mm}

  Collinder 258  & : Moffat A.F.J., Vogt N.               & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Collinder 271  & : Moffat A.F.J., Vogt N.               & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Feinstein 1    & : Feinstein A.                        & 1964, Observatory 84,111 \\

\vspace{0.8mm}

  Hogg 10        & : Moffat A.F.J., Vogt N.               & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Hogg 11        & : Moffat A.F.J., Vogt N.               & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Hogg 12        & : Moffat A.F.J., Vogt N.               & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Hogg 14        & : Moffat A.F.J., Vogt N.               & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Hogg 15        & : Feinstein A., Marraco H.G.           & 1971, Publ. Astr. Soc. Pacific 83,218 \\

\vspace{0.8mm}

  Hogg 16        & : Moffat A.F.J., Vogt N.               & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Hogg 17        & : Lindoff U.                          & 1967, Arkiv f\"{o}r Astronomi. Bd 4 nr 33,493 \\

\vspace{0.8mm}

  Hogg 18        & : Hogg A.R.                           & 1961, Observatory 81,69 \\

\vspace{0.8mm}

  Hogg 22        & : Moffat A.F.J., Vogt N.               & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  IC 2391        & : Mermilliod J.C.                     & 1976, Astron. Astrophys. Suppl. 24,159 \\

\vspace{0.8mm}

  IC 2395        & : Lyng{\aa} G.                        & 1959, Arkiv f\"{o}r Astronomi. Bd 3 nr 8,65 \\

\vspace{0.8mm}

  IC 2581        & : Evans T.L.                          & 1969, Mon. Not. R. Astr. Soc. 146,101 \\

\end{tabular}
\newpage
\begin{tabular}{lll}

  IC 2602        & : Braes L.L.E.                        & 1962, Bull. Astr. Inst. Netherl. 14, No 16,297 \\

\vspace{0.9mm}

  IC 2944        & : Ardeberg A., Maurice E.              & 1977, Astron. Astrophys. Suppl. 28,153 \\

\vspace{0.8mm}

  IC 4651        & : Lindoff U.                          & 1972, Astron. Astrophys. Suppl. 7,231 \\

\vspace{0.8mm}

  IC 4725        & : Landolt A.U.                        & 1963, Astrophys. J. Suppl. 8,352 \\

\vspace{0.8mm}

  Lod\'{e}n 1409     & : J{\o}rgensen U.G., Westerlund    & 1988, Astron. Astrophys. Suppl. 72,193 \\

\vspace{0.8mm}

  Lyng{\aa} 2        & : Lindoff U.                      & 1967, Arkiv f\"{o}r Astronomi. Bd 4 nr 32,471 \\

\vspace{0.8mm}

  Lyng{\aa} 6        & : Moffat A.F.J., Vogt N.           & 1975, Astron. Astrophys. Suppl. 20,155 \\

\vspace{0.8mm}

  Lyng{\aa} 7        & : Lyng{\aa} G.                    & 1964, Medd. Lunds Astr. Obs. 2 no 139 \\

\vspace{0.8mm}

  Markarian 18   & : Vogt N., Moffat A.F.J.               & 1972, Astron. Astrophys. Suppl.  9,97 \\

\vspace{0.8mm}

  Markarian 38   & : Grubissich C., Becker W.             & 1980, Astron. Astrophys. Suppl. 40,367 \\

\vspace{0.8mm}

  Melotte 66     & : Hawarden T.G.                       & 1976, Mon. Not. R. Astr. Soc. 174,471 \\

\vspace{0.8mm}

  Melotte 101    & : Braes L.L.E.                        & 1962, Mon. Not. Astr. Soc. Sth. Afr. 21,16 \\

\vspace{0.8mm}

  Melotte 227    & : Epstein I.                          & 1968, Astron. J. 73,556  \\

\vspace{0.8mm}

  NGC 1252       & : Bouchet R., Th\'{e} P.S.             & 1983, Publ. Astr. Soc. Pacific 95,474  \\

\vspace{0.8mm}

  NGC 1901       & : Sanduleak N. et al.                 & 1968, Astron. J. 73,566 \\

\vspace{0.8mm}

  NGC 2287       & : Cox A.N.                            & 1954, Astrophys. J. 119,188 \\

\vspace{0.8mm}

  NGC 2354       & : D\"{u}rbeck W.                      & 1960, Z. Astrophys. 49,214 \\

\vspace{0.8mm}

  NGC 2362       & : Johnson H.L.                        & 1950, Astrophys. J. 112,240 \\

\vspace{0.8mm}

  NGC 2367       & : Vogt N., Moffat A.F.J.               & 1972, Astron. Astrophys. Suppl. 7,133 \\

\vspace{0.8mm}

  NGC 2383       & : Vogt N., Moffat A.F.J.               & 1972, Astron. Astrophys. Suppl. 7,133 \\

\vspace{0.8mm}

  NGC 2384       & : Vogt N., Moffat A.F.J.               & 1972, Astron. Astrophys. Suppl. 7,133 \\

\vspace{0.8mm}

  NGC 2439       & : White S.D.M.                        & 1975, Astrophys. J. 197,67 \\

\vspace{0.8mm}

  NGC 2447       & : Becker W.                            & 1959, Z. Astrophys. 48,279 \\

\vspace{0.8mm}

  NGC 2451       & : Williams P.M.                        & 1967, Mon. Not. Astr. Soc. Sth. Afr. 26,30 \\

\vspace{0.8mm}

  NGC 2467       & : Lod\'{e}n L.O.                       & 1966, Arkiv f\"{o}r Astronomi. Bd 4 nr 5,65 \\

\vspace{0.8mm}

  NGC 2477       & : Eggen O.J., Stoy R.H.                 & 1961, R. Obs. Bull. no 24 \\

\vspace{0.8mm}

  NGC 2482       & : Moffat A.F.J., Vogt N.                & 1975, Astron. Astrophys. Suppl. 20,85  \\

\vspace{0.8mm}

  NGC 2483       & : FitzGerald M.P., Moffat A.F.J.        & 1975, Astron. Astrophys. Suppl. 20,289 \\

\vspace{0.8mm}

  NGC 2489       & : Lindoff U., Johansson K.      & 1970, Arkiv f\"{o}r Astronomi. Bd 5 nr 3,45 \\

\vspace{0.8mm}

  NGC 2516       & : Dachs J. and Kabus H.         & 1989, Astron. Astrophys. Suppl.  78,25 \\

\vspace{0.8mm}

  NGC 2527       & : Lindoff U.                   & 1973, Astron. Astrophys. Suppl.  9,229 \\

\vspace{0.8mm}

  NGC 2533       & : Lindoff U.                   & 1968, Arkiv f\"{o}r Astronomi. Bd 4 nr 39,587 \\

\vspace{0.8mm}

  NGC 2546       & : Lindoff U.                   & 1968, Arkiv f\"{o}r Astronomi. Bd 5 nr 4,63 \\

\vspace{0.8mm}

  NGC 2547       & : Clari\'{a} J.J.                  & 1982, Astron. Astrophys. Suppl.  47,323 \\

\vspace{0.8mm}

  NGC 2567       & : Lindoff U.                   & 1968, Arkiv f\"{o}r Astronomi. Bd 4 nr 39,587 \\

\vspace{0.8mm}

  NGC 2571       & : Lindoff U.                   & 1968, Arkiv f\"{o}r Astronomi. Bd 4 nr 39,587 \\

\vspace{0.8mm}

  NGC 2579       & : Lindoff U.                   & 1968, Arkiv f\"{o}r Astronomi. Bd 5 nr 4,63 \\

\vspace{0.8mm}

  NGC 2669       & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl. 9,97 \\

\vspace{0.8mm}

  NGC 2670       & : Lyng{\aa} G.                     & 1962, Arkiv f\"{o}r Astronomi. Bd 2 nr 34,379 \\

