WD0003-570    WD0003-570 consists of a non-magnetic WD and a late-type cool dwarf. (GU)
 WD0004+330    See also (NB)(NL)
 WD0005+511    Similar to the PG1159 degenerates but fewer, weaker metals and Balmer emission,X-ray corona,mass loss, Ref.(60)(84).
 WD0009+501    WD0009+501 is a magnetic degenerate,the first known below 100 kilogauss, Ref.(9W)(9V) See also(MV) (NB)
 WD0010-000    See also (NC)
 WD0011-134    LHS1044 is a magnetic degenerate, Ref.(31) See also(MV)(NN)
 WD0013+008.1  See also (NC)
 WD0014+003    See also (NC)
 WD0014-006    See also (NC)
 WD0014-015    See also (MS)
 WD0015+004    See also (MV)
 WD0015-004    See also (NC)
 WD0017+283    ABELL 21 is a PG1159-like star with no detected variability and an associated planetary nebula, Ref.(DG); TYPE E, Ref.(66).
 WD0018+147    See also (MV)
 WD0019-287    ZZ Ceti candidate (HC)
 WD0022-400    CPMB with APMPN 0025-3949A as second component (IN).
 WD0023+144    See also (NC)
 WD0023+388    Triple star system, also identifies G171-B10B as the WD and G171-B10A as the MS. Ref.(MK) Likely closer to d~60pc Ref.(MQ)
 WD0024-010    See also (NC)
 WD0025+000    See also (NC)
 WD0025-004    See also (NC)
 WD0025-277    ZZ Ceti candidate (HC)
 WD0027-636    See also (JV)
 WD0028-274    See section A1.2 in Ref. (LJ).
 WD0029+571    PG1159-like central star of SH2-136.(66).
 WD0030+006    See also (NC)
 WD0030+444    Binary (DA5+G8) system. Ref.(MK)
 WD0030-001    See also (NC)
 WD0032-175    See also (MR)
 WD0033+016    See also (MY)
 WD0033-007    See also (NC)
 WD0034+008    See also (NC)
 WD0034-211    Close double degenerate binary, Ref.(45),(MQ) See also (MY)
 WD0037+312    See also (JV)(NL)
 WD0038+555    G218-008 has strong UV absorption features, Ref.(CG).
 WD0038-226    LHS 1126 is the only know white dwarf to show JHK absorption, strong C2?  H2?  opacity, Ref.(DQ)(5X) see also (MM)
 WD0039+149    See also (NC)
 WD0041+092    Hot DA companion to the rapidly rotating K1-3V star BD+08 102, REF.(82)(4D).
 WD0041-102    FEIGE 7 is a magnetic white dwarf, Ref.(5F)(03).
 WD0044-121    NGC246 is a PG1159 star with several detected periods and an associated planetary nebula; type lgE, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
 WD0045+000    See also (NC)
 WD0046+051    VAN MAANEN2 was the only example of a DG white dwarf, Ref.(DB)(2L)(NN).
 WD0047+190    See also (MR)
 WD0047-524    See also (NL)
 WD0048-294    See also (JV)
 WD0049-011    See also (NC)
 WD0050-011    See also (NC)
 WD0050-332    See also (JV)(MV)(NB)(NL)
 WD0052+004    See also (NC)
 WD0052-006    See also (NC)
 WD0053-103    See also (NC)
 WD0057+003    See also (NC)
 WD0058+148    See also (NC)
 WD0059-008    ZZ Ceti star Ref.(KB)
 WD0101+002    See also (NC)
 WD0101+003    See also (NC)
 WD0101+048    Double degenerate system. Ref.(JP)see also (MM)(NB)(NL)
 WD0101+059    See also (MY)
 WD0104-464    BPM30551 is a ZZ CETI variable, Ref.(2W)(7I).
 WD0106-358    Possible companion <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.9.html'> Finding chart for GD 683B</A> see A4.2 in Ref.(LJ)
 WD0107+131    See also (NC)
 WD0108+000    ZZ Ceti star Ref.(KB)
 WD0108-001    See also (NC)
 WD0108-106    See also (NC)
 WD0112+132    See also (NC)
 WD0113+006    See also (NC)
 WD0114+002    See also (NC)
 WD0115+159    G033-049 has strong UV absorption features, Ref.(BO) (NB).
 WD0116-231    See also (JV)
 WD0120+154    See also (NC)
 WD0121-756    See also (JV) (KL)
 WD0122+200    Pulsating PG1159 DO degenerate, Ref.(DN)(39); TYPE A, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
 WD0126+101    Double degenerate system. Ref.(JP) see also (MM)(NB)
 WD0127+581    The DAO central star of the planetary nebula Sh2-188, Ref.(7U)
 WD0127-311    HE0127-311 is a magnetic degenerate, Ref.(3W).
 WD0128-012    See also (NC)
 WD0128-387    MCT0128-3846 is an unresolved DA + DB or DBA binary. (DM)
 WD0130+128    See also (NC)
 WD0130+141    See also (NC)
 WD0130-196    MCT0130-1937 is a PG1159 star with no detected variability, type A, Ref.(66).
 WD0131-163    See Section A5.16 in Ref.(LJ) See also (JV),(MQ),(MY)(NL)
 WD0131-287    ZZ Ceti candidate (HC)
 WD0132+127    Spectrum shows Mg I, Ref.(JJ)
 WD0133-116    R548 is a ZZ CETI variable, Ref.(5C) See also (NL)
 WD0133-299    ZZ Ceti candidate (HC)
 WD0134+181    See also (JE)
 WD0134+833    See also (NB)(NL)
 WD0134-002    See also (NC)
 WD0135-052    LP870-2 is a close detached DA binary system, Ref.(9K) Radial velocities -16.6/-41.2 km/sec Ref.(JP)N See also (NL)
 WD0136+251    Hot, low field magnetic ultra-massive DA star, Ref.(5V) See also (9U)(JV)(NL)
 WD0137-004    See also (NC)
 WD0139+143    See also (NC)
 WD0139+513    NGC650-1 is a PG1159 star with no detected variability and an associated planetary nebula, type E, Ref.(66).
 WD0139-011    See also (NC)
 WD0140+130    See also (MV)
 WD0141-675    See also (MV)(MM)
 WD0143+216    See also (MY)
 WD0145-174    See also (NN)
 WD0145-221    ZZ Ceti star ref.(JT) Has a possible Brown Dwarf Companion ref.(KX)
 WD0145-257    See also (MQ),(MY)
 WD0148+467    1400A absorption feature, Ref.(CL)  See also (NB)(NL)
 WD0148+641    GR268 common proper motion binary with G244-37 (M2 DWARF), Ref.(1R).
 WD0149-012    See also (NC)
 WD0149-082    See also (NC)
 WD0150+001    See also (NC)
 WD0155+003    Spectrum shows Mg I, Ref.(JJ)
 WD0158+235    A new hot DO with ultra highly excited ionization stages, Ref.(64).
 WD0158-160    Composite DBA + dM binary, Ref.(DP).
 WD0159-032    WD0159-032 is a magnetic degenerate, Ref.(02).
 WD0201+004    See also (NC)
 WD0201-006    See also (NC)
 WD0203+007    See also (NC)
 WD0203+131    See also (NC)
 WD0203-010    See also (NC)
 WD0204-306    CPM Binary with LP885-923 (WD+dM) Ref.(MK)
 WD0205+000    See also (NC)
 WD0205+133    See also (MQ)
 WD0205+250    See also (NL)
 WD0208+002    See also (MV)
 WD0208+396    G74-7 is the first known example of a definite DA, F degenerate, REF.(37),see also(MR)(NN)
 WD0209+085    DAB star in the DO-DB gap, Ref.(63), Teff=36,000K, Ref.(3X),(63)
 WD0209+210    See also (MV)
 WD0210+000    See also (NC)
 WD0210+086    White dwarf companion to the mild barium star XI 1 CETI; DA4 with 1400 and 1690 features, Ref.(37). Coords corrected, formerly WD0207+083
 WD0210+138    See also (NC)
 WD0210+168    See section A1.3 in Ref. (LJ).
 WD0210-010    See also (NC)
 WD0211+010    See also (NC)
 WD0211-086    ZZ Ceti star Ref.(KB)
 WD0212+140    See also (NC)
 WD0213+396    See also (MY)
 WD0213+427    See also (NN)
 WD0214+568    See also (MZ)(NL)
 WD0214-007    See also (NC)
 WD0215+005    See also (NC)
 WD0215+006    See also (NC)
 WD0216+007    See also (NC)
 WD0216+143    See also (JE)
 WD0216-005.1  See also (NC)
 WD0216-032    Luminosity of white dwarf probably dominated by wind accretion energy, Ref.(BX)(JV).
 WD0218+000    See also (NC)
 WD0221-399    CPM Binary with BD+39 0539 (WD+dM) system. Ref.(MK)
 WD0222+006    See also (NC)
 WD0222+422.1  CPM WD component with Mv > 15.0, Ref.(3A).
 WD0222+422.2  CPM WD component with Mv > 15.0, Ref.(3A).
 WD0222+648    Mv > 15.0, Ref.(51) formely WD0222+641.
 WD0222-291    We obtain T=3000 K, this may be the coolest WD known. (JW).
 WD0227+009    See also (NC)
 WD0227+050    See also (NB)(NL)
 WD0228-009    See also (NC)
 WD0228-085    See also (NC)
 WD0231-054    See also (MY)(NL)
 WD0232+035    FEIGE 24 is an EUV source, DA+dwarf M, Ref.(5Y) See also (NL)
 WD0232+525    See also (NL)
 WD0232-003    See also (NC)
 WD0233-083.1  See also (MV)
 WD0234-012    See also (NC)
 WD0235-003    See also (NC)
 WD0236+498    See also (NO)
 WD0239+109    G4-34 is a probable unresolved DA + DB binary, Ref.(23).
 WD0240+004    See also (NC)
 WD0242+002    See also (NC)
 WD0242+009    See also (NC)
 WD0243-026    See also (MR)
 WD0244+004    See also (NC)
 WD0245+541    See also (MR)
 WD0246+326    ZZ Ceti star ref.(GX)
 WD0246-301    ZZ Ceti candidate (HC)
 WD0247+053    A new DBA star from the HS survey, Ref.(4B)
 WD0248-014    See also (NC)
 WD0249-002    See also (NC)
 WD0250-007    CPMB with BD-01 0407 Ref.(EP), Referenced as 0250-008 in Ref.(MK)
 WD0252-009    See also (NC)
 WD0252-055    EUVE-discovered hot DA companion to the K0 IV star HD18131, Ref.(4D),(BP).
 WD0253+508    New magnetic degenerate, Ref.(61).
 WD0253-070    See also (NC)
 WD0253-077    See also (NC)
 WD0255+006.1  See also (NC)
 WD0255+009.2  See also (NC)
 WD0255-007    See also (NC)
 WD0255-705    See also (MV)(NB)(NL)
 WD0257+080    See also (MV)
 WD0259+004    See also (NC)
 WD0300+007    See also (NC)
 WD0300-013    A DB degenerate with calcium, Ref.(AC).
