| GCVS-Name | Other-Name | Notes |
|---|
| BE Oct | S 6633 | object in outburst; period 0.0747d (2003-82) is estimated from the
superhump period using the empirical relation given by Stolz, B. and
Schoembs, R. 1984, Astron. Astrophys., 132, 187 |
V402 And | Antipin V62 | period 0.0621d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Peg1 | PG 0008+185 | featureless hot continuum, possible DC white dwarf | DK Cas | 244.1940 | Sumner (ftp://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/sumner
/dkcas.seq) states that the southwest component is the variable | V513 Cas | MacC v4 | a spectrum by 1997-07S shows H-alpha emission on a reddish continuum | HP And | SVS 71 | faint and nebulous; flagged object confirmed as a galaxy
(EO1243-0297148; Nogami et al. 2003, IBVS 5116) | QR And | RX J0019.8+2156 | HST data is spectroscopic (STIS) | VW Tuc | HV 6327 | in the direction of, but probably not a member of, the SMC (1995-42) | CM Phe | Phe1/JL 181 | object is not to be identified with NSV 137, BPM 16078, or L 218-28
(Hoard, D.W., Wachter, S., and Kim-Quijano, J. 2001, PASP, 113, 482) | And | FBS 0019+348 | classification based on unpublished spectrum | V410 Cas | S 10141 | a spectrum by 1997-07S is that of a DA white dwarf or possibly a CV in outburst | Tuc | NGC 104-W85 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104-W82 | HST data is imaging (WFPC2) | Tuc | NGC 104-W56 | HST data is imaging (WFPC2) | Tuc | NGC 104-W55 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104-W53 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104-W51 | HST data is imaging (WFPC2) | Tuc | NGC 104-W49 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104-W44 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104-W45 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104-W122 | HST data is imaging (WFPC2) | Tuc | NGC 104-W42 | finding chart on stacked image courtesy of R. Gilliland;
period 0.25d (1992-30) is uncertain/unreliable; HST data is imaging (WFPC2) | Tuc1 | NGC 104 PC1-V47 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (FOC, WFPC2) | Tuc | NGC 104 WF4-V16 | HST data is imaging (WFPC2) | Tuc | NGC 104-W34 | possible millisecond pulsar; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Tuc | NGC 104 AKO9 | coordinates converted to reference frame of Geffert et al (1977,
Astron. Astrophys., 327, 1370; HST data is imaging (WFPC2, STIS) and
spectroscopic (STIS) | Tuc | NGC 104-W35 | exact position in image from R. Gilliland; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Tuc | NGC 104-W33 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104-W31 | exact position in image from R. Gilliland; possible millisecond
pulsar; finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104-W32 | classified based on Chandra data | Tuc | NGC 104 PC1-V53 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (FOC, WFPC2) and
spectroscopic (FOS); period 0.25d (1998-46) is uncertain/unreliable | Tuc | NGC 104-W27 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104 PC1-V52 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104-CV3 | coordinates converted to reference frame of Geffert et al. (1997, Astron.
Astrophys., 327, 137); HST data is imaging (WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 PC1-V36 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104-W25 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104-W21 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104-W20 | classified based on Chandra data | Tuc | NGC 104-W15 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104-W16 | classified based on Chandra data | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104 CV | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (STIS, WFPC2) | Tuc | NGC 104-W140 | no candidate, field map shown; HST data is imaging (WFPC2) | Tuc | NGC 104 Edmonds V5 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137) | Tuc | NGC 104-W10 | classified based on Chandra data | Tuc | NGC 104-W71 | exact position in image from R. Gilliland; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Tuc | NGC 104-W8 | exact position in image from R. Gilliland; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Tuc | NGC 104-W120 | HST data is imaging (WFPC2); period 0.22d (2003-78) is