\vspace{0.8mm}

  NGC 2910       & : Topaktas L.                  & 1981, Astron. Astrophys. Suppl. 45,111 \\

\vspace{0.8mm}

  NGC 2925       & : Topaktas L.                  & 1981, Astron. Astrophys. Suppl. 45,111 \\

\vspace{0.8mm}

  NGC 3033       & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl. 9,97 \\

\vspace{0.8mm}

  NGC 3114       & : Jankowitz N.E., Mc Cosh C.J.  & 1963, Mon. Not. Astr. Soc. Sth. Afr. 22,1 \\

\vspace{0.8mm}

  NGC 3228       & : Th\'{e} P.S. et al.              & 1974, Astron. Astrophys. Suppl. 15,141 \\

\vspace{0.8mm}

  NGC 3293       & : Turner D.E. et al.           & 1980, Astron. J. 85,1193 \\

\end{tabular}
\newpage
\begin{tabular}{lll}

  NGC 3324       & : Clari\'{a} J.J.                  & 1977, Astron. Astrophys. Suppl. 27,145 \\

\vspace{0.9mm}

  NGC 3330       & : Becker W.                    & 1960, Z. Astrophys. 49,168 \\

\vspace{0.8mm}

  NGC 3496       & : Sher D.                      & 1965, Mon. Not. R. Astr. Soc. 129,237 \\

\vspace{0.8mm}

  NGC 3532       & : Fern\'{a}ndez J.A., Salgado C.W.  & 1980, Astron. Astrophys. Suppl. 39,11 \\

\vspace{0.8mm}

  NGC 3572       & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  NGC 3590       & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  NGC 3680       & : Eggen O.J.                   & 1969, Astrophys. J. 155,439 \\

\vspace{0.8mm}

  NGC 3766       & : Ahmed F.                     & 1962, Publ. R. Obs. Edinburgh 3,60 \\

\vspace{0.8mm}

  NGC 4052       & : Engver N.                    & 1965, Arkiv f\"{o}r Astronomi. Bd 4 nr 4,53 \\

\vspace{0.8mm}

  NGC 4103       & : Wesselink A.J.               & 1969, Mon. Not. R. Astr. Soc. 146,329 \\

\vspace{0.8mm}

  NGC 4337       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 4349       & : Lohmann W.                   & 1961, Astr. Nach. 286,105 \\

\vspace{0.8mm}

  NGC 4439       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 4463       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 4609       & : Feinstein A., Marraco H.G.    & 1971, Publ. Astr. Soc. Pacific 83,218 \\

\vspace{0.8mm}

  NGC 4755       & : Arp H., Van Sant C.T.         & 1958, Astron. J. 63,341 \\

\vspace{0.8mm}

  NGC 5138       & : Lindoff U.                   & 1972, Astron. Astrophys. Suppl. 7,231 \\

\vspace{0.8mm}

  NGC 5281       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 5316       & : Rahim M.A.                   & 1966, Astr. Nach. 289,41 \\

\vspace{0.8mm}

  NGC 5460       & : Clari\'{a} J.J.                  & 1971, Astron. J. 76,639 \\

\vspace{0.8mm}

  NGC 5606       & : Lyng{\aa} G.                     & 1964, Medd. Lunds Astr. Obs. 2 no 139  \\

\vspace{0.8mm}

  NGC 5617       & : Lindoff U.                   & 1967, Arkiv f\"{o}r Astronomi. Bd 4 nr 32,471 \\

\vspace{0.8mm}

  NGC 5662       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 5749       & : Lyng{\aa} G.                     & 1964, Medd. Lunds Astr. Obs. 2 no 139 \\

\vspace{0.8mm}

  NGC 5822       & : Bozkurt S.                   & 1974, Rev. Mex. Astron. Astrofis. 1,89 \\

\vspace{0.8mm}

  NGC 5823       & : Br\"{u}ck M.T. et al.            & 1968, Publ. R. Obs. Edinburgh 6 no 9 \\

\vspace{0.8mm}

  NGC 6025       & : Feinstein A.                 & 1971, Publ. Astr. Soc. Pacific 83,800 \\

\vspace{0.8mm}

  NGC 6067       & : Thackeray A.D. et al.        & 1962, Mon. Not. R. Astr. Soc. 124,445 \\

\vspace{0.8mm}

  NGC 6087       & : Fernie J.D.                  & 1961, Astrophys. J. 133,64 \\

\vspace{0.8mm}

  NGC 6124       & : Koelbloed D.                 & 1959, Bull. Astr. Inst. Netherl. 14, No 489,265 \\

\vspace{0.8mm}

  NGC 6134       & : Lindoff U.                   & 1972, Astron. Astrophys. Suppl. 7,231 \\

\vspace{0.8mm}

  NGC 6167       & : Br\"{u}ck M.T., Smyth M.J.        & 1966, Publ. R. Obs. Edinburgh 5,195 \\

\vspace{0.8mm}

  NGC 6169       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6178       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6193       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6200       & : FitzGerald M.P., Jackson P.D. & 1977, Observatory 97,129 \\

\vspace{0.8mm}

  NGC 6204       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6208       & : Lindoff U.                   & 1972, Astron. Astrophys. Suppl. 7,231 \\

\vspace{0.8mm}

  NGC 6231       & : Seggewiss W.                 & 1968, Ver\"{o}eff. Astr. Univ. Bonn no 79 \\

\vspace{0.8mm}

  NGC 6242       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6249       & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  NGC 6250       & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,155 \\

\vspace{0.8mm}

  NGC 6281       & : Feinstein A., Forte J.C.      & 1974, Publ. Astr. Soc. Pacific 86,284 \\

\vspace{0.8mm}

  NGC 6322       & : Lohmann W., Schnur G.         & 1972, Astr. Nach. 287,17 \\

\vspace{0.8mm}

  NGC 6383       & : Evans T.L.                   & 1978, Mon. Not. R. Astr. Soc. 184,661 \\

\end{tabular}
\newpage
\begin{tabular}{lll}

  NGC 6405       & : Rohlfs K. et al.             & 1959, Z. Astrophys. 47,15 \\

\vspace{0.9mm}

  NGC 6416       & : Th\'{e} P.S., Stokes N.           & 1970, Astron. Astrophys. Suppl.  5,298 \\

\vspace{0.8mm}

  NGC 6425       & : Th\'{e} P.S., Stokes N.           & 1970, Astron. Astrophys. Suppl.  5,298 \\

\vspace{0.8mm}

  NGC 6475       & : Koelbloed D.                 & 1959, Bull. Astr. Inst. Netherl. 14, No 489,265 \\

\vspace{0.8mm}

  NGC 6494       & : Hoag A.A. et al.             & 1961, Publ. US Nav. Obs. 17,347 \\

\vspace{0.8mm}

  NGC 6514       & : Ogura K., Ishida K.           & 1975, Publ. Astr. Soc. Japan 27,119 \\

\vspace{0.8mm}

  NGC 6530       & : Kilambi G.C.                 & 1977, Mon. Not. R. Astr. Soc. 178,423 \\

\vspace{0.8mm}

  NGC 6531       & : Hoag A.A. et al.             & 1961, Publ. US Nav. Obs. 17,347 \\

\vspace{0.8mm}

  NGC 6546       & : Grayzeck E.J. et al.         & 1978, Publ. Astr. Soc. Pacific 90,742 \\

\vspace{0.8mm}

  NGC 6716       & : Lindoff U.                   & 1971, Astron. Astrophys. 15,439 \\

\vspace{0.8mm}

  Pismis 4       & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,85  \\

\vspace{0.8mm}

  Pismis 5       & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  9,97 \\

\vspace{0.8mm}

  Pismis 6       & : FitzGerald H.P. et al.       & 1979, Astron. Astrophys. Suppl. 37,351 \\

\vspace{0.8mm}

  Pismis 11      & : Moffat A.F.J., FitzGerald M.P.& 1977, Astron. Astrophys. 54,263 \\