 WD0300-066    See also (NC)
 WD0301+004    See also (NC)
 WD0301-006    See also (MV)
 WD0302+027    See also (NL)
 WD0302+621    See also (MU)
 WD0303-007    See also (NC)
 WD0303-080    See also (NC)
 WD0304+004    See also (NC)
 WD0304+154    See also (JV)
 WD0306-006    See also (NC)
 WD0306-012    See also (NC)
 WD0307+077    See also (MR)
 WD0307-428    WD0307-428 is a magnetic degenerate, Ref.(02).
 WD0308+096    The dM companion is likely a binary M2 dwarf, see A5.19 in Ref.(LJ)
 WD0309-005    See also (NC)
 WD0310-688    1400A absorption feature, Ref.(CH) See also (NB)(NL)
 WD0311-013    See also (NC)
 WD0315-011    CPMB WITH BD-01 0469
 WD0316+003    ZZ Ceti star Ref.(KB)
 WD0316-849    RE0317-853 is a magnetic degenerate, Ref.(3Z).
 WD0317-011    See also (NC)
 WD0318-068    See also (NC)
 WD0319-004    See also (NC)
 WD0320-539    See also (JV)(NL)
 WD0321-002    See also (NC)
 WD0322+452    The DAO central star of HDW3, Ref.(7U).
 WD0322-013    See also (NC)
 WD0322-019    Double degenerate system. Ref.(JP)(NN)
 WD0323+009    See also (NC)
 WD0324+738    RA=033013.89 Dec=+740157.1(2005.09), resolved triple (WD+dM5+dM6) system. Ref.(MQ)
 WD0324-012    See also (NC)
 WD0324-012.1  See also (NC)
 WD0325-005    See also (NC)
 WD0325-857    LB 9802 is the visual companion to the high-field ultramassive WD EUVEJ0317-85.5, se[eation ~ 200AU.  Ref.(MV)
 WD0326+001    See also (NC)
 WD0326-273    Double degenerate system; radial velocities 105.9/157.1 km/sec Ref.(JP)
 WD0328-010    See also (NC)
 WD0329+005    KUV03292+0035 is a magnetic degenerate, Ref.(3V). This star is listed at Dec -00 35.1 in Ref.(CP).
 WD0330-009.1  ZZ Ceti star Ref.(KB)
 WD0330-013    See also (NC)
 WD0333+004    See also (NC)
 WD0333-350    See also (JV)
 WD0334-009    See also (NC)
 WD0335-002    See also (NC)
 WD0338+007    See also (MS)
 WD0339-451    See also (JV)
 WD0340+009    See also (NC)
 WD0340-068    See also (MV)
 WD0340-075    See also (MS)
 WD0341+021    Variability in radial velocity indicates a long period binary. (EE)
 WD0341+182    See also (NN)
 WD0341-076    See also (NC)
 WD0341-459    BPM31594 is a ZZ CETI variable, Ref.(7H).
 WD0342+004    See also (MV)
 WD0342+374    Hot DA planetary nucleus, Ref.(7U).
 WD0343+247    An ultra cool White Dwarf referred to in the references as WD0346+246
 WD0345+498    IW1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type A Ref.(66).
 WD0346-011    See also (MY)(MZ)(NL)
 WD0346-063    See also (NC)
 WD0347+171    V471 TAU,HYADES DA and K0V Eclipsing and Spectroscopic binary, REF(7V). DA star has TEFF=32,500K, LOG G=8, Ref.(2N)(JV).
 WD0347-137    See also (MQ)(MY)
 WD0348+339    See also (NL)
 WD0348-066    See also (NC)
 WD0349+247    Pleiad white dwarf with mass 0.98 MSUN; VGRAV= +84+/- 9 KM/S, Ref.(CR) See also (MZ)
 WD0350-002    See also (NC)
 WD0352+096    The finding charts point to different stars. See also (MZ)(NL)
 WD0354+463    See section A5.25 in Ref. (LJ), (MQ)
 WD0357-233    1950 coords from (1Y), 2000 coords from  <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.20.html'> Finding chart for Ton S 392B</A> These differ by almost 3' see A5.26 in Ref.(LJ),(MQ)
 WD0358-051    See also (NC)
 WD0401+250    See also (NL)
 WD0406+169    See also (NL)
 WD0408-041    Contains circumstellar dust (NG) See also (MR)
 WD0410+117    See also (NL)
 WD0413-077    The mass of 40ERI B is 0.43 MSUN, Ref.(8K). 1400A absorption feature, Ref.(2A) See also (NL)
 WD0415+271    HL TAU76 is a ZZ CETI variable, Ref.(4X).
 WD0416+334    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.2.html'> Finding chart for GD 60B</A> Ref.(LJ)
 WD0416+402    See also (NO)
 WD0416-550    See also (JV)
 WD0417+361    G038-029 is a ZZ CETI variable, Ref.(7L).
 WD0418+137    A triple system. (EX)
 WD0419-487    See also (MV)
 WD0420-007    See also (NC)
 WD0421+338    A quadruple system. (EX)
 WD0425+168    See also (JV)(NL)
 WD0426+588    The mass of this star is 0.48 or 0.68 MSUN, Ref.(AW)(JV)(NN).
 WD0429+176    White dwarf-red dwarf Hyades spectroscopic binary, REF(5B).  DA white dwarf with T=20,000K, LOG G=8, Ref.(AR)(JV).
 WD0433+270    EG40 common proper motion binary with G39-27 / BD+26 0730 (K5 DWARF), Ref.(7Z).
 WD0435-088    See also (NN)
 WD0439+466    DAO nucleus of the planetary nebula S216, Ref.(7U).
 WD0440-038    See also (JV)
 WD0443-275.1  Very close common proper motion pair, Ref.(7Z).
 WD0444+049    New PG1159 star, type A, Ref.(66).
 WD0446-789    See also (JV)(NB)
 WD0453+418    See also (NL)
 WD0453-295    A rare DAB hybrid composition degenerate, Ref.(DP), MCT0453-295 is an unresolved DA + DB binary, Ref.(DM).
 WD0455+553    GR318 is a ZZ CETI variable, Ref.(7J).
 WD0455-282    A new hot DA in a region of extremely low HI density, Ref.(15) See also (NB)(NL)
 WD0457-103    K0IV + DA binary, Ref.(14).
 WD0458-665    X-ray selected hot DA + dM binary, Ref.(3P).
 WD0500-156    The DAO central star of ABELL 7, Ref.(7U).
 WD0501+527    See also (NL)
 WD0501-289    Evidence of episodic mass ejection, rich metallic EUV spectrum, Ref.(DK,DT).
 WD0503-174    LHS1734 is a magnetic degenerate, Ref.(27)(MV).
 WD0504-241    DO white dwarf with ultra-high excitation absorption, Ref.(31).
 WD0507+045.1  One component of a visual pair of DA stars, Ref.(63), ZZ Ceti star ref.(IY)
 WD0507+045.2  One component of a visual pair of DA stars, Ref.(63).
 WD0509-007    See also (MV)(NL)
 WD0513+260    V1063 TAU is a non-radial pulsator, Ref.(44).
 WD0517+307    GD 66 is a ZZ CETI variable, Ref.(57).
 WD0518-105    See also (JV)
 WD0531-022    See also (JV)
 WD0532+414    Double degenerate system; radial velocities -38/150 km/sec Ref.(JP)
 WD0532-560    ZZ Ceti star ref.(JT)
 WD0533+555    DA central star of the planetary nebula HDW4, Ref.(7U).
 WD0543+579    See also (MR)
 WD0548+000    See also (JV)(NL)
 WD0548-001    G99-37 is magnetic and polarized, Zeeman H alpha, Ref.(5H)(03)(MV).
 WD0549+158    See also (MV)(MZ)(NB)(NL)
 WD0552-041    See also (MM)(NB)(NN)
 WD0553+053    G99-47 is a magnetic white dwarf, Ref.(03) See also(MV)(MM) (NB)(NN).
 WD0556+106    Rare DA nucleus of planetary nebula with Teff > 1E+5K, Ref.(5J).
 WD0558-756    Helium-rich DO nucleus of K1-27; TEFF>1E+5;similar to KPD0005, Ref.(8O)(JV).
 WD0603-483    See also (NO)
 WD0605+241    NGC2168:LA 2 = NGC2168:LAWDS 2
 WD0605+245    NGC2168:LA22 = NGC2168:LAWDS22
 WD0606+240    NGC2168:LA15 = NGC2168:LAWDS15
 WD0606+241    NGC2168:LA11 = NGC2168:LAWDS11
 WD0606+243    NGC2168:LA27 = NGC2168:LAWDS27
 WD0606+244.1  NGC2168:LA 5 = NGC2168:LAWDS 5
 WD0606+244.2  NGC2168:LA 6 = NGC2168:LAWDS 6
 WD0612+177    G104-27 detection of trace helium in a DA star, Ref.(3K) See also (NL)
 WD0615+556    Central star of the planetary nebula PW1, Ref.(7U).
 WD0615-591    CPMB WITH CD-59 1275
 WD0616-649    RE0616-649 is a new magnetic degenerate, Ref.(4A).
 WD0621-376    See also (MV)
 WD0622-329    Unresolved DA/DB double degenerate Ref.(MD)
 WD0625+415    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.3.html'> Finding chart for GD 74B</A> see A5.13 in (LJ)
 WD0625-253    Central star of Abell 15, REF.(2B).
 WD0637+477    GD77 is a magnetic degenerate, Ref.(9X) see also(MV)
 WD0640+015    Cool DO star (TEFF = 55000K) with one of the strongest HeII 4686 absorption lines of any known star, Ref.(7C)(5Q).
 WD0642-166    SIRIUS B mass=1.02 MSUN, Ref.(BK).
 WD0642-285    CPMB WITH CD-28 3361
 WD0644+375    See also (NB)(NL)
 WD0646-253    See also (MV)
 WD0651-020    See also (JV)(NL)
 WD0659-063    Listed in ref (NN) as WD0659-064
 WD0704+618    Coolest PG1159 star, no detected variability, Ref.(2T); type A, Ref.(66).
 WD0713+399    A new DO star with ultra-highly excited ionization features, Ref.(31)
 WD0713-468    LONGMORE 3 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(7R)(KL).
 WD0714+458    Possible companion 0714+458   <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.4.html'> Finding chart for GD 84B</A> see A4.1 in Ref.(LJ)
 WD0715-703    See also (JV)(MV)(NB)
 WD0718-316    DAO+dM2 pre-cataclysmic binary. Ref.(IT) See also (MV)
 WD0721-276    See also (MV)
 WD0726+133    WD associated with PN; Type: E Ref.(KL)
 WD0727+376    See also (NC)
 WD0727+482    G107-70 binary with two DC stars, Ref.(AX)(NN).
 WD0727+600    A new intermediate temperature DO star with ultra-highly excited species, Ref.(2T).
 WD0729+397    See also (NC)
 WD0732+330    See also (NC)
 WD0733+389    See also (NC)
 WD0734-143    See also (JV)
 WD0736+053    PROCYON B has mass =0.63 MSUN, Ref.(AV)(JV).
 WD0736+278    See also (NC)
 WD0736+391    See also (NC)
 WD0737-384    Member of the open cluster NGC 2451, Ref.(4O).
 WD0738+222    See also (NC)
 WD0738+382    See also (NC)
 WD0738+418.1  See also (NC)
 WD0738-172    First detection of calcium two 1840A absorption in a white dwarf, Ref.(4L)(NN).
 WD0738-382    Member of the open cluster NGC 2451, Ref.(4O).