uncertain/unreliable | Tuc | NGC 104-W70 | finding chart on stacked image courtesy of R. Gilliland;
HST data is imaging (WFPC2) | Tuc | NGC 104 WF4-V26 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (WFPC2) | Tuc | NGC 104 WF2-V30 | HST data is imaging (WFPC2) | Tuc | NGC 104-W2 | exact position in image from R. Gilliland; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Tuc | NGC 104 WF2-V48 | coordinates converted to reference frame of Geffert et al. (1997,
Astron. Astrophys., 327, 137); HST data is imaging (WFPC2) | Tuc | NGC 104-W1 | exact position in image from R. Gilliland; finding chart on stacked image
courtesy of R. Gilliland; HST data is imaging (WFPC2) | Psc3 | NSV 15086 | the object is also catalogued as a galaxy (PGC 1528 = UM 239),
but appears stellar; also known as FBS 0022-021 | Tuc | NGC 104-B7 | no candidate, field map shown | Psc | ASAS J002511+1217.2 | also known as RX J0025.1+1217; period 0.0562d (2005-57) is estimated from the superhump period using the empirical relation given by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V709 Cas | Cas2; RX J0028+5917 | HST data is spectroscopic (STIS) | LS And | NSV 191 | in the direction of, but probably not a member of, M31 (1995-42) | And | NSV 15112 | no candidate, field map shown | Cet6 | KUV 00311-1938 | BL Lac object | VZ Tuc | HV 6334 | no candidate, field map shown; a member of the
SMC (1995-42) | Psc | NSV 206 | does not exist | LT And | M31 V0011 | in the direction of, but not a member of, M31 (1995-42) | And | S 10754 | also known as M31 V49; in the direction of, but not a
member of, M31 (1995-42); no candidate, field map shown | And | NSV 238 | in the direction of, but probably not a member of, M31
(1995-42);
no candidate, field map shown | KP Cas | S 3865 | object is in outburst on POSS-II J plate (1989.667) | PT And | Rosino N 15 | object blue on POSSII, as is the brighter star to the northeast;
unusual recurrent nova in M31 or possible dwarf nova in the Galaxy | HV And | S 10777 | HST data is spectroscopic (STIS) | And | Rosino N 66 | also known as Rosino N 81 and M31 V609; in the direction of,
but not a member of, M31 (1995-42); visible on POSS I (?); no candidate, field map shown | And | Rosino N 39 | also known as M31 V665 and Hubble N 62; in the direction
of, but not a member of, M31 (1995-42); a second outburst was recorded
in 1962.85; no candidate, field map shown | LL And | | HST data is spectroscopic (STIS) | And | Rosino N 48 | also known as Rosino N 79 and M31 979; in the direction
of, but not a member of, M31 (1995-42); no candidate, field map shown | And | D31J04306.4+413013 | finding chart from A. Bonanos | And | XMMU J004308+411247 | likely an dipping X-ray source in M31 rather than a galactic magnetic CV | Cet | SDSS J004335-003729 | period 0.056d (2004-45) is uncertain/unreliable | BL Psc | RE 0044+093 | K V plus white dwarf? | IO And | S 10785 | low redshift (z=0.134) Seyfert I galaxy | And | NSV 312 | if a nova, probably a distant member of M31; no candidate,
field map shown | And | NSV 313 | if a nova, probably a distant member of M31; no candidate,
field map shown | Psc | PG 0048+091 | subdwarf B star | V452 Cas | S 10453 | in outburst; period 0.0846d (2003-95) is estimated from the superhump
period using the empirical relation given by Stolz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | Psc1 | PG 0051+169 | subdwarf B star | Scl2 | LTT 560/G 269-70 | white dwarf + late-type star | RX And | 1E 0101+4101 | HST data is spectroscopic (GHRS) | V723 Cas | | HST data is imaging (NICMOS) | Scl | 2QZ J010946.1-274524 | flagged object is much brighter than quoted magnitude -in outburst? | Psc | | F-type star | HT Cas | S 3343 | HST data is spectroscopic (FOS) | V418 Cas | S 9142 | Mira variable | And3 | NSV 447 | no candidate, field map shown; flagged object appears