\vspace{0.8mm}

  Pismis 12      & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,85  \\

\vspace{0.8mm}

  Pismis 13      & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  9,97 \\

\vspace{0.8mm}

  Pismis 16      & : Topaktas L., Fenkart R.P.     & 1982, Astron. Astrophys. Suppl. 49,475 \\

\vspace{0.8mm}

  Pismis 18      & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Pismis 20      & : Lyng{\aa} G.                 & 1964, Medd. Lunds Astr. Obs. 2 no 139  \\

\vspace{0.8mm}

  Pismis 21      & : Moffat A.F.J., FitzGerald M.P.& 1977, Astron. Astrophys. 54,263 \\

\vspace{0.8mm}

  Pismis 24      & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135 \\

\vspace{0.8mm}

  Ruprecht 20    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  7,133 \\

\vspace{0.8mm}

  Ruprecht 32    & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,85 \\

\vspace{0.8mm}

  Ruprecht 36    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  7,133 \\

\vspace{0.8mm}

  Ruprecht 47    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  7,133 \\

\vspace{0.8mm}

  Ruprecht 49    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  7,133 \\

\vspace{0.8mm}

  Ruprecht 55    & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,85 \\

\vspace{0.8mm}

  Ruprecht 59    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  7,133 \\

\vspace{0.8mm}

  Ruprecht 76    & : Vogt N., Moffat A.F.J.        & 1972, Astron. Astrophys. Suppl.  9,97 \\

\vspace{0.8mm}

  Ruprecht 78    & : Topaktas L., Fenkart R.P.     & 1982, Astron. Astrophys. Suppl. 49,475 \\

\vspace{0.8mm}

  Ruprecht 82    & : Topaktas L.                  & 1981, Astron. Astrophys. Suppl. 45,111 \\

\vspace{0.8mm}

  Ruprecht 92    & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  Ruprecht 93    & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  Ruprecht 97    & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Ruprecht 98    & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135  \\

\vspace{0.8mm}

  Ruprecht 108   & : Moffat A.F.J., Vogt N.        & 1973, Astron. Astrophys. Suppl. 10,135  \\

\vspace{0.8mm}

  Ruprecht 127   & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,155 \\

\vspace{0.8mm}

  Sher 1         & : Moffat A.F.J., Vogt N.        & 1975, Astron. Astrophys. Suppl. 20,125 \\

\vspace{0.8mm}

  Stock 13       & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  Stock 14       & : Peterson C. J. et al.        & 1988, Mon. Not. R. Astr. Soc. 235,1439 \\

\vspace{0.8mm}

  Stock 16       & : Fenkart R.P. et al.          & 1977, Astron. Astrophys. Suppl. 30,307 \\

\vspace{0.8mm}

  Tombaugh 1     & : Turner D.G.                  & 1983, J. R. Astron. Soc. Can. 77,31 \\

\vspace{0.8mm}

  Trumpler 9     & : Pismis P.                    & 1970, Bol. Obs. Tonantzintia Tacubaya 35,293 \\

\vspace{0.8mm}

  Trumpler 10    & : Lyng{\aa} G.                     & 1959, Arkiv f\"{o}r Astronomi. Bd 2 nr 34,379 \\

\vspace{0.8mm}

  Trumpler 12    & : Lindoff U.                   & 1967, Arkiv f\"{o}r Astronomi. Bd 4 nr 32,471 \\

\end{tabular}
\newpage
\begin{tabular}{lll}

  Trumpler 14    & : Feinstein A. et al.          & 1973, Astron. Astrophys. Suppl. 12,331 \\

\vspace{0.9mm}

  Trumpler 15    & : Feinstein A. et al.          & 1980, Astron. J. 85,708 \\

\vspace{0.8mm}

  Trumpler 16    & : Th\'{e} P.S. et al.              & 1980, Astron. Astrophys. Suppl. 41,93 \\

\vspace{0.8mm}

  Trumpler 17    & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  Trumpler 18    & : Steppe H.                    & 1977, Astron. Astrophys. Suppl. 27,415 \\

\vspace{0.8mm}

  Trumpler 21    & : Peterson C.J. et al.         & 1988, Mon. Not. R. Astr. Soc. 235,1439 \\

\vspace{0.8mm}

  Trumpler 22    & : Lindoff U.                   & 1967, Arkiv f\"{o}r Astronomi. Bd 4 nr 33,493 \\

\vspace{0.8mm}

  Trumpler 27    & : Moffat A.F.J. et al.         & 1977, Astrophys. J. 215,106 \\

\vspace{0.8mm}

  Trumpler 28    & : Th\'{e} P.S., Stokes N.      & 1970, Astron. Astrophys. Suppl.  5,298 \\

\vspace{0.8mm}

  Trumpler 33    & : Grubissich C.                & 1964, Z. Astrophys. 58,276 \\

\end{tabular}

\vspace{10.mm}
\centering{\underline{\bf{Notes }}}

\vspace{3.mm}

Hogg 16 = Basel 19	          \\
Markarian 18 = Collinder 205         \\

\vspace{10.mm}

\begin{center}
\underline{\bf{Abbreviations used }}
\end{center}

\vspace{3.mm}

\begin{tabular}{l@{\hspace{30.mm}}l@{\hspace{30.mm}}l}
Bas = Basel     & Hog = Hogg      & Pis = Pismis \\
Bla = Blanco    & Lod = Lod\'{e}n & Rup = Ruprecht \\
Boc = Bochum    & Lyn = Lyng{\aa} & Sto = Stock \\
Col = Collinder & Mrk = Markarian & Tom = Tombaugh \\
Fei = Feinstein & Mel = Melotte   & Tru = Trumpler \\
\end{tabular}


\newpage
\begin{center}
\vspace{20.mm}
\Large{\underline{\bf{ANNEX V}}} \\[40.mm]
\large{\framebox(120,10){\bf{Notes (Stars indicated by a *) }}} \\[40.mm]
\end{center}

\begin{tabular}{rp{125.mm}}

   594 & SAO 255642 = HD 661 + HD 662 (spectroscopic binary)                                                \\

\vspace{1.mm}

   736 & Is also BPM 46113                                                                                  \\

\vspace{1.mm}

  1507 & Variable eta Scl                                                                                 \\

\vspace{1.mm}

  1796 & Variable teta Tuc                                                                                \\

\vspace{1.mm}

  1821 & The CPC 18 153a identifier is unrelated to the duplicity of the star. It is a supplementary number added to the series
         of running numbers by the authors of the CPC 18 catalogue. \\

\vspace{1.mm}

  2004 & Is also PLX 104                                                                                    \\

\vspace{1.mm}

  2254 & Variable ksi Phe                                                                                     \\

\vspace{1.mm}

  2735 & Variable rho Phe                                                                                     \\

\vspace{1.mm}

  3472 & Is also RMC 39                                                                                     \\

\vspace{1.mm}

  3606 & Variable zeta Phe                                                                                \\

\vspace{1.mm}

  3785 & Is also PHL 1003                                                                                   \\

\vspace{1.mm}

  3944 & SAO 248345 = IDS 01124-6924B with a magnitude of 7.3V was not observed since it is too near. \\

\vspace{1.mm}

  4532 & Variable gamma Phe                                                                                   \\

\vspace{1.mm}

  4874 & Read IDS 01304-3026ABC                                                                               \\

\vspace{1.mm}

  5075 & Is also G 272-61 : The sighted object is the sum of : LHS 9 and LHS 10;  \\
       & L 726 -8A and L 726 -8B; LP 768 -26 and LP 768 -27; LTT 892 and LTT 893;  \\
       & GJ 65A and GJ 65B; LFT 144 and LFT 145.                                             \\

\vspace{1.mm}

  5114 & SAO 232490 = HD 10360 + HD 10361                                                                     \\

\vspace{1.mm}

  5115 & See previous note \\

\vspace{1.mm}

  5549 & Is also BPM 47357                                                                                  \\