 WD0739+238    See also (NC)
 WD0739+412    See also (NC)
 WD0740+325    See also (NC)
 WD0740+348    See also (NC)
 WD0741+356    See also (NC)
 WD0742+238    See also (NC)
 WD0742+653    A new intermediate temperature DO star, Ref.(2T).
 WD0743+442    See also (MY)
 WD0743+474    See also (NC)
 WD0743-336    VB3 common proper motion with HD63077 (G0 DWARF), shown to be low luminosity DC9 degenerate, not an M dwarf, Ref.(4T).
 WD0744+382    See also (NC)
 WD0744+384    See also (NC)
 WD0744+431    See also (NC)
 WD0745+210    See also (NC)
 WD0745+247    See also (NC)
 WD0745+258    See also (NC)
 WD0745+304    See also (MV)
 WD0745+436    See also (NC)
 WD0746+384    See also (NC)
 WD0746+396    See also (NC)
 WD0746-375    Member of the open cluster NGC 2451, Ref.(4O).
 WD0747+073.1  LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN).
 WD0747+073.2  LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN).
 WD0748+230    See also (NC)
 WD0748+436    See also (NC)
 WD0750+267    See also (NC)
 WD0750+317    See also (NC)
 WD0750+379    See also (NC)
 WD0751+299    See also (NC)
 WD0751-595    Foreground star not a cluster member, Ref.(8S).
 WD0752+278    See also (NC)
 WD0752+398    See also (NC)
 WD0752+402    See also (MS)
 WD0752+424    See also (NC)
 WD0752-146    Slight variability in radial velocity indicates a possible binary. Emission line has a VR0= -146.8km/s. (EE)
 WD0753+313    See also (NC)
 WD0753+478    See also (NC)
 WD0753+535    VV47 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(5O)(1M); type E, Ref.(66).
 WD0754+326    See also (NC)
 WD0755+358    See also (MV)
 WD0756+324    See also (NC)
 WD0756+350    See also (NC)
 WD0756+437    A new magnetic degenerate with a 220 MG field, Ref.(8N).
 WD0756+493    See also (NC)
 WD0756-607    Foreground star not a cluster member, Ref.(8S).
 WD0757+501    See also (NC)
 WD0757-603    Member of the open cluster NGC 2516, Ref.(8S).
 WD0757-606.1  Member of the open cluster NGC 2516, Ref.(8S).
 WD0757-606.2  Member of the open cluster NGC 2516, Ref.(8S).
 WD0758+224    See also (NC)
 WD0758-476    See also (JV)
 WD0800+233    See also (NC)
 WD0800+417    See also (NC)
 WD0801+186    See also (MV)
 WD0801-608    Foreground star not a cluster member, Ref.(8S).
 WD0802+220    See also (MV)
 WD0803+340    See also (NC)
 WD0803+407    See also (NC)
 WD0804+075    See also (NC)
 WD0804+397    See also (MV)
 WD0805+654    See also (JV)
 WD0806+376.1  See also (MV)
 WD0806-661    L0097-003 shows strong UV CI absorption, Ref.(DD).
 WD0807+190    Probably a moderate velocity red dwarf. private comm. J.Farihi 9/2008
 WD0807+416    See also (NC)
 WD0807+463    See also (NC)
 WD0808+058    See also (NC)
 WD0808+272    See also (MT)
 WD0809+034    See also (NC)
 WD0809+235    See also (NC)
 WD0810+329    See also (NC)
 WD0810+455    See also (NC)
 WD0811+411    See also (NC)
 WD0811+414    See also (NC)
 WD0812+433    See also (NC)
 WD0812+447    ZZ Ceti star Ref.(KB)
 WD0813+265    See also (NC)
 WD0813+358    See also (NC)
 WD0814+043    See also (MV)
 WD0814+058    See also (NC)
 WD0814+271    See also (NC)
 WD0816+356    See also (NC)
 WD0816+376    GD90 magnetic, not polarized, Zeeman H lines, Ref.(05)(03).
 WD0816+433    See also (NC)
 WD0817+062    See also (NC)
 WD0817+255    See also (NC)
 WD0818+461    See also (NC)
 WD0819+355    See also (NC)
 WD0819+461    See also (NC)
 WD0821+275    See also (NC)
 WD0821-252    See also (MV)
 WD0822+036    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD0822+342    See also (NC)
 WD0822+414    ZZ Ceti star Ref.(KB)
 WD0823+039    See also (NC)
 WD0823+062    See also (NC)
 WD0823+316    See also (JE)
 WD0823+336    See also (NC)
 WD0824+066    See also (NC)
 WD0824+082    See also (NC)
 WD0824+288    Double lined spectroscopic binary, DA + dwarf carbon star, Ref.(2R). dC companion VR0 = -36.8(EE) Triple system: DA+dC+M3V (IH)N(JV), see A5.4 Ref.(LJ)
 WD0824+474    See also (NC)
 WD0825+072    See also (NC)
 WD0825+297    See also (MV)
 WD0826+271    See also (NC)
 WD0826+282    See also (NC)
 WD0827+291    See also (NC)
 WD0827+321    See also (NC)
 WD0827+368    See also (NC)
 WD0827+472    See also (NC)
 WD0828+412    See also (NC)
 WD0830+536    See also (NC)
 WD0830-535    See also (NO)
 WD0831+056    See also (NC)
 WD0831+072    See also (NC)
 WD0832+436    See also (NC)
 WD0833+049    See also (NC)
 WD0834+270    See also (NC)
 WD0834+500    See also (JE)
 WD0834+532    See also (NC)
 WD0836+197    Praesepe member.
 WD0836+199    Praesepe member.
 WD0836+201    Praesepe member.
 WD0836+237    See also (NL)
 WD0836+404    ZZ Ceti star ref.(KA)
 WD0837+199    Praesepe member. See also (MV)
 WD0837+271    See also (NC)
 WD0837+273    See also (MV)
 WD0837+280    See also (NC)
 WD0837+283    See also (NC)
 WD0837+330    See also (MS)
 WD0837+458    See also (NC)
 WD0838+035    See also (JV)
 WD0838+375    CBS78 is the second known DB star showing accreted calicium, Ref.(AN).
 WD0839+025    See also (MV)
 WD0839+086    See also (NC)
 WD0839+372    ZZ Ceti star Ref.(KB)
 WD0839-327    See also (MV)(MM)(NB)(NL)
 WD0839-528    Not a confirmed cluster member, Ref.(4O)(JV).
 WD0840+047    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD0840+200    Possible PRAESEPE member, Ref.(BV)(JV).
 WD0841+055    See also (NC)
 WD0841+098    See also (NC)
 WD0842+375    See also (NC)
 WD0842+490    See also (JV)
 WD0844+287    See also (NC)
 WD0844+453    ZZ Ceti star Ref.(KB)
 WD0845+011    See also (NC)
 WD0845+440    See also (NC)
 WD0845-188    CPMB WITH CD-18 2482
 WD0846+052    See also (NC)
 WD0846+249    See also (JE)
 WD0846+346    See also (MR)
 WD0847+456    See also (NC)
 WD0848+007    See also (NC)
 WD0848+037    See also (NC)
 WD0848+062    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD0849+068    See also (NC)
 WD0849+549    See also (NC)
 WD0850+472    See also (NC)
 WD0853+049    See also (NC)
 WD0853+057    See also (NC)
 WD0853+069    See also (NC)
 WD0853+163    Misidentified as LB 8827 in much of the literature (IW)
 WD0855+328    See also (NC)
 WD0855+373    See also (NC)
 WD0855+407    See also (NC)
 WD0855+416    See also (MV)
 WD0855+583    See also (NC)
 WD0855+604.2  Possible CV? Ref.(AT).
 WD0856+047    See also (NC)
 WD0856+331    EG182 common proper motion binary with HD77408 (F8 dwarf);  G47-18 is a strong carbon band, DQ star polarized, Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therefore not CPMB.
 WD0858+363    GD99 is a ZZ CETI variable, Ref.(7M) See also (NL)
 WD0858+441    See also (NC)
 WD0859-039    See also (MV)
 WD0900+426    See also (NC)
 WD0900+565    See also (NC)
 WD0901+140    Visual double degenerate <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.11.html'> Finding chart for PG 0901+140B</A> see A5.8 in Ref.(LJ)
 WD0902+097    See also (NC)
 WD0903+083    See also (MV)
 WD0903+166    See also (JV)
 WD0903-002    ZZ Ceti star Ref.(KB)
 WD0904+358    See also (MV)
 WD0904+511    See also (JV)
 WD0905+062    See also (NC)
 WD0905+372    See also (NC)
 WD0905+538    See also (NC)
 WD0906+076    See also (NC)
 WD0908+033    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD0908+226    DA star, spectroscopic composite with dM, Ref.(7Z).
 WD0908+422    See also (MV)
 WD0910+014    See also (NC)
 WD0910+584    See also (MS)
 WD0910+593    See also (NC)
 WD0911+059    See also (MV)
 WD0912+105    See also (NC)
 WD0912+318    See also (NC)
 WD0912+453    See also (NC)
 WD0912+536    Polarization observed, Ref.(06) See also (MV) (NB)(NN)
 WD0913+055    Propose that spectrum originates from two unrelated stars on same line of sight. Ref.(MS)
 WD0913+408    See also (NC)
 WD0913+442    EG64 common proper motion binary with G115-64 (G5 dwarf),  Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therfore not CPMB.
 WD0913+444    See also (NC)
 WD0913-003    See also (NC)
 WD0914+096    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD0914+610    See also (NC)
 WD0914-195    See also (JV)
 WD0915+414    See also (NC)
 WD0915+551    See also (NC)
 WD0916+090    See also (NC)
 WD0917+430    See also (NC)
 WD0917-000    See also (NC)
 WD0918+047    See also (NC)
 WD0918+111    See also (NC)
 WD0918+398    See also (NC)
 WD0918+593    See also (NC)
 WD0919+104    See also (NC)
 WD0920+015    ZZ Ceti star Ref.(KB)
 WD0921+012    See also (NC)
 WD0921+016    See also (NC)
 WD0921+020    See also (NC)
 WD0921+354    G117-B15A is a ZZ CETI variable, Ref.(7M) See also(8W)(JE)(NL)
 WD0922+006    See also (NC)
 WD0922+014    See also (MV)
 WD0922+065    See also (NC)
 WD0922+162    Double degenerate ref.(JE)
 WD0922-000    See also (NC)
 WD0924+337    See also (NC)
 WD0925+386    See also (NC)
 WD0928+379    See also (NC)
 WD0928+399    See also (NC)
 WD0928+399.1  See also (NC)
 WD0928-713    Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart
 WD0929+350    See also (NC)
 WD0929+380    See also (NC)
 WD0930+096    See also (NC)
 WD0930+294    See also (MY)
 WD0930+815    A DA white dwarf companion to the hybrid K3II giant HD81817A.
 WD0931+034    See also (NC)
 WD0931+054    See also (NC)
 WD0931+058    See also (NC)
 WD0931+105    See also (MV)
 WD0931+444    See also (NC)
 WD0931+507    See also (MV)
 WD0933+345    See also (NC)
 WD0933+423    See also (NC)
 WD0933+526    Spectrum shows Mg I, Ref.(JJ)
 WD0933+729    Possible companion <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.12.html'> Finding chart for PG 0933+729B</A> see A4.3 in Ref.(LJ)
 WD0934+067    See also (NC)
 WD0935+577    See also (NC)
 WD0935-371.1  Strong UV CI lines, Ref.(CK).