blue on POSS II plates | BE Tuc | HV 2205 | red colors, no line emission in spectrum | WX Cet | BV 416 | HST data is spectroscopic (STIS) | Psc | NSV 15271 | no candidate, field map shown | Cas3 | ISV 0115+63 | coordinates based on finding chart; no candidate, field map shown | AH Psc | BD +8 215 | no candidate, field map shown; missing BD star | UY Phe | S 7154 | RR Lyrae variable | Hyi | RX J012254.1-752117 | PG1159 star | TY Psc | S 10900 | HST data is spectroscopic (STIS) | AS Psc | S 10828 | finding chart from J. Thorstensen; object is extremely
blue (U-B=-1.25) | Cet | SDSS J013132-090122 | HST data is imaging (ACS) and spectroscopic (ACS) | TU Tri | GR 287 | A spectrum by 2000-01S reveals a very blue continuum, with no strong
emission. However, weak emission cannot be ruled out due to the low
signal-to-noise of the data; period 0.0724d (2005-07) is estimated
from the superhump period using the empirical relation given by Stolz,
B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Tri | NSV 15358/S 10832 | AGN (z=0.257) | BL Hyi | H 0139-68 | HST data is spectroscopic (STIS) | Psc | HS 0139+0559 | = PHL 1111? | Tri | RX J0146.8+3152 | quasar | For2 | GD 1401 | detached white dwarf-red dwarf; J2000 coordinates for
epoch J1977.927 | Ari | SDSSp J015151+140047 | also known as PG 0149+137 | Cas | RX J0153.3+7446 | HST data is spectroscopic (STIS) | Cas4 | Lanning 159 | A spectrum by 2000-01S shows an early-type spectrum with moderate strength Balmer absorption. Object is either in outburst, has an optically thick disk seen face-on, or is not a CV | Cet | SDSSp J015543+002807 | in low state on GSC plate (1983.691) | UZ Tri | S 10911 | nebulous object nearby is a background galaxy (Bond, private communication) | For | 2QZ J015940.6-281040 | large outburst (Schmeer, private communication) indicates
ug or ugwz type | Cet | PG 0157+001 | Seyfert I galaxy | Cet | FBS 0204-024;PB 6657 | B star, possibly Be | TT Ari | BD +14 341 | in bright state on POSS II F image shown;
HST data is spectroscopic (FOS) | WX Hyi | HV 8016 | HST data is spectroscopic (GHRS) | UV Per | 87.1911 | HST data is spectroscopic (STIS) | UW Per | 21.1912 | object (not visible) near center of circle shown | TZ Per | 28.1912 | HST data is spectroscopic (STIS) | For | 2QZ J021927.9-304545 | period 0.0784 (2005-114) is estimated from the superhump
period using the empirical relation given by Stoltz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | And | TSS J022216.4+412260 | no candidate, field map shown; period 0.0546 (2005-112) is
estimated from the superhump period using the empirical relation given
by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Cep2 | NSV 786 | late F-star; also known as BD +78 79 | XX Cet | PHL 4037 | quasar | WY Tri | S 10919 | period 0.07597d (2001-08) is estimated from the superhump period
using the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | RW Tri | 5.1938 | HST data is astrometric (FGS) and spectroscopy (GHRS) | PQ And | TAV 0226+39 | period 0.0560 (2005-116) is uncertain/unreliable | Per | NSV 837 | no candidate, field map shown | Cet5 | NSV 870 | no flickering reported by Haefner, R., Fielder, A., and Rau, S. (1996, IBVS, 4366) | Per | NSV 895 | possible supernova in irregular galaxy UGC 2172 = MCG 7-6-55; coordinates
based on the finding chart; no candidate, field map shown | PU Per | S 9727 | period 0.0713d (1999-101) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | PT Per | S 9530 | the spectrum is that of a late B star, perhaps observed during
outburst or wrong object observed | Cet1 | PG 0240+066 | no flickering reported by 1995-35; the spectrum shows a weak emission component in the red wing of the Balmer lines (1999-09S), so the identification as a CV is still in question | PV Per | S 9728 | period 0.0778 (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Ari | NSV 907 | flagged object blue on POSS II plates; possible ROSAT ID is 1RXS
J0244+2731; period 0.0703d (2004-83) is estimated from the superhump
period using the empirical relation given by Stolz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | UW Tri | SVS 2558 | marked object not visible on deeper POSSII-F plate; period 0.0561
(2001-27) is estimated from the superhump period using the empirical
relation given by Stolz, B. and Schoembs, R. 1984, Astron.
