2RE J002444-741253: Star HD21330 observed at high resolution at Ca II H&K. Upper
		     limit of 0.1 A on equivalent width of emission cores.
2RE J010349-725446: Crowded field where we've done little work. The star to the 
		     north of the error circle was observed - it is probably an 
		     A star or late B star, and so is unlikely to be the EUV 
		     source.
2RE J021420+513453: Three ~15th-magnitude stars near the edge of the error 
		     circle were observed at low resolution. Nothing remarkable.
                     Many other potential candidates.
2RE J042537-571348: 2RE error circle has moved in direction away from three 
		     stars observed. Significant difference between the position
		     of the 2RE error circle and the XRT error circle. The XRT 
		     error circle is consistent with the position of a 
		     ~15th-magnitude blue object, LB 01727, which is a Seyfert 1
		     galaxy (Pye et al. 1995).
2RE J045325-421347: Four stars close to or within the 2RE error circle were 
		     observed. These included a ~19th-magnitude star coincident 
		     with the XRT position. The spectrum of the faint star was 
		     too noisy to distinguish any features. However, subsequent 
		     work reveals this to be a polar CV (Beuermann and 
		     Thomas 1993). 
2RE J050003-362401: Various stars in and around 2RE error circle were observed 
		     at low resolution, and the ~13th magnitude star near the 
		     centre was also observed at high resolution in the vicinity
		     of Ca II H&K. No evidence of activity. 
2RE J050046-345113: Various stars observed at low resolution. The 
		     ~11th-magnitude star to the north of the error circle is an
		     unremarkable F star. The ~17th-magnitude star just within 
		     the northern boundary of the 2RE error circle at 
		     RA(2000) 05h 00m 45.94s, Dec(2000) -34d 50' 37.7" is very 
		     blue and is a good candidate as the optical ID of the 
		     source. However, our spectrum is too noisy for a more 
		     detailed classification. 
2RE J051523+324045: IUE observations reveal a white dwarf companion to the 
                     bright star (KW Aur) (Barstow et al. 1994; 
		     Hodgkin et al. 1993). 
2RE J061654-645724: Two of the brighter stars in the vicinity of the error 
		     circle were observed at low resolution. No remarkable 
		     properties.
2RE J063758-613159: High-resolution spectrum of HR2468 (V=6.2) in the vicinity 
		     of Ca II H&K does not reveal any evidence for emission 
		     cores with an upper limit to the equivalent width of 0.2A. 
2RE J065048-003236: High-resolution spectra of BD-00 1462 (V=5.8) in 1991 May, 
		     August and December failed to reveal emission cores in 
		     either CaII H&K or Halpha with an upper limit to the 
		     equivalent width of 0.05A. 
2RE J074345-391154: 2RE error circle has moved towards XRT position and away 
		     from stars observed in this programme.
2RE J084549+485255: HD74389 (V=9.4 A star) has V=15.5 white dwarf companion 
		     identified from IUE observations (Barstow, private 
		     communication).
2RE J102713+322356: The V=13 star near the XRT position may have weak emission 
		     cores in Ca II H&K, but these may be too weak to account 
		     for the observed WFC flux. Identified with `hidden' white 
		     dwarf by Barstow (private communication) from IUE 
		     observations.
2RE J111645+445417: Four stars observed at low resolution. The V=10 K star near 
		     the XRT position was also observed at high resolution in 
		     the vicinity of Ca II H&K and Halpha but the resulting 
		     spectra were relatively noisy. The upper limit on the 
		     equivalent width of any emission cores is ~0.6A. 
2RE J112617-684044: Three stars were observed at low resolution within the 
		     crowded WFC error circle. No remarkable properties. The XRT
		     position is significantly different from the WFC position. 
		     Identified with GU Mus (Nova Muscae 1991) by Pye et al. 
		     (1995).
2RE J130320-405654: Four stars observed at low resolution. No remarkable 
		     properties.
2RE J130928+081503: Six stars observed at low resolution. No remarkable 
		     properties. Bright star to north-east of current error 
		     circle was not observed as it was too far from the original
		     error circle.
2RE J192559-563327: The V=7.7 G star exhibits Ca II H&K emission cores with an 
		     equivalent width of 0.4A. However, this is probably 
		     insufficient to account for EUV flux. Barstow et al. (1994)
		     find that the G star has a white dwarf companion from IUE 
		     observations. 
2RE J205118-134132: Three stars observed at low resolution. No remarkable 
		     properties, but the spectrum of the faint star within the 
		     error circle is very noisy.
2RE J223428+081245: Five stars observed at low resolution. No remarkable 
		     properties. 
2RE J230034-070423: No evidence for emission cores in the Ca II H&K absorption 
		     lines in the V=9.6 G star spectrum (upper limit to 
		     equivalent width 0.05A). Barstow et al. (1994) report that 
		     this star has a white dwarf companion from IUE observations