 WD0935-371.2  Very close white dwarf pair; UBV photometry, Ref.(61).
 WD0936+054    See also (NC)
 WD0936+378    See also (NC)
 WD0936+382    See also (NC)
 WD0936+563    ZZ Ceti star Ref.(KB)
 WD0936+595    See also (NC)
 WD0937+049    See also (NC)
 WD0937+505    See also (JV)(MZ)
 WD0937+505    See also (NO)
 WD0937+513    See also (NC)
 WD0937+527    See also (NC)
 WD0938+002    See also (NC)
 WD0938+577    ZZ Ceti star Ref.(KB)
 WD0939+071    Spectra doesn't look like a single WD, P.Bergeron and J.Holberg, private comm 3/2008.
 WD0939+262    See also (NL)
 WD0940+619    See also (NC)
 WD0941+458    See also (MV)
 WD0943+441    See also (NL)
 WD0944+115    See also (NC)
 WD0944+452    has a common proper motion companion 20" away Ref.(KR)
 WD0945+127    See also (NC)
 WD0945+245    LB11146 is a magnetic DX degenerate in a double degenerate binary with a non-magnetic DA companion, Ref.(5I) see also (JE)(MV).
 WD0945+372    See also (NC)
 WD0945+578    See also (NC)
 WD0946+002    ZZ Ceti star Ref.(KB)
 WD0946+020    See also (NC)
 WD0946+036    See also (NC)
 WD0946+488    See also (NC)
 WD0947+016    See also (NC)
 WD0947+857    See also (NL)
 WD0948+031    See also (NC)
 WD0948+043    See also (NC)
 WD0949+256    Double degenerate ref.(JE)
 WD0949+451    Resolved triple (WD+dM4.5+dM4.5) system. Ref.(MQ)
 WD0949+484    See also (NC)
 WD0950+021    See also (MT)
 WD0950+139    DA star with Teff > 1E+5K, Ref.(5P) Planetary Nebula nucleus.
 WD0950-200    Double degenerate close binary, Ref.(45).
 WD0951+132    ZZ Ceti star Ref.(KB)
 WD0952+094    See also (NC)(MV)
 WD0952+182    ZZ Ceti star Ref.(KB)
 WD0953+621    See also (NC)
 WD0954+007    See also (NC)
 WD0954+023    See also (NC)
 WD0954+247    This star is listed in ref.(EE) as being a white dwarf.
 WD0954+342    SW LMI is a non-radial pulsator, Ref.(44).
 WD0954+697    See also (JV)
 WD0954-710    See also (NL)
 WD0955+017    ZZ Ceti star Ref.(KB)
 WD0955+412    See also (NC)
 WD0956+045    Visual double see A5.20 in Ref.(LJ)
 WD0957+022    See also (MV)
 WD0957+028.1  See also (NC)
 WD0957+089    See also (NC)
 WD0957+112    See also (NC)
 WD0957-666    Possible double degenerate binary, Ref.(BY) see also (MV)
 WD0958+024    See also (NC)
 WD0958+102    See also (NC)
 WD0959+038    See also (NC)
 WD0959+441    See also (NC)
 WD1000+044    See also (NC)
 WD1001+058    See also (MV)
 WD1001+203    See also (MY)
 WD1001+473    See also (NC)
 WD1002+525    See also (NC)
 WD1003+009    See also (NC)
 WD1003+612    See also (NC)
 WD1003-441    LONGMORE 4 is a PG1159 star with 9-11 detected periods and an associated planetary nebula mass ejection, Ref.(DJ); type lgEp, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
 WD1004+124    See also (NC)
 WD1004+128    See also (MV)
 WD1004+409    See also (NC)
 WD1005+002    ZZ Ceti candidate (HC)
 WD1005+465    See also (NC)
 WD1006+029    See also (NC)
 WD1007-002    See also (NC)
 WD1008-179    NOTE: Should be classified as an extremely hot, Teff > 100,000K, from ref(LX).
 WD1009+034    See also (NC)
 WD1010+049    See also (NC)
 WD1010+049.1  See also (NC)
 WD1010+064    See also (JV)(NL)
 WD1011+459    See also (NC)
 WD1011+601    ZZ Ceti star Ref.(KB)
 WD1012+093    See also (MV)
 WD1013+033    ZZ Ceti star Ref.(KB)
 WD1013+044    See also (MV)
 WD1013+494    See also (NC)
 WD1013-050    DAO white dwarf in a pre-CV, RE1016+053, REF.(BC), Quadruple system DAO + 3 dM stars, Ref(LJ) See also (MV)
 WD1014+083    See also (NC)
 WD1015+014    Polarized magnetic white dwarf, Ref. (04) see also (MV)
 WD1015+076    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.13.html'> Finding chart for PG 1015+076B</A> see A5.21 in Ref.(LJ)
 WD1015+161    See also (MR)
 WD1015+468    See also (NC)
 WD1016+406    See also (NC)
 WD1016+535    See also (NC)
 WD1017+125    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.14.html'> Finding chart for PG 1017+125B</A> Ref.(LJ)
 WD1017+366    GD116 is a magnetic degenerate, Ref.(9L).
 WD1018+515    See also (NC)
 WD1019+462    Binary (WD+M0) system. Ref.(MK)
 WD1019+583    See also (NC)
 WD1020+047    See also (NC)
 WD1020+442    See also (NC)
 WD1020+541    See also (MS)
 WD1022+009    See also (NN)
 WD1022+050    Double-degenerate candidate Ref.(KP).
 WD1022+108    See also (NC)
 WD1024-002    ZZ Ceti candidate (HC)
 WD1026+002    Radial Velocities 36.5/48.0 km/sec Ref.(JP) Section A3.2 in Ref.(LJ) indicates the companion is a high velocity background star, not a CPMB see also (MY)(NL)
 WD1026+117    LHS2273 is a magnetic degenerate, Ref.(28) see also (MV)
 WD1026+453    See also (NL)
 WD1027+398    See also (NC)
 WD1027+469    See also (NC)
 WD1029+537    See also (JV)
 WD1030+598    See also (NC)
 WD1031+234    A new magnetic degenerate with a field strength exceeding 500 megagauss, Ref.(9Y)(JE)N.
 WD1031-114    See also (NB)(NL)
 WD1032+027    See also (NC)
 WD1032+109    See also (NC)
 WD1032+393    See also (NC)
 WD1032+400    See also (NC)
 WD1033+464    Composite spectrum with dM, Ref.(9V), also see Section A5.14 in Ref.(LJ) See also (NL)
 WD1033+656    See also (MV)
 WD1034+001    Hot DO degenerate with C,N,O,Si absorption in the far UV, Ref.(AL).
 WD1034+077    LHS2288 MV > 15.0, Ref.(51).
 WD1034+661    See also (NC)
 WD1036-204    LP790-29 is a polarized,carbon band,magnetic degenerate, Ref.(5G).
 WD1037+521    See also (NC)
 WD1038+088    See also (NC)
 WD1038+096    See also (NC)
 WD1038+518    See also (NC)
 WD1039+447    See also (NC)
 WD1040+054    See also (NC)
 WD1040+406    See also (NC)
 WD1040+451    See also (JV)
 WD1041+063    See also (NC)
 WD1041+580    See also (NL)
 WD1041+580    See also (NO)
 WD1042-000    See also (NC)
 WD1042-690    See also (MV)
 WD1043+600    See also (NC)
 WD1043+610    See also (NC)
 WD1043-188    See also (NN)
 WD1045+056    See also (NC)
 WD1045+629    See also (NC)
 WD1045-091    HE1045-0908:a new magnetic DA white dwarf with a distinctive Zeeman line splitting pattern, Ref.(8R).
 WD1046+398    See also (NC)
 WD1048+668    See also (NC)
 WD1050+541    See also (NC)
 WD1050+598    See also (MV)
 WD1051+516    See also (NC)
 WD1051+533.1  CPMB with WD1051+533.2
 WD1051+533.2  CPMB with WD1051+533.1
 WD1052+273    See also (MY)(NL)
 WD1053+001    ZZ Ceti star Ref.(KB)
 WD1053+049    See also (NC)
 WD1053+511    See also (NC)
 WD1053+656    See also (MV)
 WD1053-550    Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart see also (MV)
 WD1055-072    DA6 observed to be featureless? Ref.(9V) (NB)(NN).
 WD1056+012    See also (NC)
 WD1056+516    DA1 may be a double degenerate, Ref.(81)(JV).
 WD1057+719    See also (NL)
 WD1058+078    See also (NC)
 WD1059+126    See also (NC)
 WD1101+364    double degenerate DA + DA double lined, Ref.(7F).
 WD1102+748    See also (MY)
 WD1103+015    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1103+078    See also (NC)
 WD1103-008    See also (NC)
 WD1104+602    See also (NL)
 WD1104+656    See also (NC)
 WD1105+053    See also (NC)
 WD1105+097    See also (NC)
 WD1105-048    See also (JE)(MZ)(NL)
 WD1105-340    CPMB with M4Ve companion Ref.(MD)
 WD1106+121    See also (NC)
 WD1107+055    See also (NC)
 WD1107+602    See also (MV)
 WD1107-257    Common proper motion pair.
 WD1108+207    See also (NN)
 WD1108+325    See also (NL)
 WD1109+244    See also (JV)(NL)
 WD1109-005    ZZ Ceti candidate (HC)
 WD1111+455    See also (NC)
 WD1112+096    See also (NC)
 WD1112+669    See also (NC)
 WD1113+542    See also (NC)
 WD1114+026    See also (NC)
 WD1114+113    See also (NC)
 WD1115+017    See also (NC)
 WD1115+101    See also (MV)
 WD1115+135    See also (NC)
 WD1115+158    A new pulsating DB star, Ref.(DV).
 WD1115+166    An Unresolved DAB Double Degenerate Binary. (GW)(HE)(JE)N
 WD1116+026    See also (MR)(NL)
 WD1119+042    ZZ Ceti star Ref.(KB)
 WD1120+008    See also (NC)
 WD1120+439    See also (MY)
 WD1120+509    Spectrum shows Mg I, Ref.(JJ)
 WD1121+216    Ross 627 is a DA white dwarf not DA, F or DF, Ref.(6A) see also (MM)(NB)(NN)
 WD1121-008    See also (NC)
 WD1123+014    See also (NC)
 WD1123+040    ZZ Ceti star Ref.(KB)
 WD1123+189    Composite DA + DM binary, Ref.(9V) see also (MY)(NL)
 WD1124+431    See also (NC)
 WD1125+131    See also (NC)
 WD1125-002    See also (NC)
 WD1126+089    See also (NC)
 WD1126+185    See section A1.3 in Ref. (LJ).