Astrophys., 132, 187 | RU Hor | HV 11902 | period 0.0697d (2003-105) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | SU Ari | BD +16 354 | missing BD star; coordinates in D+S are for Duerbeck's candidate 1,
which is a galaxy (Duerbeck, private communication). Coordinates
presented here are for candidate 2 (not visible on chart) | PY Per | S 9160 | in outburst on POSS II F plate shown | Cet | US 3215 | Seyfert 1 Galaxy | Cet2 | PG 0248+054 | no flickering reported by Haefner, R., Fielder, A., and Rau, S. (1996, IBVS, 4366) | V502 Cas | GR 195 | no candidate, field map shown | Oct | LB 9963 | =? GSC 9499-00510 | SY For | CoD -38 946/S 7603 | semiregular variable | XY Ari | H 0253+193 | Optically obscured by Lynds Dark Nebula LDN 1457 | LW Cas | SVS 1144 | T Tauri star | V664 Cas | Cas1; PK 136+5 1 | HST data is imaging (WFPC) | V400 Per | | period 0.179d (2005-05) is uncertain/unreliable | Per | FBS 0306+333 | coordinates refer to the combined light of a close pair; both
stars are late-type stars | CP Eri | PHL 1475 | HST data is spectroscopic (STIS) | Eri | EUVE J0311-2254 | no candidate, field map shown; the coordinates
listed in 1999, AJ, 117, 2466 differ by 9'' in declination
(47'' instead of 38'') | EF Eri | 2A 0311-227 | HST data is photometric (HSP) | QY Per | S 9178 | period 0.0761d (2000-19) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Per | BD +34 620;NSV 15667 | missing BD star; no candidate, field map shown | W Ari | BD +28 518 | missing BD star; no candidate, field map shown | FT Cam | Antipin V64 | also known as 1RXS J0321+6105; period 0.07499 (2002-76) is
uncertain/unreliable | SV Ari | 116.1905 | candidate not visible, field map shown | VX For | For3 | tentative identification; object blue on SERC plate | Per | CXOAYSB J033108+4357 | ID tentative, flagged object red on POSS | GK Per | BD +43 740a | HST data is imaging (WFPC2) and spectroscopic (STIS) | Per | CXOAYSB J033131+4356 | ID tentative, flagged object neutral-colored on POSS | Cam | Lanning 302 | single outburst observed; no candidate, field map shown | AF Cam | SVS 1153 | HST data is spectroscopic (STIS) | UZ For | EXO 033319-2554.2 | HST data is spectroscopic (FOS, STIS) | SZ For | PHL 4482? | quasar | CW Cam | BD +57 739 | irregular variable | V701 Tau | SVS 1972 | period 0.0672 (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | SZ Per | BD +33 715 | missing BD star; no candidate, field map shown | MR Per | S 8540 | M-star spectrum, possible flare star | V1212 Tau | NSV 15820 | object is blue on POSS II plates | Eri | 1RXS J035410-165244 | object flagged is variable between POSS I and UK plate shown | Tau2 | KUV 03580+0614 | HST data is spectroscopic (STIS) | Tau | RX J0403.1+0444 | flagged object blue on POSS II plates | FO Per | 22.1939 | period 0.18248 (2005-106) is uncertain/unreliable | MY Per | S 8548 | observations in 1999-08S reveal that the identification given in D+S
is correct | VW Hyi | RE J0409-7125 | HST data is spectroscopic (FOS, GHRS, STIS) | Tau | IRAS 04183+1619 | spurious notice, object is a red star | Eri | 1RXS J042556-194534 | period 0.0605 (2002-102) is uncertain/unreliable | Cam | NSV 16032 | no candidate, field map shown | TU Men | S 6732 | HST data is spectroscopic (STIS) | V392 Per | S 10653 | the chart in 1970-03 has the chart mislabelled as S 10652 | Per1 | NSV 1725 | late-A or early-F star | HV Aur | S 8480 | period 0.0823d (1995-38) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | RS Cae | Cae1; RX J0453-4213 | period 0.0708d (1996-06) is uncertain/unreliable | V1208 Tau | Tau3/RX J0459+1926 | period 0.0688d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | HY Eri | RX J0501-0359 | revised identification from Helmut Steinle | HW Tau | SVS 1023 | minor planet (49) Pales | AQ Eri | 431.1934 | HST data is spectroscopic (STIS) | Cep | HS 0455+8315 | HST data is spectroscopic (STIS) | Dor | RX J0507.1-6743 | no identified candidate, field map shown; object is either a CBSS in