\vspace{1.mm}

  5765 & Variable eta 01 Hyi                                                                              \\

\vspace{1.mm}

  5827 & Variable psi Phe                                                                                     \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

  6300 & Variable nu For                                                                                      \\

\vspace{1.3mm}

  7287 & Is also LTT 1230                                                                                   \\

\vspace{1.mm}

  8796 & Is also Ci 20 211 and PLX 664                                                                       \\

\vspace{1.mm}

  8812 & Is close to 8813, however the distance varies rapidly :
         31" in 1950, 26" in 1975, 53" in 2000 (minimum : 23" around 1966) \\

\vspace{1.mm}

  8813 & See previous note \\

\vspace{1.mm}

  9065 & Variable tau 04 Eri                                                                                  \\

\vspace{1.mm}

  9080 & Is also Ci 20 227                                                                                  \\

\vspace{1.mm}

  9530 & CD-26 1339 = CD-26 1340 = PHL 1556 = ESO 482 -7                                                      \\

\vspace{1.mm}

 10034 & Is also UBV 3627                                                                                   \\

\vspace{1.mm}

 10155 & CPD-54 599 = HD 24185 + HD 24186 (spectroscopic binary) \\

\vspace{1.mm}

 10618 & Variable tau 09 Eri                                                                                  \\

\vspace{1.mm}

 10674 & Variable gamma Ret                                                                                   \\

\vspace{1.mm}

 11301 & Variable gamma Dor                                                                                   \\

\vspace{1.mm}

 11539 & Is also PLX 966                                                                                    \\

\vspace{1.mm}

 11805 & The star located 1' to the south seems to be LTT 1995 = L 663 -20 (not included) \\

\vspace{1.mm}

 12014 & Variable alpha Dor                                                                                   \\

\vspace{1.mm}

 12239 & Is also UBV 4538                                                                                   \\

\vspace{1.mm}

 12804 & Is also ARDB 40                                                                                    \\

\vspace{1.mm}

 12814 & Is also ARDB 39                                                                                    \\

\vspace{1.mm}

 12894 & Is also ARDB 53                                                                                    \\

\vspace{1.mm}

 12899 & Is also ARDB 57                                                                                    \\

\vspace{1.mm}

 12909 & Is also ARDB 61                                                                                    \\

\vspace{1.mm}

 12949 & Located in a cluster in the Large Magellanic Cloud \\

\vspace{1.mm}

 13005 & Is also ARDB 79                                                                                    \\

\vspace{1.mm}

 13153 & Is also ARDB 103                                                                                   \\

\vspace{1.mm}

 13239 & Is also LTT 2151                                                                                   \\

\vspace{1.mm}

 13342 & Is also ARDB 122                                                                                   \\

\vspace{1.mm}

 13481 & Is also ARDB 141                                                                                   \\

\vspace{1.mm}

 13524 & Is also ARDB 147                                                                                   \\

\vspace{1.mm}

 13568 & Is also ARDB 151                                                                                   \\

\vspace{1.mm}

 13584 & Is also ARDB 154                                                                                   \\

\vspace{1.mm}

 13686 & Kapteyn star                                                                                   \\

\vspace{1.mm}

 13950 & Is also ARDB 184                                                                                   \\

\vspace{1.mm}

 13974 & Is also ARDB 185                                                                                   \\

\vspace{1.mm}

 14203 & In NGC 1925                                                                                        \\

\vspace{1.mm}

 14208 & In NGC 1925                                                                                        \\

\vspace{1.mm}

 14223 & Is also ARDB 203                                                                                   \\

\vspace{1.mm}

 14263 & Is also ARDB 210                                                                                   \\

\vspace{1.mm}

 14275 & Is also ARDB 212                                                                                   \\

\vspace{1.mm}

 14290 & Is also ARDB 213                                                                                   \\

\vspace{1.mm}

 14408 & Is also ARDB 225                                                                                   \\

\vspace{1.mm}

 14551 & Is also ARDB 246                                                                                   \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 14650 & Is also ARDB 262                                                                                   \\

\vspace{1.3mm}

 14672 & Is also ARDB 260                                                                                   \\

\vspace{1.mm}

 14700 & Is also ARDB 265                                                                                   \\

\vspace{1.mm}

 14730 & Is also ARDB 272                                                                                   \\

\vspace{1.mm}

 14745 & Is also ARDB 271                                                                                   \\

\vspace{1.mm}

 14942 & Variable beta Dor                                                                                \\

\vspace{1.mm}

 15063 & Is also ARDB 318                                                                                   \\

\vspace{1.mm}

 15066 & Variable iota Men                                                                                    \\

\vspace{1.mm}

 15183 & Is also ARDB 334                                                                                   \\

\vspace{1.mm}

 15325 & Is also ARDB 341                                                                                   \\

\vspace{1.mm}

 15330 & Is also ARDB 340                                                                                   \\

\vspace{1.mm}

 15341 & Has several companions that are not separate \\

\vspace{1.mm}

 15551 & Is also ARDB 367                                                                                   \\

\vspace{1.mm}

 15661 & Is also ARDB 375                                                                                   \\

\vspace{1.mm}

 15748 & Is also ARDB 381                                                                                   \\

\vspace{1.mm}

 15777 & Is also ARDB 385                                                                                   \\

\vspace{1.mm}

 16008 & Star observed in a nebulosity. According to HDE, the spectrum is continuous. \\

\vspace{1.mm}

 16337 & Variable lambda Col   \\

\vspace{1.mm}

 16375 & Is also ARDB 400                                                                                   \\

\vspace{1.mm}

 16788 & Is also LTT 2431. Read : IDS 05566-3103ABC                                                         \\

\vspace{1.mm}

 17447 & Variable delta Pic                                                                                   \\

\vspace{1.mm}

 17540 & According to HIC, L 452 -2 is CD-35 2744, at 46" North of CD-35 2745 \\
       & According to Luyten, L 452 -2 = LTT 2481 = CD-35 2745                                                       \\

\vspace{1.mm}

 17544 & See previous note \\

\vspace{1.mm}

 18269 & Is also IRC -30060                                                                                 \\

\vspace{1.mm}

 18795 & Variable ksi 01 CMa                                                                                  \\

\vspace{1.mm}

 19624 & The companion IDS 06387-3754B was not observed \\

\vspace{1.mm}

  19625 & See previous note \\

\vspace{1.mm}

 19967 & Is NGC 2287 1 : Lod\'{e}n L.O. (1957, Arkiv f\"{o}r Astronomi. Bd 2 nr 5,39) \\

\vspace{1.mm}

 19970 & Is NGC 2287 8 : Lod\'{e}n L.O. (1957, Arkiv f\"{o}r Astronomi. Bd 2 nr 5,39) \\

\vspace{1.mm}

 19987 & Is also BD-20 1555                                                                                 \\

\vspace{1.mm}

 20094 & Is also BD-20 1576                                                                                 \\

\vspace{1.mm}

 20343 & Variable kappa CMa                                                                                   \\

\vspace{1.mm}

 20674 & Variable omicron 01 CMa                                                                              \\

\vspace{1.mm}

 20803 & Is also BD-22 1602                                                                                 \\

\vspace{1.mm}

 20903 & Two companions were observed with magnitudes of 14 (20904 and 20905) instead of the single companion,
         with a magnitude of 12, described in the IDS \\

\vspace{1.mm}

 21163 & IDS 06558-2235A = SAO 172722 was not measured \\

\vspace{1.mm}

 21337 & Variable sigma CMa                                                                                   \\

\vspace{1.mm}

 21505 & Arbitrary identification. ADS only mentions one companion, whilst CDS mentions two.
         The included object is therefore B or C or the sum of both. \\