 WD1126+499    NOTE: 2000 coords are from ref(MH),Ref(LR) gives J112924.74+493931.9 but no star found at these coords using SDSS Finding Chart Tool. See also (MV)
 WD1126+668    See also (NC)
 WD1126-008    See also (MV)
 WD1129-030    See also (NC)
 WD1131+521    See also (MV)
 WD1132+661    See also (NC)
 WD1133+489    See also (MQ)(MS)(MT)(NC)
 WD1134+044    See also (NC)
 WD1134+300    No 1400a absorption feature observed, Ref.(CL)(JV) see also (MY)(NB)(NL)
 WD1135+000    See also (NC)
 WD1135+579    See also (MV)
 WD1136+514    See also (NC)
 WD1136-015    LBQS1136-0132 is a magnetic degenerate, Ref.(85) see also (MV)
 WD1137+423    ZZ Ceti star ref.(KA)
 WD1137+614    See also (MV)
 WD1138+046    See also (NC)
 WD1138-026    See also (NC)
 WD1140+004    ZZ Ceti candidate (HC) See also (NC)
 WD1141+462    See also (NC)
 WD1141+504    See also (NC)
 WD1142-645    L0145-141 shows strong UV absorption features, Ref.(DC).
 WD1143+321    See also (NL)
 WD1144+004    PG1159 degenerate, Ref.(DI); type EP, Ref.(66)(JV).
 WD1145+041    See also (NC)
 WD1145+487    See also (MV)
 WD1146+443    See also (NC)
 WD1146-015    See also (NC)
 WD1147+255    Common proper motion binary Ref.(JP)
 WD1147-010    See also (NC)
 WD1148+544    LP129-587 is a CPMB with LP129-586 Ref.(JL)
 WD1148-230    See also (NF)
 WD1149+001    See also (NC)
 WD1150+006    See also (NC)
 WD1151+015    See also (MV)
 WD1151+548    See also (NC)
 WD1151-029    PG1159 degenerate, Ref.(DN); type LGE, Ref.(66).
 WD1154+061    ZZ Ceti star Ref.(KB)
 WD1154+456    See also (NC)
 WD1156+117    See also (NC)
 WD1156+619    See also (MV)
 WD1159+619    See also (MV)
 WD1159+803    G255-002 is a ZZ CETI variable, Ref.(BN).
 WD1159-034    Proto-type of a new class of pulsating, hot, helium-rich DO degenerates (PG1159), Ref.(7K); type E, Ref.(66)(JV) Non-radial g-mode pulsator Ref.(KO)N.
 WD1201+035    See also (NC)
 WD1201-001    see also (MZ)
 WD1201-023    ZZ Ceti candidate (HC)
 WD1202+034    See also (NC)
 WD1202+608    Peculiar DAO white dwarf in a pre-CV; binary? Ref.(29), close double degenerate Ref.(3L)(JE)N.
 WD1203+085    See also (MV)
 WD1203+097    See also (NC)
 WD1203+432    See also (NC)
 WD1204+444    See also (MV)
 WD1204+450    Triple system <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.15.html'> Finding chart for PG 1204+450C</A> see A5.5 in Ref.(LJ)
 WD1204-026    ZZ Ceti candidate (HC)
 WD1206+654    See also (NC)
 WD1207-005    See also (NC)
 WD1208+039    See also (NC)
 WD1208+422    See also (NC)
 WD1208-025    See also (NC)
 WD1209+018    See also (NC)(MV)
 WD1210+464    is an unresolved binary see A5.22 in Ref.(LJ)
 WD1210+533    Peculiar DAO white dwarf, Ref.(3M)(JE)N.
 WD1210-011    See also (NC)
 WD1211-025    See also (NC)
 WD1211-169    HS1211-170 is a new magnetic degenerate, Ref.(4C).
 WD1212+589    See also (NC)
 WD1212-022    Heavily blanketed, cool(~6000K) magnetic(Zeeman split NaI and MgI) DZ. (EM)
 WD1213+096    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1213+437    See also (NC)
 WD1213+528    DA and dwarf M spectroscopic binary post-common envelope, Ref.(5A); DA degenerate with T=13,000K; log g=8; 1400A absorption, Ref.(AQ)(JV).
 WD1213+532    See also (NC)
 WD1214+267    See also (JE)
 WD1215+009    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1217+635    See also (NC)
 WD1218+496    See also (NC)
 WD1218+497    See also (MQ)(MY)(NC)
 WD1219+005    See also (MV)
 WD1219+098    See also (NC)
 WD1219-024    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1220+234    PG1220+234 is a magnetic degenerate, Ref.(31) see also (MV)
 WD1220+484    See also (MV)
 WD1221+422    See also (MV)
 WD1221-006    See also (NC)
 WD1223-659    See also (MM)
 WD1225+589    See also (NC)
 WD1225+637    Spectrum shows Mg I, Ref.(JJ)
 WD1225-015    See also (NC)
 WD1228+541    See also (NC)
 WD1229+290    See also (JV)
 WD1229+558    See also (NC)
 WD1229-028    See also (NC)
 WD1230+596    See also (NC)
 WD1230+605    See also (NC)
 WD1231+130    See also (NC)(MV)
 WD1231+447    See also (NC)
 WD1234+481    See also (JV)(NB)(NL)
 WD1235+012    See also (NC)
 WD1235+620    See also (NC)
 WD1236+012    See also (NC)
 WD1236+457    Listed in ref (NN) as WD1239+454
 WD1236+661    See also (NC)
 WD1236-004    See also (MQ)(NC)
 WD1236-495    BPM 37093 is a ZZ CETI variable, Ref.(44) see also (MY)(NB)(NL)
 WD1237+487    See also (NC)
 WD1237-028    See also (MY)
 WD1238+439    See also (NC)
 WD1238+618    See also (NC)
 WD1240+453    See also (NC)
 WD1240+644    See also (NC)
 WD1241-010    New double degenerate close binary, Ref.(7G), Triple system, see section A5.6 in Ref.(LJ).
 WD1245+413    See also (MV)
 WD1246+441    See also (NC)
 WD1246-022    See also (MV)
 WD1247+550    Possibly the coolest known degenerate star, Ref.(5S)(5N)(MQ)(NN).
 WD1248+009    See also (NC)
 WD1248+161    See also (MV)
 WD1249+016    See also (NC)
 WD1249+450    See also (NC)
 WD1250-018    See also (NC)
 WD1250-226    The central star of the Planetary Nebula A3, is a binary consisting of a white dwarf and a cool G8 IV star.(HD)
 WD1251+584    See also (NC)
 WD1252+031    See also (NC)
 WD1252+559    See also (NC)
 WD1252+564    See also (MV)
 WD1253+024    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1253+261    Central Star of PN LoTr 5, Ref.(JV)
 WD1253+378    HZ 34 is classified DAO in Ref.(DN)(JE)N.
 WD1254+003    ZZ Ceti candidate (HC)
 WD1254+019    See also (NC)
 WD1254+223    See also (JV)(NL)
 WD1254+345    HS1254+3430 is a magnetic degenerate, Ref.(63).
 WD1254+428    See also (NC)
 WD1255+481    See also (NC)
 WD1255+552    See also (NC)
 WD1257+037    See also (NN)
 WD1257+047    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.5.html'> Finding chart for GD 267B</A> Ref.(LJ)
 WD1257+278    See also (MY)
 WD1258+013    ZZ Ceti star Ref.(KA) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog.
 WD1258+593    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.7.html'> Finding chart for GD 322B</A> Ref.(LJ)
 WD1259+053    See also (NC)
 WD1300+263    See also (NN)
 WD1302+597    GD323 is classified DAB (peculiar).  First known stratified H/HE atmosphere?  Ref.(5W)(4K).
 WD1304+227    Common proper motion pair.
 WD1305+125    See also (NC)
 WD1307+354    GD 154 is a ZZ CETI variable, Ref.(8Y) See also (NL)
 WD1307-017    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1308+537    See also (NC)
 WD1309+853    A new magnetic degenerate with a 4.9 Mg field (8N) see also (MV)
 WD1310+597    See also (NC)
 WD1310-230    An interacting double-degenerate binary star with a period of 65.1 min. (FL)
 WD1310-472    A new, very low luminosity, degenerate star, one of the intrinsically faintest white dwarfs known, Ref.(9E).
 WD1311+028    See also (NC)
 WD1312+098    PG1312+098 is a magnetic degenerate, Ref.(9Z).
 WD1312+156    See also (NC)
 WD1314+003    See also (MS)
 WD1314+293    HZ43 soft X-ray EUV source, Ref.(7C) See also (JV)(NL)
 WD1314-153    The star indicated in both the Marsh and Arizona finding charts is at 13 16 47.5 -15 36 05 This is not consistent with the coords above which are for LP737-047, LHS2712 and NLTT33503. Also the coordinates on the Marsh chart are not consistent with the marked position.
 WD1317+018    See also (NC)
 WD1317+117    See also (NC)
 WD1317+135    See also (MV)
 WD1317+453    Newly identified double degenerate close binary, Ref.(7G)(JV).
 WD1318+042    See also (NC)
 WD1318+664    See also (NC)
 WD1320-026    See also (NC)
 WD1321+545.1  See also (NC)
 WD1322+130    See also (NC)
 WD1324+004    See also (NC)
 WD1325+581    See also (JV)
 WD1326+120    See also (NC)
 WD1326+132    See also (NC)
 WD1327+594    See also (MV)
 WD1327-083    1400a absorption feature, Ref.(CL). See also (KP)(NB)(NL)
 WD1328+017    See also (NC)
 WD1328+307    G165-007 has more identifiable line features than any other known degenerate, Ref.(DA).
 WD1328+461    See also (NC)
 WD1328+648    Spectrum shows Na I, Ref.(JJ)
 WD1329+666    See also (NC)
 WD1330+015    G62-46 is an unresolved double degenerate with a magnetic DA and a DC white dwarf, Ref.(24) see also (MV)
 WD1331+111    See also (NC)
 WD1332+643    See also (MV)
 WD1333+005    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.10.html'> Finding chart for LP 618-14</A> see A5.9 in Ref.(LJ)
 WD1333+487    Spectroscopic composite DB + DM, Ref.(1V).
 WD1333+510    See also (JV)
 WD1333-012    See also (NC)
 WD1334+013    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1334+039    See also (NN)
 WD1334-001.1  See also (NC)
 WD1334-160    See also (MY)
 WD1335+001    ZZ Ceti candidate (HC)
 WD1336+123    Common proper motion pair.
 WD1336+422    See also (NC)
 WD1337+021    See also (NC)
 WD1337+598    See also (NC)
 WD1337+705    See also (NL)
 WD1339+050    See also (NC)
 WD1339+606    See also (NC)
 WD1339+616    See also (NC)
 WD1339+659    See also (MV)
 WD1339-340    VR = 212 km/sec corrected for gravitational redshift ref.(MI)
 WD1342+414    See also (NC)
 WD1342+443    Single WD model atmosphere does not fit balmer lines, Ref.(81).
 WD1342+672    See also (MS)
 WD1343-006    ZZ Ceti star Ref.(KB)
 WD1344+106    See also (NN)
 WD1345+238    Common proper motion binary Ref.(JP) See also (NN)
 WD1345+417    See also (NC)
 WD1347+477    See also (NC)
 WD1347-129    Eclipsing binary (EH)
 WD1348+400    See also (NC)
 WD1349+144    See also (JE)
 WD1349+545    SBS1349+5434 is a magnetic degenerate, Ref.(5T).
 WD1349+552    ZZ Ceti star ref.(KA)
 WD1350+457    See also (NC)
 WD1350+656    ZZ CETI variable, Ref.(87)(JE)N.
 WD1350-090    WD1350-090 is a magnetic degenerate, Ref.(9W).
 WD1351+489    A new pulsating DB star, Ref.(DV).
