2RE J003939+103925: POSS and Guide Star Catalog coordinates for BD+09 73 differ by 19 arcsec, suggesting proper motion. Spectroscopic binary (Jeffries et al. 1995). 2RE J004117+342547: Probably a single star (Jeffries 1995). 2RE J004403+093406: Also has a DA white dwarf companion (Barstow et al. 1994; Kellett et al. 1994). Both stars probably contribute to the EUV flux. Photometry of the K star reveals a period of 10h, the variation probably being due to a star-spot whose visibility is modulated by the rotation of the star (Kellett et al. 1994). 2RE J013739+183603: Close visual binary (separation ~2 arcsec) with similar components, both of which are active (Jeffries 1995). 2RE J025543+474630: Both stars in this visual K-type pair are active (separation ~3 arcsec) although the western component showed the greater activity. See also Jeffries (1995). 2RE J031222-442448: Emission cores are weak and variable in strength. 2RE J033314+461519: Resolved G5/dMe pair, separation ~2 arcsec, both active (see also Jeffries 1995). There is a discrepancy between the POSS and Guide Star Catalog coordinates of 7 arcsec which may be due to proper motion. 2RE J040237-001605: The identification is based on very weak emission cores observed on one occasion at Ca H&K. However, no emission was observed in the calcium triplet at 8500/8600A six months later. 2RE J040731+380423: Ca H&K emission seen in both stars of the pair, but Halpha emission from the northern component only. 1RE J042049+135206: Halpha emission line variable in strength by at least a factor of five between two observations 4 months apart. 2RE J044721-275015: dMe star is south-eastern component of visual pair. 2RE J050650-213504: Only SE component of BD-21 1074 observed. 2RE J053655-475802: ID is active K-star companion to 6th-magnitude G star. RE J061809+750557: Double dM3e system with a period of 0.539d (Jeffries et al. 1993). 2RE J072047-314645: White dwarf+dM binary, Porb~1.2d (Barstow et al. 1995b; Vennes & Thorstensen 1994). 2RE J072513-002551: Spectroscopic binary, period 1.40 d, both components active (Jeffries et al. 1995). 2RE J074335+224228: Spectroscopic binary (Jeffries et al. 1995). 2RE J075119+144551: Intermediate polar (IP) with a white dwarf spin period of 833.7s and an orbital period of 5.2h. Unusually bright in the EUV for an IP, and exhibits pulsed, polarized optical emission in the red which is also unique among known CVs of the IP subclass. See Mason et al. (1992), Rosen, Mittaz & Hakala (1993), Piirola et al. (1993), Duck et al. (1994) and Hellier, Ramseyer & Jablonski (1995) for further information. 2RE J085855+082754: POSS and Guide Star Catalog coordinates of M star differ by 17 arcsec, suggesting proper motion. 2RE J093036+103513: Visual binary, separation ~10 arcsec. North-eastern component shows the greater activity, but both active. 2RE J093348+624928: Spectroscopic binary, period 3.3d (Jeffries et al. 1995). 2RE J101627-052043: Unresolved white dwarf/dM-star pair. See Jomaron et al. (1993) and Tweedy et al. (1993). 2RE J103439+393806: Narrow line Seyfert 1 at redshift z=0.042 with an unusually hot (kTeff~100eV) and strong soft X-ray component whose intrinsic turnover towards low energies is observed in the soft X-ray (0.1-2.0keV) spectrum (Puchnarewicz et al. 1995). At the same time there is no evidence of a big blue bump component in its UV spectrum. 2RE J103439+393806 is also an IRAS source. 2RE J110159+223509: Spectroscopic binary, period 1.53d (Jeffries et al. 1995). 2RE J110441-041314: Visual multiple system. Components A and B both active, separation ~10 arcsec, brighter component to north-east. Component C not observed. 2RE J113246+121100: Spectroscopic binary, period 0.786d (Jeffries et al. 1995). 2RE J114746+125404: Probably single (Jeffries 1995). 2RE J114955+284508: Polar cataclysmic variable with a period of 90 min. See Mittaz et al. (1992). 2RE J115802+140208: Spectroscopic binary, period 0.92d (Jeffries et al. 1995). 2RE J123735+264329: Narrow-line Seyfert 1. The optical emission line spectrum of this object is very similar to that of 2RE J103439+393806 except that the forbidden oxygen lines are much weaker. In 2RE J103439+393806 we find the ratio F(Hbeta)/F([OIII]5007)=1.4, while, for 2RE J123735+264329, F(Hbeta)/F([OIII]5007)>=9. The soft X-ray flux is highly variable; the count rate recorded in subsequent ROSAT pointed observations was a factor of 70 less than during the ROSAT survey (Brandt et al. 1995). The optical ID spectrum was taken in 1991 May and we derive an uncorrected slit magnitude of V=16.2+/-0.2 through a 1.5-arcsec slit in good seeing. 