\vspace{1.mm}

 22534 & Variable omega CMa                                                                               \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 23734 & Is also BD-22 1855                                                                                 \\

\vspace{1.3mm}

 23833 & Is also UBV M 32507                                                                                \\

\vspace{1.mm}

 24683 & SAO 235287 was observed as an inseparable binary. \\

\vspace{1.mm}

 24936 & SAO 256428 = HD 62153 + HD 62154                                                                     \\

\vspace{1.mm}

 25060 & Is also VDB 98 \\

\vspace{1.mm}

 25298 & Is also LF 12 36                                                                                   \\

\vspace{1.mm}

 25884 & Is also LF 12 73                                                                                   \\

\vspace{1.mm}

 25935 & Is also LF 12 76                                                                                   \\

\vspace{1.mm}

 26539 & Is also LF 12 112                                                                                  \\

\vspace{1.mm}

 26900 & Is also BD-22 2058                                                                                 \\

\vspace{1.mm}

 27083 & Is also LF 12 150                                                                                  \\

\vspace{1.mm}

 27482 & SAO 219184  = HD 65461 + HD 65462 (spectroscopic binary) \\

\vspace{1.mm}

 27516 & Is also NGC 2516 3 : Cox  A.N. (1955, Astrophys. J. 121,628) \\

\vspace{1.mm}

 27534 & Is also NGC 2516 101 : Cox  A.N. (1955, Astrophys. J. 121,628) \\

\vspace{1.mm}

 27561 & Is NGC 2516 230 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27575 & Is also NGC 2516 96 : Cox  A.N. (1955, Astrophys. J. 121,628) \\

\vspace{1.mm}

 27607 & Is NGC 2516 407 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27618 & Is also LTT 3021, UBV 7702 \\

\vspace{1.mm}

 27659 & Is NGC 2516 36 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27674 & Is NGC 2516 919 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27706 & Is also LS 896                                                                                     \\

\vspace{1.mm}

 27709 & Is also NGC 2516 60 : Cox A.N. (1955, Astrophys. J. 121,628) \\

\vspace{1.mm}

 27717 & Is NGC 2516 937 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27739 & Is NGC 2516 912 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 27824 & Is NGC 2516 710 : Dachs J. and Kabus H. (1989, Astron. Astrophys. Suppl. 78,25) \\

\vspace{1.mm}

 28012 & Is also NGC 2516 29 : Cox  A.N. (1955, Astrophys. J. 121,628) \\

\vspace{1.mm}

 28227 & IDS 07589-3056B was not observed \\

\vspace{1.mm}

 28630 & Sum of HD 67417 and HD 67418 \\

\vspace{1.mm}

 28820 & Variable rho Pup                                                                                     \\

\vspace{1.mm}

 29069 & Variable gamma 02 Vel                                                                                \\

\vspace{1.mm}

 29102 & SAO 175293  = HD 68022 + HD 68023 (spectroscopic binary) \\

\vspace{1.mm}

 32089 & Is also VDBH 17a, NGC 2626 and LS 1097 \\

\vspace{1.mm}

 32486 & Is also LTT 3202                                                                                   \\

\vspace{1.mm}

 32612 & Variable omicron Vel                                                                                 \\

\vspace{1.mm}

 32886 & Precedes 32887 by 7.5" \\

\vspace{1.mm}

 32887 & Follows 32886 by 7.5" \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 34260 & Is also VDBH 25c \\

\vspace{1.3mm}

 35111 & Variable lambda Vel                                                                                  \\

\vspace{1.mm}

 35380 & Is also BPM 34020                                                                                  \\

\vspace{1.mm}

 36028 &  Is also UBV 8918                                                                                  \\

\vspace{1.mm}

 37703 & Variable zeta Cha                                                                                \\

\vspace{1.mm}

 37955 & The sum of HD 83386A and B (IDS 09329-4735AB) is possibly PLX 2286 \\

\vspace{1.mm}

 37956 & See previous note \\

\vspace{1.mm}

 38605 & Is also ESO 167 -3 and He 2 -36. Position inaccurate \\

\vspace{1.mm}

 38691 & SAO 177908 = GJ 366.1A + GJ 366.1B                                                                   \\

\vspace{1.mm}

 38774 & IDS 09412-4933B = CPD-49 2746B = CD-49 4652B may correspond to the star 38774 or 38775 or the sum of both stars. \\

\vspace{1.mm}

 38775 & See previous note \\

\vspace{1.mm}

 39536 & CD-83 151 = CPC 22 1225 + CPC 22 1226                                                                \\

\vspace{1.mm}

 39548 & See previous note \\

\vspace{1.mm}

 40389 & Is also NGC 3114 184 : Lyng{\aa} (1962, Arkiv f\"{o}r Astronomi. Bd 3 nr 8,65) \\

\vspace{1.mm}

 40668 & Is also NGC 3114 136 : Lyng{\aa} (1962, Arkiv f\"{o}r Astronomi. Bd 3 nr 8,65) \\

\vspace{1.mm}

 40741 & Is also NGC 3114 163 : Lyng{\aa} (1962, Arkiv f\"{o}r Astronomi. Bd 3 nr 8,65) \\

\vspace{1.mm}

 40831 & Is also NGC 3114 33 : Lyng{\aa} (1962, Arkiv f\"{o}r Astronomi. Bd 3 nr 8,65) \\

\vspace{1.mm}

 40880 & Is also LF 13 4                                                                                    \\

\vspace{1.mm}

 40924 & Is also LF 13 7                                                                                    \\

\vspace{1.mm}

 41059 & CPD-56 2884 and CPD-56 2885 are without doubt the same star \\

\vspace{1.mm}

 41543 & Is also LF 13 41                                                                                   \\

\vspace{1.mm}

 41574 & Is also LF 13 45                                                                                   \\

\vspace{1.mm}

 41614 & Is also LF 13 48                                                                                   \\

\vspace{1.mm}

 41701 & Is also L 101 -52                                                                                  \\

\vspace{1.mm}

 41827 & Is also LF 13 62                                                                                   \\

\vspace{1.mm}

 41865 & Is also LF 13 64                                                                                   \\

\vspace{1.mm}

 41880 & Is also LF 13 65                                                                                   \\

\vspace{1.mm}

 42090 & Is also LF 13 77                                                                                   \\

\vspace{1.mm}

 42372 & Is also BPM 35015                                                                                  \\

\vspace{1.mm}

 42379 & Is also LF 13 90                                                                                   \\

\vspace{1.mm}

 42703 & Is also LF 13 106                                                                                  \\

\vspace{1.mm}

 42957 & Is also LF 13 118                                                                                  \\

\vspace{1.mm}

 42997 & Is also LS 1588                                                                                    \\

\vspace{1.mm}

 43065 & HD 300774 was observed as an inseparable binary. \\

\vspace{1.mm}

 43198 & Is also LF 13 126                                                                                  \\

\vspace{1.mm}

 43237 & Is also LF 13 127                                                                                  \\

\vspace{1.mm}

 43312 & Is also L 681 -12                                                                                  \\

\vspace{1.mm}

 43384 & Is also L 681 -21                                                                                  \\

\vspace{1.mm}

 43431 & Is also LF 13 143                                                                                  \\

\vspace{1.mm}

 43432 & Occasionally named HD 91324B \\

\vspace{1.mm}

 43453 & Is also LF 13 144    \\

\vspace{1.mm}

 43545 & Is also LF 13 150                                                                                  \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 43658 & Is also VDBH 40c                                                                                   \\

\vspace{1.3mm}

 43695 & Is also LF 13 156                                                                                  \\

\vspace{1.mm}

 43704 & Is also LF 13 158                                                                                  \\

\vspace{1.mm}

 44809 & Doubt whether it is CD-61 2773 or CD-61 2774 \\

\vspace{1.mm}

 44956 & Is also LS 1844                                                                                    \\

\vspace{1.mm}

 44996 & Is also LS 1854                                                                                    \\