 WD1352+013    ZZ Ceti star Ref.(KB)
 WD1352-022    See also (NC)
 WD1354+340    CPMB WITH BD+34 2473
 WD1357+366    See also (NC)
 WD1401+051    See also (MS)
 WD1401-014    See also (NC)
 WD1401-147    ZZ Ceti star ref.(KA)
 WD1402+545    See also (NC)
 WD1403+043    See also (NC)
 WD1403+451    See also (NC)
 WD1403-077    See also (JV)
 WD1404+008    See also (NC)
 WD1404+603    See also (NC)
 WD1406+050    NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog,
 WD1407-475    Variability in radial velocity indicates a possible binary with a period of ~ 1 day. (EE)
 WD1408-018    See also (NC)
 WD1411+659    See also (NC)
 WD1412+612    New magnetic degenerate, Ref.(63).
 WD1412-013    See also (NC)
 WD1413+015    See also (NL)
 WD1414+012    ZZ Ceti star Ref.(KB)
 WD1414+020    See also (NC)
 WD1414-088    Component B of the double-lined DA+DA binary system HE 1414-0848. (HG)
 WD1414-088.1  Component A of the double-lined DA+DA binary system HE 1414-0848. (HG)
 WD1416+633    Binary (WD+dM) system. Ref.(MK)
 WD1417+473    See also (NC)
 WD1418-088    Double degenerate system. Ref.(JP)
 WD1419+576    Resolved triple (WD+dM2+dM2) system. Ref.(MQ)
 WD1420+518    See also (NC)
 WD1422+095    CX BOO is a ZZ CETI variable, Ref.(44).
 WD1422+497    See also (NC)
 WD1423+027    See also (NC)
 WD1423+371    See also (NC)
 WD1424+534    PG1159 DO degenerate, Ref.(DN); type A, Ref.(66).
 WD1424+602    See also (NC)
 WD1425+375    See also (MV)
 WD1425+540    G200-39 common proper motion binary with G200-40 (K dwarf).  Prototype of the class of DBA stars, Ref.(5R).
 WD1425-811    L0019-002 is a ZZ CETI variable, Ref.(7I) See also (8Z)(NB)(NL)
 WD1427-024    See also (NC)
 WD1429-121    Non-radial g-mode pulsator Ref.(KO)
 WD1430+432    See also (MV)
 WD1430+460    See also (MV)
 WD1431+614    See also (NC)
 WD1433+367    See also (NC)
 WD1433+377    See also (NC)
 WD1433+538    See section A5.15 in Ref. (LJ) See also (NC)
 WD1434-014    See also (NC)
 WD1435+383    See also (NC)
 WD1435+621    See also (NC)
 WD1436+424    See also (NC)
 WD1436+578    See also (NC)
 WD1437+368    See also (NC)
 WD1437-008    See also (NC)
 WD1440+003    See also (NC)
 WD1440+017    ZZ Ceti star Ref.(KB)
 WD1440+753    See also (NO)
 WD1440+753    See also (MV)
 WD1443+336    See also (MQ)
 WD1444+592    See also (MV)
 WD1444+637    See also (JV)
 WD1444-174    See also (NN)
 WD1445+414    See also (NC)
 WD1446+050    See also (NC)
 WD1446+575    See also (MS)
 WD1447+356    See also (NC)
 WD1447-190    Reported as sdB in an earlier Ref. (EH).
 WD1448+419    See also (NC)
 WD1449+003    G066-036 common proper motion binary with G66-35 (G5 dwarf), Ref.(75). SectionA2.2 in Ref.(LJ) reports different motions for the pair therfore not CPMB.
 WD1449+168    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.16.html'> Finding chart for PG 1449+168B</A> Ref.(LJ)
 WD1449+522    See also (NC)
 WD1449+559    See also (NC)
 WD1450+011    See also (NC)
 WD1451+006    NOTE: Simbad currently shows coordinates for WD1451+006.1 not WD1451+006 See also (MZ)
 WD1451+006.1  Mistakenly identified as WD1451+006 in Ref. (MH)
 WD1451+411    See also (NC)
 WD1452+435    See also (MV)
 WD1452-022    See also (NC)
 WD1454+486    See also (NC)
 WD1454+595    See also (NC)
 WD1454+614    See also (NC)
 WD1454-630.1  L151-81 a rare binary with DA and DB components, Ref.(8A).
 WD1454-630.2  L151-81 a rare binary with DA and DB components, Ref.(8A).
 WD1456+103    CW BOO is a non-radial pulsator, Ref.(44).
 WD1456+515    See also (NC)
 WD1457+349    See also (NC)
 WD1457+455    See also (NC)
 WD1457+462    See also (NC)
 WD1458+045    See also (NC)
 WD1458+171    See also (MQ)
 WD1459+001    ZZ Ceti star Ref.(KB) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog.
 WD1459+013    See also (NC)
 WD1459+347    See also (MY)
 WD1500+011    See also (NC)
 WD1500+447    See also (NC)
 WD1501+664    H1504 may be the hottest known star,H and He lines absent;high gravity OVI features; HEAO-1 A-2 and EXOSAT powerful soft X-ray source, Ref.(7X); type EP, Ref.(66)(JV)(KL).
 WD1502+324    See also (NC)
 WD1502+586    See also (NC)
 WD1503+331    See also (NC)
 WD1503-070    See also (MV)
 WD1504+006    See also (NC)
 WD1504+546    See also (MQ)
 WD1504-011    See also (NC)
 WD1505+483    See also (NC)
 WD1506+399    See also (MV)
 WD1507+434.1  See also (NC)
 WD1508+008    See also (NC)
 WD1508+025    See also (NC)
 WD1508+409    See also (NC)
 WD1509+020    See also (NC)
 WD1509+322    See also (NB)
 WD1509+425.1  See also (MV)
 WD1514+353    See also (NC)
 WD1516+460    See also (NC)
 WD1516+534    See also (NC)
 WD1516+612    See also (MV)
 WD1517+357    See also (NC)
 WD1517+502    A rare dwarf carbon star plus white dwarf binary, Ref.(5I),(MQ). See also (NC)
 WD1517+740    HS1517+7403 is a PG1159 star with no detected variability, Ref.(DI); type A, Ref.(66).
 WD1518+328    See also (NC)
 WD1518+381    See also (NC)
 WD1519+323    See also (NC)
 WD1519+611    See also (NC)
 WD1520+388    See also (NC)
 WD1520+525    PG1520+535 is a PG1159 star with a detected planetary nebula but no detected variability, Ref.(DI) DO degenerate, Ref.(DN).
 WD1521+310    See also (JE)
 WD1521-003    ZZ Ceti star Ref.(KB)
 WD1522+462    See also (NC)
 WD1522+479    See also (NC)
 WD1522+508    See also (NC)
 WD1522+662    See also (JV)
 WD1524+005.1  See also (NC)
 WD1526+005    See also (NC)
 WD1526+333    See also (NC)
 WD1526+348    See also (NC)
 WD1529-772    See also (MV)
 WD1530+037    See also (NC)
 WD1530-019    NOTE: 2000 coords are from ref(MH),Ref(LU) gives J153332.9-020600.0 but no star found at these coords using SDSS Finding Chart Tool.
 WD1531-022    See also (MY)
 WD1532+033    See also (NL)
 WD1532+394    See also (NC)
 WD1532+415    See also (NC)
 WD1532+420    See also (NC)
 WD1533+423    See also (MV)
 WD1533-057    New magnetic degenerate, Ref.(5U)(JE)N.
 WD1534+503    Double degenerate system? Radial velocities -106/159? Ref.(JP)
 WD1537+382    See also (NC)
 WD1537+532    See also (MV)
 WD1537+651    See also (JE)
 WD1537-006    See also (NC)
 WD1539+035    See also (NC)
 WD1539+039    See also (MV)
 WD1539+333    See also (NC)
 WD1539+530    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.17.html'> Finding chart for PG 1539+530B</A> see A5.11 in Ref.(LJ)
 WD1541+061    See also (NC)
 WD1541+558    See also (NC)
 WD1541+650    ZZ Ceti star ref.(JE)
 WD1542-275    Common proper motion pair.
 WD1543+332    See also (NC)
 WD1544-377    L481-60 common proper motion binary with HR5965 (G6 dwarf) see also (MV)(NL)
 WD1545+303    See also (NC)
 WD1545+495    See also (NC)
 WD1546+316    See also (NC)
 WD1546+376    See also (NC)
 WD1546+426    See also (MS)
 WD1547+390    See also (NC)
 WD1547+411    See also (NC)
 WD1548+539    See also (NC)
 WD1549-000    Correct Declination is +00 04 16 (1950). (DY)
 WD1550+437    See also (NC)
 WD1551+051    See also (NC)
 WD1552+486    See also (MS)
 WD1553+414    See also (NC)
 WD1554+550    See also (NC)
 WD1555+366    See also (NC)
 WD1555+401    See also (NC)
 WD1556+026    See also (NC)
 WD1558+378    See also (NC)
 WD1559+343    See also (NC)
 WD1559+365    See also (NC)
 WD1559+366    See also (NC)
 WD1559+369    R808 is a ZZ CETI variable, Ref.(7M) See also (NL)
 WD1600+472    See also (NC)
 WD1602+543    See also (NC)
 WD1603+492    See also (MV)
 WD1604+463    See also (NC)
 WD1605+424    See also (NC)
 WD1605+428    See also (NC)
 WD1606+422    Double degenerate system. Ref.(JP) see also (NB)
 WD1608+002    See also (NC)
 WD1608+258    See also (NC)
 WD1609+011    See also (NC)
 WD1609+135    See also (MY)
 WD1609+468    See also (NC)
 WD1609+493    See also (NC)
 WD1611+459    See also (NC)
 WD1615+390    See also (NC)
 WD1615-154    See also (NB)(NL)
 WD1616+010    See also (NC)
 WD1616+430    See also (NC)
 WD1616+435    ZZ Ceti star Ref.(KB)
 WD1619+123    Companion to HD 147528 Ref.(LJ)
 WD1619+525    Probably triple (DA2.8+dM5+dM7) Ref.(MQ)
 WD1620-391    CD-38 10980 25,000k DA degenerate with gravitational redshift, Ref.(CB)(JV), Companion to HD 147513.(LJ) see also (MV)(NL)
 WD1621+347    See also (NC)
 WD1621+360    See also (NC)
 WD1621-002    See also (NC)
 WD1621-010    See also (NC)
 WD1622+323    See also (MQ)
 WD1622+369    See also (NC)
 WD1622+406    See also (NC)
 WD1626+291    See also (NC)
 WD1626+368    See also (NB)
 WD1631+781    DA + DM detached binary RE1629+780, Ref.(AJ)(JV). Resolved triple (WD+dM3+dM3) system. Ref.(MQ) See also (NL)
 WD1632+387    See also (NC)
 WD1633+313    See also (NC)
 WD1633+572    CPM companion of CM Dra, Ref.(JV)
 WD1634-573    Hot (55,000K) DO degenerate with photospheric carbon in UV; hottest white dwarf with Einstein redshift, Ref.(AH)(AS)(JV).