the LMC or a soft foreground cv | Cam | HS 0506+7725 | also known as 1RXS J051336.1+772836 | RY Dor | HV 4004 | a member of the LMC (C1995-12); no candidate, field map shown | V1309 Ori | Ori1; RX J0515+0104 | HST data is spectroscopic (FOS) | XX Tau | 100.1927 | period 0.136d (2005-05) is uncertain/unreliable | Men | OGLE 051955-702753 | possibly in LMC | GR Ori | 2.1916 | candidate not visible, field map shown | ZZ Lep | HD 35914 | central star of planetary nebula PK 215-24 1. The paper referenced for
type does not mention novalike classification, although 75th Namelist
(Kazarovets, E.V., Samus, N.N., and Durlevich, O.V. 2000, IBVS, 4870)
bases classification on the paper; HST data is imaging (WFPC, WFPC2)
and spectroscopic (STIS, GHRS) | TV Col | 2A 0526-328 | close double; HST data is astrometric (FGS) | V650 Ori | S 9560 | star observed in 1998-03S is previous, incorrect candidate | UW Pic | Pic1; RX J0531-4624 | northern object of close pair; HST data is spectroscopic (STIS) | T Aur | BD +30 923a | HST data is imaging (WFPC2) and spectroscopic (STIS) | Cam | 1RXS J053234+624755 | period 0.0563d (2005-64) uncertain/unreliable | TW Pic | H 0534-581 | period 0.265d (2000-97) is uncertain/unreliable | Dor | CAL 86 | in the direction of the LMC; object bright on plate 05ZW
(1987.06); period 0.0661 (2005-99) is uncertain/unreliable | FS Aur | S 3946 | HST data is spectroscopic (STIS) | V421 Tau | S 10491 | minor planet (586) Thekla | LS Cam | HS 0551+7241 | flagged object barely visible on POSS II J plate A2JQ
(1996.87), but is much brighter on POSS II J plate A08E (1991.93); HST
data is spectroscopic (STIS) | V405 Aur | Aur1; RX J0558+5353 | HST data is spectroscopic (STIS) | V529 Ori | | a spectrum of the nova candidate is given in 2000-28; the
emission-line candidate (number 5) found by Fienberg (1995, Sky
Telesc. 89, No. 3, 11; labelled as 5 in the chart) has subsequently
been shown to be a visual binary (separation 1.1'') with emission-line
M0 and K7 stars (Ringwald and Naylor, 1997, Astron. Astrophys. 326,
629) | HM Gem | S 8466 | measured object is real, as it appears in both the USNO-A1.0 and
USNO-A2.0 catalogs | AD Men | HV 12703 | in the direction of, but not a member of, the LMC (1995-42); object
observed in 1995-07X is the bright star about 40'' southwest of AD Men | Gem | NGC 2158 V57 | status as a cluster member is uncertain; object in outburst on POSS II
plate (shown above) obtained on 1992.066 | V347 Pup | Pup2; LB 1800 | HST data is spectroscopic (FOS) | Gem1 | NSV 2853 | identification uncertain; no flickering reported by Haefner, R., Fielder, A., and Rau, S. (1996, IBVS, 4366); a spectrum by 2000-01S is that of a late-G star. The object may be mid-identified, and may be the star to the southwest
of the marked object | AH Men | Men1; 1H 0551-819 | object is southeast component of blended double shown | SS Aur | 31.1907 | HST data is astrometric (FGS) and spectroscopic (STIS) | Aur2 | NSV 2872 | early-K star spectrum (2000-01), but object shows flickering | Cam | 1RXS J0625+7334 | HST data is spectroscopic (STIS) | KT Mon | | no candidate, field map shown | BZ Cam | 0623+71 | HST data is spectroscopic (GHRS) | CI Gem | S 3428 | object detected in outburst (1999), and is 0.15s east and 6.7'' south of previous position; not visible on POSS | RR Pic | He 3-15 | HST data is imaging (WFPC2) | KN Gem | AN 645.1936 | minor planet (123) Brunhild; postdiscovery observations attributed
to KN Gem in fact refer to the Mira variable BR Gem | Cam | RX J0636.3+6554 | object not marked in 1998-23, but coordinates reveal the only object in
the error circle is the identification | UV Gem | 18.1916 | period 0.089d (2002-130) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | SY Gem | BD +31 1380 | missing BD star? A declination error in the BD
is possible: there is a bright double (GSC 2435-00868/872),
obvious on the plate shown, 1.9 arcminute south of the
nominal BD position. Spectra by 1997-07S of Duerbeck's
candidates 1 and 2 (= GSC 2435-00868) show neither has a