\vspace{1.mm}

 45061 & Variable eta Car                                                                                 \\

\vspace{1.mm}

 45065 & Is also LS 1870                                                                                    \\

\vspace{1.mm}

 45103 & Is also LS 1874                                                                                    \\

\vspace{1.mm}

 45118 & Is also LS 1878                                                                                    \\

\vspace{1.mm}

 45157 & Is also L 753 -52                                                                                  \\

\vspace{1.mm}

 45358 & CPC 20.1 2944 = CPC 20 3161                                                                          \\

\vspace{1.mm}

 45368 & HD 305612 = LS 1911 designated in the Bochum 11 cluster, the sum of Boc 11 2, Boc 11 5 and Boc 11 6
         (since the latter was not measured for this catalogue) \\

\vspace{1.mm}

 45369 & See previous note \\

\vspace{1.mm}

 46029 & Is also LTT 3994                                                                                   \\

\vspace{1.mm}

 46045 & SAO 256770 = HD 94650 + HD 94651                                                                     \\

\vspace{1.mm}

 46074 & Is also PK 288-00 1 .Nebula \\

\vspace{1.mm}

 47460 & Variable khi 02 Hya                                                                                  \\

\vspace{1.mm}

 48044 & Is also LS 2211                                                                                    \\

\vspace{1.mm}

 48466 & This is not IDS 11100-5129B. The latter, with a magnitude of 12.4, was observed but was too faint and too close to the
          main object (48465) to be sighted \\

\vspace{1.mm}

 48553 & SAO 251334 = HD 98027 + HD 98028 (spectroscopic binary) \\

\vspace{1.mm}

 49453 & CPC 20.1 3176 = LHS 2402 = GJ 428A + GJ 428B                                                         \\

\vspace{1.mm}

 49456 & See previous note \\

\vspace{1.mm}

 49975 & Is also UBV 10403 \\

\vspace{1.mm}

 50097 & Variable omicron 01 Cen                                                                              \\

\vspace{1.mm}

 50107 & Variable omicron 02 Cen                                                                              \\

\vspace{1.mm}

 50902 & SAO 251522 = HD 101379 + HD 101380 (spectroscopic binary) \\

\vspace{1.mm}

 51460 & Is also PLX 2716 and possibly LS 2481 \\

\vspace{1.mm}

 51542 & Is also LF 14 2                                                                                    \\

\vspace{1.mm}

 51742 & Variable mu Mus                                                                                      \\

\vspace{1.mm}

 51831 & Is also LF 14 13                                                                                   \\

\vspace{1.mm}

 51889 & Is also LF 14 17                                                                                   \\

\vspace{1.mm}

52107 & Variable beta Hya                                                                                \\

\vspace{1.mm}

 52118 & Occasionally called HD 103224B or CPD-63 2021B. Is possibly HD 310896 \\

\vspace{1.mm}

 52249 & Is also UBV 10699                                                                                  \\

\vspace{1.mm}

 52387 & Precedes (32") HD 103653 = CPD-62 2436 = LF 14 42 = UBV M 17522 = GCRV 21393.
         Mag. : 10.11V; Sp. : B9; Observed on 04/05/1975 = 1975.34  at : \\
       & 11h 53m 33s.255 \(-62^{o}\)  39' 24".71 (1950.0)      0.24"  0.45"                                   \\
       & 11h 56m 04s.000 \(-62^{o}\)  56' 06".47 (2000.0)                                                     \\

\vspace{1.mm}

 52414 & Is also LF 14 44                                                                                   \\

\vspace{1.mm}

 52550 & Is also LF 14 54                                                                                   \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 52607 & Is also LF 14 56                                                                                   \\

\vspace{1.3mm}

 52869 & Is also UBV 10783                                                                                  \\

\vspace{1.mm}

 52899 & SAO 239600 = HD 104533 + HD 104534 (spectroscopic binary) \\

\vspace{1.mm}

 53072 & Variable teta 02 Cru                                                                             \\

\vspace{1.mm}

 53272 & Is also LS 2590                                                                                    \\

\vspace{1.mm}

 53297 & Is also LF 14 94                                                                                   \\

\vspace{1.mm}

 53328 & Is also LS 2596                                                                                    \\

\vspace{1.mm}

 53427 & CD-60 3992 and CD-60 3993 are without doubt the same star \\

\vspace{1.mm}

 53462 & Variable delta Cen                                                                                   \\

\vspace{1.mm}

 53750 & This is not IDS 12066-5316B. The latter, with a magnitude of 13.2, was observed but was too faint and too near the
         main object (53749) to be sighted  \\

\vspace{1.mm}

 54055 & Variable delta Cru                                                                                   \\

\vspace{1.mm}

 54254 & Variable epsilon Mus                                                                                 \\

\vspace{1.mm}

 54286 & Read : IDS 12127-2327ABC                                                                             \\

\vspace{1.mm}

 54312 & Is also LF 14 142. This star should not be used as a photometric standard since it is variable. \\

\vspace{1.mm}

 54594 & SAO 251863 = HD 107463 + HD 107464 (spectroscopic binary) \\

\vspace{1.mm}

 54879 & Is also GCRV 4337 E                                                                                \\

\vspace{1.mm}

 54896 & SAO 251884 = HD 107979 + HD 107980 (spectroscopic binary) \\

\vspace{1.mm}

 55442 & Is possibly IRAS 12277-6319                                                                    \\

\vspace{1.mm}

 55822 & Appears to have a very close companion in addition to IDS 12287-6721B \\

\vspace{1.mm}

 56054 & Variable alpha Mus                                                                                   \\

\vspace{1.mm}

 56467 & Is the sum of 3 components that are not separate \\

\vspace{1.mm}

 56509 & This is not IDS 12364-5554B. The latter, with a magnitude of 14.3, was observed but was too faint and too near the
         main object (56508) to be sighted \\

\vspace{1.mm}

 57172 & Is also IRC -20245                                                                                 \\

\vspace{1.mm}

 57410 & Appears to be a galaxy \\

\vspace{1.mm}

 57411 & Appears to be a galaxy \\

\vspace{1.mm}

 57768 & Variable mu 02 Cru                                                                                   \\

\vspace{1.mm}

 57770 & Variable lambda Cru                                                                                  \\

\vspace{1.mm}

 58277 & Very close to the NGC 4833 cluster \\

\vspace{1.mm}

 58682 & Is also UBV 11784                                                                                  \\

\vspace{1.mm}

 59115 & Variable teta Mus                                                                                \\

\vspace{1.mm}

 59502 & SAO 240645 is made up of 3 stars that are not separate. See IDS 13060-5923ABC \\

\vspace{1.mm}

 59809 & Variable eta Mus                                                                                 \\

\vspace{1.mm}

 60186 & Is also VDBH 60a                                                                                   \\

\vspace{1.mm}

 61054 & Is also Bas 19 19                                                                                  \\

\vspace{1.mm}

 61060 & Is also Bas 19 20                                                                                  \\

\vspace{1.mm}

 61067 & Is also Bas 19 21                                                                                  \\

\vspace{1.mm}

 61094 & Is also Bas 19 14                                                                                  \\

\vspace{1.mm}

 61730 & SAO 252382 = HD 118137 + HD 118138 (spectroscopic binary) \\

\vspace{1.mm}

 62023 & Variable epsilon Cen                                                                                 \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 62128 & This is not IDS 13342-5846B. The latter, with a magnitude of 10.0 was observed but was too faint and too near the
         main object (62127) to be sighted \\

\vspace{1.3mm}

 62182 & SAO 252413 = HD 118885 + HD 118886 (spectroscopic binary) \\

\vspace{1.mm}

 62591 & Is also Ci 20.800                                                                                  \\

\vspace{1.mm}

 63012 & Variable mu Cen                                                                                      \\

\vspace{1.mm}

 63034 & Is also L 691 -29                                                                                  \\