 WD1635+252    See also (NC)
 WD1635+315    See also (NC)
 WD1635+478    See also (NC)
 WD1636+351    See also (JV)(NL)
 WD1637+335    See also (NB)
 WD1639+153    See also (MY)
 WD1639+211    See also (NC)
 WD1639+537    Only single magnetic degenerate with emission lines, Ref.(2H) see also (MV)
 WD1640+384    See also (NC)
 WD1641+241    See also (MV)
 WD1641+387    See also (JV)
 WD1643+143    See also (MY)
 WD1643+425    See also (NC)
 WD1644+424    See also (NC)
 WD1645+251    See also (NC)
 WD1645+325    The first known pulsating DB white dwarf, Ref.(DW) See also (NB)
 WD1645+372    See also (MV)
 WD1646+361    See also (NC)
 WD1647+591    G226-029 is a ZZ CETI variable, Ref.(7J); 1400A absorption, Ref.(3N) see also (MY)(NB)(NL)
 WD1648+342    See also (MV)
 WD1648+391    See also (NC)
 WD1648+407    See also (NO)
 WD1648+407    See also (JV)
 WD1649+300    See also (NC)
 WD1649+419    See also (NC)
 WD1650+355    See also (MV)
 WD1653+188    See also (NC)
 WD1653+200    See also (NC)
 WD1653+256    ZZ Ceti Candidate (Ref. JL)
 WD1654+160    V824 HER is a non-radial pulsator, Ref.(44), see section A5.23 in Ref.(LJ).
 WD1655+215    See also (NB)
 WD1657+343    See also (JV)
 WD1658+440    Ultra-massive DA degenerate 1.31 MSUN, low B-field, X-ray source, Ref.(9U) see also (8L)(5V)(JV)(MV)
 WD1659+303    <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.18.html'> Finding chart for PG 1659+303B</A> see A5.24 in Ref.(LJ)
 WD1659+344    See also (NC)
 WD1659+359    ZZ Ceti star Ref.(KB)
 WD1659+442    See also (JV)
 WD1659-531    BPM24601 common proper motion binary with HR6314 (F7 dwarf). Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart. See also (NB)
 WD1702+322    See also (MV)
 WD1703+199    See also (NC)
 WD1703+212    See also (NC)
 WD1703+388    See also (NC)
 WD1704+217    See also (NC)
 WD1704+481.1  Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH).
 WD1704+481.2  Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH).
 WD1706+220    See also (NC)
 WD1707+295    See also (NC)
 WD1707+427    PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) variable WD Ref(KL) Non-radial g-mode pulsator Ref.(KO)N.
 WD1710+559    See also (NC)
 WD1710+683    Binary (DA7.2+K7/M0 dwarf) system.  Ref.(MK)
 WD1711+657    ZZ Ceti star Ref.(KB)
 WD1712+274    See also (NC)
 WD1712+298    See also (NC)
 WD1712+629    See also (NC)
 WD1713+332    Double degenerate close binary, Ref.(7G).
 WD1713+393    See also (MV)
 WD1714-547    ZZ Ceti star ref.(KA)
 WD1715+547    See also (NC)
 WD1715+601    See also (MV)
 WD1716+020    Common proper motion binary. Ref.(JP) See also(NB)
 WD1716+598    See also (NC)
 WD1717+610    See also (NC)
 WD1717-345    Possible red dwarf companion, Ref.(8P)N.
 WD1719+569    See also (NC)
 WD1719+629    See also (NC)
 WD1720+283    See also (NC)
 WD1720+638    See also (NC)
 WD1722+541    See also (MV)
 WD1723+563    See also (NC)
 WD1723+586    ZZ Ceti star Ref.(KB) See also (NL)
 WD1723+595    See also (NC)
 WD1724+626    See also (NC)
 WD1725+561    See also (NC)
 WD1725+586    See also (NO)
 WD1726+545    See also (NC)
 WD1727+589    See also (NC)
 WD1728+565    See also (MV)
 WD1728+621    See also (NC)
 WD1729+371    Contains circumstellar dust (NG) See also (MR)
 WD1730+625    See also (NC)
 WD1731+591    ZZ Ceti star Ref.(KB)
 WD1732+608    See also (NC)
 WD1734+542    See also (NC)
 WD1735-318    An extremely hot DA white dwarf close to the open cluster NGC6405, Ref.(4P).
 WD1736+133    White dwarf companion to HD160365, Ref.(36).
 WD1736+540    See also (NC)
 WD1736+562    See also (NC)
 WD1738+669    Hottest known DA star associated with nebula, Ref.(12).
 WD1740+541    See also (NC)
 WD1741+543    See also (NC)
 WD1748+708    G240-072 is magnetic and polarized, Ref.(03) see also (MV)(NB)(NN)
 WD1750+098    EG124 common proper motion binary with G140-b1a / BD+09 3501 (K2 dwarf).
 WD1751+106    ABELL 43 is a hybrid, PG1159-like central star; type LGEH, Ref.(66) CSPN effective temperature 116,900K. (IO)N.
 WD1756+827    See also (MM)(NB)(NN)
 WD1800+685    See also (NL)
 WD1802+213    See also (JV)
 WD1814+248    A new magnetic degenerate, Ref.(8M).
 WD1818+126    See also (MV)
 WD1821+643    PG1159 DO degenerate, type LGE, Ref.(66)(JV)(KL) Non-radial g-mode pulsator Ref.(KO)N.
 WD1822+008    SH2-68 is a PG1159-type planetary nucleus, type AH, Ref.(66) CSPN effective temperature 125,900K. (IO)N.
 WD1823+063    NGC6633:LA15 = NGC6633:LAWDS15 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
 WD1824+040    Double-degenerate candidate Ref.(KP), Triple degenerate system DA3.4(a)+DC5.0(b)+DC10.6(c) see A5.1 in Ref.(LJ) <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.1.html'> Finding chart for G21-15C</A>
 WD1824+062    NGC6633:LA 8 = NGC6633:LAWDS 8 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
 WD1824+063    Calculated Mv=11.84 from model spectrum and radius and conclude star is too bright to be a member of NGC6633. (ED) nOTE: NGC6633:LA14 = NGC6633:LAWDS14
 WD1824+063.1  NGC6633:LA27 = NGC6633:LAWDS27 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009
 WD1824+063.2  NGC6633:LA13 = NGC6633:LAWDS13
 WD1824+064    Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 4 = NGC6633:LAWDS 4
 WD1825+063    Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 7 = NGC6633:LAWDS 7
 WD1825+067    NGC6633:LA16 = NGC6633:LAWDS16
 WD1826+064    NGC6633:LA12 = NGC6633:LAWDS12
 WD1829+547    G227-035 is a magnetic white dwarf, Ref.(03).
 WD1830+721    HS1830-721 is an intermediate temperature DO star with TEFF > 80,000K, Ref.(2T).
 WD1831-002    White dwarf companion of a binary pulsar, Ref.(9S).
 WD1837-619    Strong UV lines of neutral carbon, Ref.(CI).
 WD1840+042    See also (MY)
 WD1844-654    See also (JV)
 WD1845+019    See also (NL)
 WD1845+683    See also (NO)
 WD1845+683    White dwarf is likely, neither a suspected nor confirmed binary. Ref. (MQ) See also (NL)
 WD1855+096    White dwarf companion of a binary pulsar, Ref.(9S).
 WD1855+338    G207-009 is a ZZ CETI variable, Ref.(8Z) see also (MY)(NL)
 WD1856+534    A possible triple system, Ref.(7Z).
 WD1858+393    See also (MR)
 WD1900+140    Central star of SH2-28; type A, Ref.(66).
 WD1900+705    G260-015 is a magnetic white dwarf, Ref.(06)(03). See also (NB)
 WD1906-600    See also (JV)
 WD1909+304    PG1159-like central star of NGC6765; type lgE, Ref.(66).
 WD1910+047    Photospheric X-ray emission detected by HEAO-B, TEFF= 22,500K, Ref.(7D)(7B)(JV).
 WD1917-077    LDS678A shows strong CI lines in UV, weak HeI in optical, Ref.(CF)(AO), Binary DA+dm3.5, Ref.(LJ).
 WD1919+145    See also (NB)(NL)
 WD1935+276    G185-032 is a ZZ CETI variable, Ref.(7J) See also (NL)
 WD1936+327    See also (MZ)(NL)
 WD1942+499    See also (NO)
 WD1942+499    See also (NB)
 WD1944-421    See also (JV)
 WD1950+250    GR394 is a ZZ CETI variable, Ref.(86).
 WD1950-432    See also (NO)
 WD1953-011    See also (MM)(NB)(NL)
 WD1957+225    See also (JV)
 WD1958+015    K1-18 is a PG1159-like central star of NGC6852, type lgE, Ref.(66).
 WD2002-110    See also (NN)
 WD2003+437    GD387 probable unresolved DA+DC system, Ref.(23).
 WD2007-303    See also (NB)
 WD2009+622    See also (MQ)
 WD2010+310    GD229 is magnetic and polarized, Ref.(6)(03); UV spectrum discussed in Ref.(1Q).
 WD2011+398    DAO + M dwarf pre-cataclysmic binary, Ref.(10)(JV).
 WD2014-575    See also (NO)
 WD2014-575    See also (JV)(NB)(NL)
 WD2020-425    See also (NO)
 WD2020-425    See also (JV)
 WD2027+068    A new hot DO star with ultra highly excited ionization stages, Ref.(64).
 WD2028+390    See also (JV)
 WD2029+183    The finding charts point to different stars.
 WD2031-277    See also (JV)
 WD2032+248    See also (JV)(NB)(NL)
 WD2038-013    See also (NC)
 WD2039-001    See also (MS)
 WD2039-003    See also (NC)
 WD2039-202    See also (NL)
 WD2039-682    See also (MV)(MY)(NB)
 WD2041-064    See also (NC)
 WD2043-053    See also (NC)
 WD2043-073    See also (MV)
 WD2043-635    See also (NO)
 WD2044+001    See also (NC)
 WD2045-000    See also (NC)
 WD2046+396    See also (NL)
 WD2046-059    See also (NC)
 WD2047+372    See also (NB)(NL)
 WD2048-002    See also (NC)
 WD2049-004    See also (MV)
 WD2051+464    See also (JV)
 WD2052+006    See also (NC)
 WD2054+005    See also (NC)
 WD2054-050    See also (NN)
 WD2055+221    See section A1.1 in Ref. (LJ).
 WD2056+033    See also (JV)
 WD2056-070    See also (NC)
 WD2058+342.1  GD 392B is ultracool CPMB companion to GD 392 Ref.(JP)
 WD2059+190    See also (MY)
 WD2059+316    Strong UV CI lines, Ref.(CK).
 WD2102+101    See also (NC)
 WD2103-061    See also (NC)
 WD2104-070    See also (NC)
 WD2105-820    See also (MV)(NB)(NL)
 WD2108+094    See also (NC)
 WD2109+010    See also (NC)
 WD2109+100    See also (NC)
 WD2111+498    See also (JV)(NB)(NL)
 WD2111-012    See also (NC)
 WD2114+239    The DAO degenerate central star of ABELL 74, Ref.(66).
 WD2115+008    See also (NC)
 WD2115+118    A new hot DAO star with ultra highly excited ionization stages, Ref.(64).
 WD2115+339    RXJ2117.1+3417 is a PG1159 star with 24 detected periods and an associated planetary nebula, Ref.(DF,BA); type lgE, Ref.(66)(JV) Non-radial g-mode pulstaor Ref.(KO)N.
