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Search for associations containing young stars (SACY). I. Sample and searching method We report results from a high-resolution optical spectroscopic surveyaimed to search for nearby young associations and young stars amongoptical counterparts of ROSAT All-Sky Survey X-ray sources in theSouthern Hemisphere. We selected 1953 late-type (B-V~≥~0.6),potentially young, optical counterparts out of a total of 9574 1RXSsources for follow-up observations. At least one high-resolutionspectrum was obtained for each of 1511 targets. This paper is the firstin a series presenting the results of the SACY survey. Here we describeour sample and our observations. We describe a convergence method in the(UVW) velocity space to find associations. As an example, we discuss thevalidity of this method in the framework of the β Pic Association.
 
  |  Walraven photometry of nearby southern OB associations Homogeneous Walraven (VBLUW) photometry is presented for 5260 stars inthe regions of five nearby southern OB associations: Scorpio Centaurus(Sco OB2), Orion OB1, Canis Major OB1, Monoceros OB1, and Scutum OB2.Derived V and (B - V) in the Johnson system are included.
 
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Dades d'Observació i Astrometria
| Constel·lació: | Scorpius |  
    | Ascensió Recta: | 15h48m08.75s |  
    | Declinació: | -23°21'32.2" |  
    | Magnitud Aparent: | 9.188 |  
    
    
    | Moviment propi RA: | -28 |  
    | Moviment propi Dec: | -28 |  
    | B-T magnitude: | 9.859 |  
    | V-T magnitude: | 9.244 |  
    
 
 
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