\vspace{1.mm}

 64453 & Variable beta Cen                                                                                \\

\vspace{1.mm}

 64613 & Variable teta Aps                                                                                \\

\vspace{1.mm}

 64691 & Variable khi Cen                                                                                     \\

\vspace{1.mm}

 65674 & CPC 20.1 4228 = CPD-62 4017A + CPD-62 4017B                                                          \\

\vspace{1.mm}

 65675 & See previous note \\

\vspace{1.mm}

 66814 & Variable tau 01 Lup                                                                                  \\

\vspace{1.mm}

 67227 & Is also LS 3252                                                                                    \\

\vspace{1.mm}

 67233 & Is also LS 3254                                                                                    \\

\vspace{1.mm}

 67260 & Proxima \\

\vspace{1.mm}

 67895 & Variable eta Cen                                                                                 \\

\vspace{1.mm}

 68624 & Variable alpha Lup                                                                                   \\

\vspace{1.mm}

 70296 & Variable teta Cir                                                                                \\

\vspace{1.mm}

 70363 & Is also UBV 12990 and IRC -20275                                                                    \\

\vspace{1.mm}

 70605 & Is also HE 2-113 and HE 3-1044                                                                      \\

\vspace{1.mm}

 70915 & SAO 252997 = HD 132539 + HD 132540 (spectroscopic binary) \\

\vspace{1.mm}

 71038 & Variable sigma Lib                                                                                   \\

\vspace{1.mm}

 71315 & Is NGC 5822 167 : Br\"{u}ck et al. (1968 Publ. R. Obs. Edinburgh 6 no 9).                          \\

\vspace{1.mm}

 71660 & Error in the CD catalogue, which located it at \(-61^{o}\) 59.7' instead of \(-60^{o}\) 59.7'. This star should
         have been CD-60 ... The use of identifier CD-61 4686 is therefore inadvisable.  \\

\vspace{1.mm}

 72058 & Is also L 695 -15                                                                                  \\

\vspace{1.mm}

 72413 & SAO 206406 was observed as an inseparable binary. \\

\vspace{1.mm}

 72427 &  CPD-67 2807 = HD 134897 + HD 134898 (spectroscopic binary) \\

\vspace{1.mm}

 72981 & Variable delta Lup                                                                                   \\

\vspace{1.mm}

 73116 & Is also UBV 13212                                                                                  \\

\vspace{1.mm}

 73208 & SAO 242463 = HD 136415 + HD 136416 (spectroscopic binary) \\

\vspace{1.mm}

 74176 & Variable kappa 01 Aps                                                                                \\

\vspace{1.mm}

 75987 & SAO 253297 = HD 140483 + HD 140484                                                                   \\

\vspace{1.mm}

 77058 & SAO 207152 = HD 142691 + HD 142692 (spectroscopic binary) \\

\vspace{1.mm}

 77069 & Is also LS 3430 and VDBH 68 \\

\vspace{1.mm}

 77237 & Is also VDB 99 \\

\vspace{1.mm}

 77719 & This is not IDS 15532-6616B. The latter, with a magnitude of 14.2, was observed but was too faint and too near the
          main object (77718) to be sighted \\

\vspace{1.mm}

 77853 & Is also GJ 9539A                                                                                   \\

\vspace{1.mm}

 77855 & Is also GJ 9539B and L 697-41                                                                       \\

\vspace{1.mm}

 78490 & Is possibly HD 144941 = CD-26 11229 = UBV 13664 = UBV M 21189                                 \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 78826 & Is also VDB 100 \\

\vspace{1.3mm}

 79787 & Is also VDB 101 \\

\vspace{1.mm}

 79934 & Is also VDB 102 \\

\vspace{1.mm}

 79998 & Variable delta 01 Aps                                                                                \\

\vspace{1.mm}

 80030 & Is also VDB 103 \\

\vspace{1.mm}

 80126 & Is also VDB 104 and Variable sigma Sco         \\

\vspace{1.mm}

 80716 & Is also VDB 105 \\

\vspace{1.mm}

 80736 & Is also VDB 106                                                                                    \\

\vspace{1.mm}

 80767 & According to the notes in the HD catalogue (Volume 96, page 232, published in 1921) : \\
       & HD 147824 = CPD-40 7309 + CPD-40 7310. \\
       & The identifier HD 325539 (80768) only appeared in 1949 in HDE. \\

\vspace{1.mm}

 80768 & See previous note \\

\vspace{1.mm}

 80880 & Variable khi Oph                                                                                     \\

\vspace{1.mm}

 81175 & Variable alpha Sco = Antar\'{e}s \\

\vspace{1.mm}

 81265 & Is also VDB 108 \\

\vspace{1.mm}

 81448 & Variable omega Oph                                                                               \\

\vspace{1.mm}

 81634 & Is also PK 336 -00 1                                                                               \\

\vspace{1.mm}

 81662 & Variable mu Nor                                                                                      \\

\vspace{1.mm}

 82094 & Is also VDBH 72b                                                                                   \\

\vspace{1.mm}

 82136 & Is also HD 149711B                                                                        \\

\vspace{1.mm}

 82362 & The companion IDS 16335-3943B was not observed. \\

\vspace{1.mm}

 82491 & Is also VDB 109 \\

\vspace{1.mm}

 82841 & Is also LS 3728                                                                                    \\

\vspace{1.mm}

 83079 & Is also VDBH 73a \\

\vspace{1.mm}

 83605 & Variable mu 01 Sco                                                                                   \\

\vspace{1.mm}

 83830 & Is possibly LP 919 -11                                                                         \\

\vspace{1.mm}

 83918 & Variable zeta 01 Sco                                                                             \\

\vspace{1.mm}

 83949 & The companions IDS 16471-4140B and C were not measured. \\

\vspace{1.mm}

 84372 & Is possibly CPD-40 7646 \\

\vspace{1.mm}

 84677 & SAO 208258 = GJ 646A + GJ 646B = LTT 6774 + LTT 6775                                                 \\

\vspace{1.mm}

 84685 & Is also UBV M 21813 \\

\vspace{1.mm}

 86471 & Is also IRAS 17120-2159                                                                            \\

\vspace{1.mm}

 86531 & Is also UBV 14557                                                                                  \\

\vspace{1.mm}

 86730 & CPC 20.1 5200 = CPD-60 6745A + CPD-60 6745B                                                          \\

\vspace{1.mm}

 86731 & See previous note \\

\vspace{1.mm}

 86936 & Is also UBV 14705                                                                                  \\

\vspace{1.mm}

 87052 & Is also LS 4081 \\

\vspace{1.mm}

 87109 & Is also UBV 14564                                                                                  \\

\vspace{1.mm}

 87323 & Variable teta Oph                                                                                \\

\vspace{1.mm}

 87399 & SAO 208740 = HD 157038 + HD 157039 (spectroscopic binary) \\

\vspace{1.mm}

 87495 & Variable iota Ara                                                                                    \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

 87728 & Is also UBV M 38978                                                                                \\

\vspace{1.3mm}

 87972 & HD 157661 =  SAO 227971 + SAO 227972 : Inseparable \\

\vspace{1.mm}

 88174 & Is also UBV 14873                                                                                  \\

\vspace{1.mm}

 88974 & Identified according to Fitzgerald et al. (1978, Mon. Not. R. Astron. Soc. 182,607) \\

\vspace{1.mm}

 88977 & Identified according to FitzGerald et al. (1978, Mon. Not. R. Astron. Soc. 182,607)                       \\

\vspace{1.mm}

 89331 & Is also Ci 20 1046 and GCRV 20417                                                                   \\

\vspace{1.mm}

 90145 & Variable kappa Sco                                                                                   \\

\vspace{1.mm}

 90738 & Is HIC 87000                                                                                       \\

\vspace{1.mm}

 91436 & Is also LP 808 -23                                                                                 \\