 WD2115-082    See also (NC)
 WD2115-560    Contains circumstellar dust (NG) See also (MV)(NB)
 WD2116+736    See also (NO)
 WD2117+539    1400A absorption feature, Ref.(CL) See also (NL)
 WD2118-011    See also (NC)
 WD2118-061    See also (NC)
 WD2120+002    See also (NC)
 WD2122+361    NGC7063:LA 3 = NGC7063:LAWDS 3
 WD2122+362    NGC7063:LA 4 = NGC7063:LAWDS 4
 WD2122+362.1  NGC7063:LA 1 = NGC7063:LAWDS 1
 WD2122+362.2  NGC7063:LA 2 = NGC7063:LAWDS 2
 WD2122+363    NGC7063:LA 6 = NGC7063:LAWDS 6
 WD2122-013    See also (NC)
 WD2123-226    White dwarf companion to the barium star ZETA Cap with MWD=0.96Msun TEFF= 23,200K, Ref.(35).
 WD2124+550    See also (MY)
 WD2126+734    1400A absorption feature, Ref.(2I), (3N), Binary system - companion probable WD, see section A5.7 in Ref.(LJ) See also (NL)
 WD2128+469    Binary system classified as a Cataclysmic Variable. (JF).
 WD2129+003    See also (NC)
 WD2131+066    PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) Binary system: PG1159+M2V (IJ)N(KL)N Non-radial g-mode Pulsator Ref.(KO)N.
 WD2132+096    See also (MR)
 WD2134+125    High gravity PG1159-like central star of NGC7094, type lgEH, Ref.(66) CSPN effective temperature 125,900K. (IO)N.
 WD2134+218    See also (NB)
 WD2136+828    See also (NL)
 WD2137+102    See also (NC)
 WD2140+207    Weak C2 reported, Ref.(5D) See also (NB)
 WD2144+128    See also (NC)
 WD2146+005    See also (MV)
 WD2146+412    Reclassified as a helium strong sub-dwarf B star.(EG) The coolest known DBA white dwarf; TEFF= 12,500K, Ref.(62).
 WD2146-077    See also (MV)
 WD2147+280    G188-27 shows weak HeI; coolest DB? Ref.(CE).
 WD2148-075    See also (NC)
 WD2149+000    See also (NC)
 WD2149+002    See also (MV)
 WD2149+021    See also (MR)(NB)(NL)
 WD2149+126    See also (MV)
 WD2150-008    See also (NC)
 WD2151+125    See also (NC)
 WD2151-015    Companion VR0 = +6.8 (EE) see section A5.17 in Ref.(LJ) see also (MY)
 WD2152-310    ZZ Ceti candidate (HC)
 WD2153-419    See also (JV)
 WD2154+408    WD2154+408 is a PCEB binary (P=0.26772 day) consisting of a hot white dwarf primary and a cool late MS companion. (HF)
 WD2154-512    See also (JV)
 WD2155-009    See also (NC)
 WD2157-074    See also (NC)
 WD2200+113    See also (NC)
 WD2200-000    See also (NC)
 WD2201-005    See also (NC)
 WD2202-282    ZZ Ceti candidate (HC)
 WD2203+005    See also (NC)
 WD2204-005    See also (NC)
 WD2204-012    See also (NC)
 WD2206+121    See also (NC)
 WD2207-004    See also (NC)
 WD2207-303    See also (NL)
 WD2211+372    See also (MQ)
 WD2211-316    ZZ Ceti candidate (HC)
 WD2211-495    See also (MV)
 WD2212+656    The DA degenerate central star of IW2, Ref.(7U).
 WD2213+007    See also (NC)
 WD2213+125    See also (NC)
 WD2214+005    See also (NC)
 WD2215+388    GD 401 is a DB degenerate with upper limit calcium and magnesium abundances, Ref.(49).
 WD2215-002    See also (MV)
 WD2216+484    GD402   probable unresolved DA+DC system, Ref.(23).
 WD2216-000    See also (NC)
 WD2216-657    L119-34, DZ star with rare carbon, Ref.(DE).
 WD2218+002    See also (NC)
 WD2218+706    The DA central star of DEHT5, Ref.(7U).
 WD2220+124    See also (NC)
 WD2220+133    See also (MY)
 WD2221-165    See also (MR)
 WD2223+130    See also (NC)
 WD2224-004    See also (NC)
 WD2226+139    See also (NC)
 WD2226-007    See also (NC)
 WD2226-210    Hydrogen dominated CSPN Ref.(KL)
 WD2226-754    Wide CPM pair with WD2226-755 Ref. (FF)
 WD2226-755    Wide CPM pair with WD2226-754 Ref. (FF)
 WD2227-010    See also (NC)
 WD2227-010.1  See also (NC)
 WD2228+126    See also (NC)
 WD2229+235    See also (MR)
 WD2230+125    See also (NC)
 WD2230-125    See also (MR)
 WD2231-005    See also (NC)
 WD2232+009    See also (NC)
 WD2233+142    See also (NC)
 WD2234-095    See also (NC)
 WD2235-305    ZZ Ceti candidate (HC)
 WD2237+143    See also (NC)
 WD2237-365    This is NOT LHS 3841 = LP 984-76 = Lephm 1-4978 as reported elswhere as per J.Farhi private communication 9/29/09 <A HREF='../Misc/WD2237-365.jpg')">Finding Chart</A>) 
 WD2238-098    See also (NC)
 WD2239+001    See also (NC)
 WD2240+125.1  A visual double DA binary, Ref.(2T).
 WD2240+125.2  A visual double DA binary, Ref.(2T).
 WD2241+009    See also (NC)
 WD2242-002    See also (NC)
 WD2244+030    = PG2244+031 Star A is the WD. <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.19.html'>  Finding Chart</A> see A5.12 in Ref.(LJ) Also see WD2244+031
 WD2244+031    Acccording to section A5.12 in Ref.(LJ) the star at these coords is a G5 and the info from Ref.(1P) belongs to 22 44 49.7 +03 05 54(1950) = WD Catalog number WD2244+030
 WD2245+146    See also (MV)
 WD2246+223    See also (MY)(NB)(NL)
 WD2246-001    See also (NC)
 WD2246-105    See also (NC)
 WD2248+293    See also (NN)
 WD2249-105    See section A5.10 in Ref. (LJ).
 WD2250-093    See also (NC)
 WD2251-070    See also (NN)
 WD2252-005    See also (NC)
 WD2253+054    Very weak spectrum, common proper motion pair.
 WD2253-081    G156-64 common proper motion binary with BD-8 5980 (G6 dwarf).
 WD2254+126    ZZ Ceti star ref.(KA)
 WD2256+249    GD245 is a composite DA + dM pre-cataclysmic binary, Ref.(9V) see also (MY)
 WD2257-073    DA + G5V binary, REF.(14).
 WD2258+134    See also (NC)
 WD2300-008    See also (NC)
 WD2301-072.1  CPM WD component with M > 15.0, Ref.(3A).
 WD2301-072.2  CPM WD component with M > 15.0, Ref.(3A).
 WD2303+242    KR Peg is a ZZ CETI variable, Ref.(44).
 WD2304+251    White dwarf companion to the mild barium star 56 PEG; may have accretion disk, Ref.(9T).
 WD2309+006    See also (NC)
 WD2309+007    See also (NC)
 WD2309+105    See also (JV)(MZ)(NL)
 WD2310+005    See also (NC)
 WD2313-313    ZZ Ceti candidate (HC)
 WD2315+003    See also (NC)
 WD2315-098    See also (NC)
 WD2316+123    New magnetic degenerate, with a 30Mg field, Ref.(5U).
 WD2316-011    See also (NC)
 WD2316-064    See also (MW)(NN)
 WD2316-098    See also (NC)
 WD2316-173    IUE detection of CaII 1840A, Ref.(4L); strong UV CI lines, Ref.(CK).
 WD2317+008    See also (MV)
 WD2317-295    ZZ Ceti candidate (HC)
 WD2318+009    See also (NC)
 WD2319+691.1  = A on <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.8.html'> Finding chart for GD 559B</A> Ref.(LJ)
 WD2319+691.2  = B on <A HREF='http://www.iop.org/EJ/article/0067-0049/161/2/394/62424.fg4.8.html'> Finding chart for GD 559B</A> Ref.(LJ)
 WD2319-012    See also (NC)
 WD2320+003    See also (MV)
 WD2321+005    See also (NC)
 WD2321-010    See also (MV)
 WD2321-549    See also (JV)
 WD2322-011.1  See also (NC)
 WD2322-097    See also (NC)
 WD2323+157.2  Atmosphere virtually devoid of Hydrogen; Coolest known He atmosphere WD; Teff~3650K; Common proper motion pair with WD2323+157.1 (GD) Authors have witdrawn this paper. Star is a background subdwarf K7/M0 see A3.1 Ref.(LJ) see http://xxx.lanl.gov/abs/astro-ph/0207265
 WD2323-006    See also (NC)
 WD2323-014    See also (NC)
 WD2324+397    Peculiar PG1159-like degenerate star of type lgEH, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N.
 WD2326+049    G029-038 is a ZZ CETI variable, Ref.(AE)(JE)(MR), Contains circumstellar dust (NG) See also (NL)
 WD2326-001    See also (NC)
 WD2326-004    See also (NC)
 WD2329+134    See also (NC)
 WD2329+267    See also (MV)
 WD2329-090    See also (NC)
 WD2330-296    ZZ Ceti candidate (HC)
 WD2331+290    Newly identified double degenerate close binary, Ref.(7G).
 WD2331-005    See also (NC)
 WD2331-475    See also (MV)(NB)(NL)
 WD2333+301    WD associated with PN; Type: E Ref.(KL)
 WD2333-007    See also (NC)
 WD2335+305    JN1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type E, Ref.(66).
 WD2335-002    See also (NC)
 WD2336-005    See also (NC)
 WD2336-006    See also (NC)
 WD2337-760    Double-degenerate candidate Ref.(KP).
 WD2338+003    See also (NC)
 WD2339+157    See also (NC)
 WD2339-100    See also (NC)
 WD2341+322    EG162 common proper motion binary with G130-6 (M3 dwarf) See also (NL)
 WD2342+806    GD561, the DAO central star of a newly discovered planetary nebula, Ref.(7T).
 WD2343+386    See also (MV)
 WD2343-005    See also (NC)
 WD2343-008    See also (NC)
 WD2343-106    See also (MV)
 WD2344-006    See also (NC)
 WD2345-089    See also (NC)
 WD2345-313    ZZ Ceti candidate (HC)
 WD2347+128    ZZ Ceti star ref.(KA)
 WD2348-011    ZZ Ceti star Ref.(KB)
 WD2348-244    EC23487-2424 is a ZZ CETI variable, Ref.(44).
 WD2349+286    See also (NL)
 WD2349-283    See also (MQ)
 WD2350-083    The finding Charts place this star at 23 53 27.6 -8 4 41(2000) near the position of G273-B1A not G273-B1B.
 WD2350-279    ZZ Ceti candidate (HC)
 WD2351+650.1  CPM WD component with M > 15.0, REF.(3A).
 WD2351+650.2  CPM WD component with M > 15.0, REF.(3A).
 WD2351-335    Triple system DA5.5+dM3.5+dM8 see A5.3 in Ref.(LJ)
 WD2351-368    See also (MV)
 WD2352+401    G171-027 has weak C2, Ref.(CE).
 WD2357+296    See also (NL)
 WD2359-434    See also (NB)