2RE J130755+535144: Polar cataclysmic variable with a period of 79 min. See Osborne et al. (1994). RE J132046+070128: Southern component of visual pair, separation ~12 arcsec, is active. No activity detected in northern component. RE J133723+242300: Seyfert 1 galaxy, z=0.11. IRAS source which exhibits high linear polarization increasing from 1.4 per cent in the K band to 8 per cent in the U band (Wills et al. 1992). Strong iron emission in the optical spectrum. Detection by WFC may be inconsistent with reddening of E(B-V)~0.3 inferred by Wills et al. RE J141103+075036: Visual pair of dMe stars, separation ~2 arcsec, both active. 2RE J142642+500644: Visual triple. The northern component, an inactive M star, is the faintest and is separated from the other, closer, pair by about 7 arcsec. The middle component of the three stars is an active M star, while the southern component is a DA white dwarf. 2RE J144602+632929: Visual binary consisting of a white dwarf and an F star. The white dwarf (assumed to be the ID) is the western component of the double. 2RE J144206+352600: (=Mrk 478) This is a narrow-line Seyfert 1 with a steep soft X-ray spectrum (alpha=2.3^+0.25^_-0.13_; Gondhalekar et al. 1994). Also an IRAS source. 2RE J150110-434055: Double dM2e system with a period of 3.27d (Jeffries, James & Bromage 1994b). 2RE J150748+761225: Probably young and single. Has deep lithium absorption at 6707 A (Jeffries 1995). 2RE J152922+802720: Visual triple system. The main components (A,B) are separated by 31 arcsec. The brighter of these, the eastern component, exhibits emission cores in the Ca H&K lines. The western component, which is about 1 mag fainter, may also have very weak emission, but substantially less than its companion. Component C (136arcsec from A) was not observed. 2RE J160334-574532: The ID is the south-western component of the visual triple HD 143474, about 11 arcsec from the brighter pair (which are A stars). It is an RS CVn star with components G8V+K4V and an orbital period of 0.82376d (Kellett 1994, private communication). 2RE J160401-215512: Visual double. Brighter, northern component is active. May also be weak activity in fainter, southern component. 2RE J171126+664549: The white dwarf is the southern component of a close visual double. The northern component is an inactive M star. 2RE J171735+102508: Spectroscopic binary, period 0.65 d (Jeffries et al. 1995). 2RE J180214+641548: POSS and Guide Star Catalog coordinates for G227-22 differ by 16 arcsec because of proper motion. 2RE J181617+541029: Rapidly rotating single dM1-2e star (Jeffries et al. 1994a). 2RE J184450-741853: Polar cataclysmic variable with a period of 90 min. See O'Donoghue et al. (1993). 2RE J184609+191301: Probably single (Jeffries 1995). 2RE J190624+274308: Brighter (south-western) component of visual double is active. Spectroscopic binary, period 2.73d (Jeffries et al. 1995). 2RE J193835-461259: Polar cataclysmic variable with a period of 140 min. See Buckley et al. (1992). 2RE J201309+400240: Unresolved DAO+dM binary system, period ~ 0.7d (see Barstow et al. 1995a). 2RE J202414+200102: Unresolved white dwarf/dM binary system. 2RE J204746-363543: HD197890 is a rapidly rotating, probably single star. The EUV source is variable. See Matthews et al. (1994). 2RE J210755-051630: Eclipsing polar cataclysmic variable with a period of 125min. See Hakala et al. (1992). 2RE J220745+252017: The south-western component of a visual double (approximate separation 6 arcsec) is a white dwarf. Schwartz et al. (1995) suggest that the white dwarf and its visual companion, which they estimate to be a K4V star, form a physical pair. 2RE J221028-300514: North-western component of visual double is a white dwarf. 2RE J222009+493005: Probably single (Jeffries 1995). 2RE J224839-510928: Seyfert 1, redshift z=0.10. Beuermann & Thomas (1993) report a new polar CV detected in the ROSAT XRT survey data that is approximately 3 arcmin south of the 2RE source, and was not apparently detected in the WFC survey. This CV is formally inconsistent with the WFC 2RE position. Moreover, a pointed observation of 2RE J224839-510928 made with ROSAT confirms that the Seyfert galaxy is an X-ray source which is sufficiently bright to account for the WFC detection (Puchnarewicz et al. 1995). The source may have a variable soft X-ray excess. The optical permitted lines show a pronounced narrow component, and the single Gaussian fit quoted in Table 1 is a poor representation of the profile. A two-component Gaussian fit suggests a narrow-line FWHM of 330km/s (equivalent width 6.7A and a broad-line FWHM of 2900km/s (EW 50A). RE J230611+635614: POSS and Guide Star Catalog coordinates for the M star differ by 14 arcsec, suggesting proper motion.