\vspace{1.mm}

 92190 & SAO 209497 = HD 163195 + HD 163196                                                                   \\

\vspace{1.mm}

 93621 & SAO 228708 = HD 165189 + HD 165190                                                                   \\

\vspace{1.mm}

 93673 & Is also BPM 79362                                                                                  \\

\vspace{1.mm}

 93860 & Is also VDB 113 \\

\vspace{1.mm}

 94025 & Is also BD-22 4588                                                                                 \\

\vspace{1.mm}

 94240 & SAO 161152 = HD 166391 + HD 166392 (spectroscopic binary) \\

\vspace{1.mm}

 94630 & Variable mu Sgr                                                                                      \\

\vspace{1.mm}

 94771 & Is also VDB 117 \\

\vspace{1.mm}

 95154 & Is also VDB 118 and LS 4858                                                                         \\

\vspace{1.mm}

 95265 & Variable eta Sgr                                                                                 \\

\vspace{1.mm}

 96168 & Is also BD-19 4992                                                                                 \\

\vspace{1.mm}

 96471 & Is possibly GJ 2136B                                                                           \\

\vspace{1.mm}

 96836 & Is also L 206 -187                                                                                 \\

\vspace{1.mm}

 96852 & Is also IC 4725 1 : Johnson (1960, Astrophys. J. 131,620)                                        \\

\vspace{1.mm}

 96906 & Is also IC 4725 4 : Johnson (1960, Astrophys. J. 131,620)                                        \\

\vspace{1.mm}

 96967 & Is also BD-18 4986                                                                                 \\

\vspace{1.mm}

 97105 & The star U corresponds to Burnham's star C, near to B and not measured for this catalogue \\

\vspace{1.mm}

 97168 & Is also BD-19 5053                                                                                 \\

\vspace{1.mm}

 99121 & Variable lambda Pav                                                                                  \\

\vspace{1.mm}

 99573 & Variable kappa Pav                                                                                   \\

\vspace{1.mm}

 99742 & Variable epsilon CrA                                                                                 \\

\vspace{1.mm}

100441 & Is also UBV 16179                                                                                  \\

\vspace{1.mm}

 100826 & Very close to the NGC 6752 cluster \\

\vspace{1.mm}

101762 & Variable rho 01 Sgr                                                                                  \\

\vspace{1.mm}

104467 & Is also LP 870 -57 and L 709 -50                                                                    \\

\vspace{1.mm}

104558 & Is also L 709 -63                                                                                  \\

\vspace{1.mm}

105103 & Is also L 781 -32                                                                                  \\

\vspace{1.mm}

107117 & Variable rho Pav                                                                                     \\

\vspace{1.mm}

108648 & Is also GJ 2151                                                                                    \\

\vspace{1.mm}

108999 & Variable sigma Oct                                                                                   \\

\end{tabular}
\newpage
\begin{tabular}{rp{125.mm}}

109037 & Is also UBV 18226                                                                                  \\

\vspace{1.3mm}

109719 & Variable teta 01 Mic                                                                             \\

\vspace{1.mm}

110389 & Is also L 714 -21                                                                                  \\

\vspace{1.mm}

110446 & Is also L 354 -89                                                                                  \\

\vspace{1.mm}

110610 & Variable epsilon Cap                                                                                 \\

\vspace{1.mm}

111082 & Is also UBV 18661                                                                                  \\

\vspace{1.mm}

112896 & Variable pi 01 Gru                                                                                   \\

\vspace{1.mm}

113240 & Is also GCRV 14134                                                                                 \\

\vspace{1.mm}

113243 & Variable delta 02 Gru                                                                                \\

\vspace{1.mm}

113394 & Variable nu Tuc                                                                                      \\

\vspace{1.mm}

113950 & Variable beta Gru                                                                                \\

\vspace{1.mm}

115045 & LHS 3889 (115048) is close to PLX 5575.2 (115045). The pair is not mentioned by Luyten. If a proper movement equal
         to zero for the latter is assumed, the distance is increasing : 17" in 1950, 35" in 1975, 53" in 2000 \\

\vspace{1.mm}

115048 & See previous note \\

\vspace{1.mm}

115176 & Variable pi PsA                                                                                      \\

\vspace{1.mm}

115752 & Is also LTT 9423 and BPM 68205                                                                      \\

\vspace{1.mm}

116818 & Variable iot Phe                                                                                     \\

\vspace{1.mm}

117358 & Error of 1' in right ascension in the CD catalogue \\

\vspace{1.mm}

117957 & LTT 9818 is also LP 764 -39 and L 793 -35

\end{tabular}

\newpage
\vspace{20.mm}

\begin{center}
\large{\framebox(120,10){\bf{Explanations to the files SHB}}} \\[30.mm]
\end{center}

\begin{tabular}{lp{95.mm}}
File 1 : (SHB\_pre.tex) & : The tex file of this preface (records of 130 bytes). \\
File 2 : (SHB.cds)        & : The catalogue of 118065 stars with two lines for each star.
                              (236130 records of 130 bytes, blocksize=13000 bytes). \\
\end{tabular}
\vspace{10.mm}

First line  \\

\begin{tabular}{rrrp{100.mm}}
\\
 2 -&  7 : & i6    : & Designation of the star in the SHB catalogue. \\
    &  9 : & a1    : & Designation of companion. (a,b,c...) \\
11 -& 16 : & a5,a1 : & Magnitude,color  \\
18 -& 19 : & a2    : & Spectral type  \\
21 -& 29 : & i9    : & Right ascension for the equinox J2000 on the system
                       FK4, at the mean epoch of observations. (1/1000 sec. of time) \\
31 -& 39 : & i9    : & Declinaison for the equinox J2000 on the system FK4,
                       at the mean epoch of observations. (1/100 sec. of arc) \\
41 -& 49 : & i9    : & Right ascension for the equinox B50 on the system FK4,
                       at the mean epoch of observations. (1/1000 sec. of time) \\
51 -& 59 : & i9    : & Declinaison for the equinox B50 on the system FK4,
                       at the mean epoch of observations. (1/100 sec. of arc) \\
62 -& 63 : & i2    : & Deviation in right ascension (1/100 sec. of arc). \\
65 -& 66 : & i2    : & Deviation in declinaison (1/100 sec. of arc). \\
68 -& 74 : & f7.2  : & Mean epoch \\
    & 76 : & i1    : & Number of measurements \\
78 -& 80 : & a3    : & Comment 1. (See preface 2.6). Possible values : \\
    &      &         & m\_\_ : estimated magnitude. \\
    &      &         & nn : Indicates that the star forms part of a group of nn stars. \\
    &      &         & a=b : Components a and b appear to be equal in magnitude. \\
    &      &         & D : The star in question may be a double star (69 cases). \\
    &      &         & S : The star in question is part of a pair that is too close together to enable the
                       measurement of the two components. \\
82 -& 84 : & a3    : & Comment 2. (See preface 2.6). Possible values : \\
    &      &         & ? : A doubt exists as to the identification of the components. The allocation of the letters
                           a and b is arbitrary. \\
    &      &         & \verb|*| : See notes (listed in Annex V) \\
\end{tabular}

\newpage
Second line \\

\begin{tabular}{rrrp{100.mm}}
\\
     &      &       : & Identifiers \\
  2 -&  7 : & i6    : & SHB \\
 10 -& 18 : & a9    : & LHS or Variable \\
 21 -& 26 : & i6    : & PPM \\
 29 -& 34 : & i6    : & HIC     \\
 37 -& 42 : & i6    : & SAO     \\
 45 -& 52 : & a8    : & HD      \\
 55 -& 65 : & a11   : & CD \\
 68 -& 76 : & a9    : & CPC \\
 79 -& 89 : & a11   : & CPD \\
 92 -&103 : & a12   : & ADS or IDS \\
105 -&130 : & a26   : & Others catalogues. \\
\\
\end{tabular}
\end{document}
