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Table 3:

Summary of the properties of the spectroscopic datasets employed in this study.

Date
MJD Telescope Instrument Setting $\lambda $ Resln. Reference
          ($\AA$)    
23-25/06/01 52 083-5 ESO 1.52m Boller & Chivens Grat. #1 6000-11 000 500 C05
07/06/02 + 52 432 NTT EMMI Grat. #7 6310-7835 2600 C05
06-08/06/03 52796-8     Grat.#6 8225-8900 5000 Negueruela & Clark (2005)
12-13/06/04 53168-69 VLT FORS longslit G1028z 7730-9480 $\sim$7000 Negueruela et al. (2010)
        G1200R 5750-7310 $\sim$7000  
      FORS MXU G1200R 7730-9480a 2560  
      FORS MXU G1028z 5750-7310a 2140  
25/03/05 + 53 454 VLT FLAMES+ LR6 6438-7184 8600 Ritchie et al. (2009b)
29/05/05 + 53519   MEDUSA LR8 8206-9400 6500  
13/07/05 53 564            
29-30/06/05 53 550-1 NTT SOFI IJ Grism 9500-13 500 1000 Crowther et al. (2006)
        HK Grism 15 000-22 700 1000  
17/02/06 53 783 NTT EMMI Grat. #6 5740-8730 1500 Marco & Negueruela (2009)
11-12/03/06 53805-6 VLT ISAAC SWS(MR) 22 490-23 730 9000 Mengel &
              Tacconi-Garman (2007)
20+29/06/08 + 54367+76 VLT FLAMES+ HR21 8484-9001 16200 Ritchie et al. (2009a)
18+24/07/08 + 54665+71   MEDUSA        
14+17/08/08 + 54692+95            
04+15/09/08 + 54713+24            
19+25/09/08 + 54728+34            
14+18/05/09 + 54965+69            
20/08/09 55063            

Notes. aNote that the nominal wavelength range is given for the 2004 FORS MXU observations; in practice this can be displaced by a few hundred $\AA$ depending on the position of an individual star on the CCD.


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