CV-like spectrum | BT Mon | 67.1939 | HST data is imaging (WFPC2) | CMa | RX J0643-2052 | no candidate, field map shown | DM Gem | HD 48328 | period 0.1228d (2000-84) is uncertain/unreliable | HL CMa | 1E 0643-1648 | finding chart from J. Thorstensen | EQ Mon | 92.1936 | red star | Gem | NSV 3313 | no candidate, field map shown | MV Gem | S 10220 | mid-F dwarf | V838 Mon | | HST data is spectroscopic (STIS) and imaging (ACS) | CG CMa | | object not visible, but outburst image shows it immediately east of
nearby star; period 0.0623d (1999-83) is estimated from the superhump
period using the empirical relation given by Stolz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | LW Cam | RX J0704.2+6203 | flagged object blue on POSS II plates | EU CMa | S 7991 | in outburst on POSS I plate | CMi | NSV 3432 | no candidate, field map shown | HQ Mon | 93.1933 | period 0.316d (2003-27) is uncertain/unreliable | WY CMa | | F2 III star | V348 Pup | Pup1; 1H 0709-360 | HST data is spectroscopic (FOS) | AQ CMi | 14.1934 | period 0.0648d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | FQ Mon | 107.1936 | ROSAT ID is RXS J071641.6-065653; period 0.0665 (2004-111) is
estimated from the superhump period using the empirical relation
given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | IN CMa | RE 0720-318 | pre-cataclysmic variable | AW Gem | 8.1933 | period 0.07684d (1998-46) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | HM Aur | BV 23 | late-M star | CL Pup | S 4069 | possible rapid irregular variable | KQ Mon | 119.1943 | period 0.128d (2005-48) is uncertain/unreliable | BG CMi | 3A 0729+103 | HST data is photometric (HSP) | Cam2 | FBS 0726+728 | DA white dwarf | V574 Pup | Nova Pup 2004 | no candidate, field map shown | V436 Car | Car1; RX J0744-5257 | near HD 63177 | Lyn | SDSSp J074716+424849 | HST data is spectroscopic (STIS) | PQ Gem | RE 0751+14 | HST data is spectroscopic (FOS) | V716 Mon | NSV 3775 | RR Lyrae star | BX Pup | | in NGC 2482 | U Gem | BD +22 1807 | HST data is astrometric (FGS) and spectroscopy (GHRS, FOS) | Pup | NSV 3846 | no candidate, field map shown; 1990-29 note
that the spectrum of Duerbeck's candidate shows narrow Balmer
absorption superimposed on a blue continuum | Cam | SBS 0755+600 | object in outburst on POSS-I plate (1954.012); photometry by
J. Thorstensen (private communication) shows the object with V=19.84,
(U-B)=-0.96, (B-V)=0.00, (V-I)=+0.94. The object to the southeast is
also blue, with (U-B)=-0.65, (B-V)=+0.11, (V-I)=+0.08, and V=20.23. | Cnc | SDSS J080303+251627 | southwest star of pair | Cnc | RXS J0806.3+1527 | note dec sign error in original reference (1999-12S) | Z Cha | S 4893 | HST data is photometric (HSP) and spectroscopic (FOS) | VZ Gem | BD +31 1736 | no candidate, field map shown; missing BD star | Lyn | SBS 0804+563 | weak Balmer absoprtion | Lyn | SDSS J080908+381406 | HST data is spectroscopic (STIS) | Vel | CPD -48 1517 | typographical error in original reference (really refers
to IX Vel = CPD -48 1577) | YZ Cnc | BV 131 | HST data is astrometric (FGS) | V351 Pup | | HST data is imaging (WFPC2) | CP Pup | He 3-130 | HST data is imaging (WFPC2) | Cnc | SDSS J081352+281317 | object in possible low state on POSS II plate (1989.837) | VV Pup | 1E 0812-1854 | HST data is spectroscopic (STIS) and photometric (HSP) | IX Vel | CPD -48 1577 | HST data is spectroscopic (STIS) | BH Lyn | PG 0818+513 | HST data is spectroscopic (STIS) | Cam3 | FBS 0827+738 | late-F to early-G star | DE Cnc | S 10803 | featureless continuum | SW UMa | 44.1909 | HST data is spectroscopic (STIS) | BB Vel | | close pair | AA Cnc | G 40-31 | M star spectrum, possible flare star | Lyn | SDSS J083751+383012 | secondary star visible in spectrum | RX Vol | S 6185 | flagged object is a close E-W pair (2.3'' separation), with the
eastern object being the variable; period 0.0601d (2003-82) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | EG Cnc | | HST data is spectroscopic (STIS) | FV Cnc | HIP 43199 | G0-4 star | CT Hya | 114.1936 | period 0.06495 (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | EU Cnc | M67-186 | our coordinates are 0.8s west and 12" north of 1995-41 | BZ UMa | PG 0849+580 | HST data is spectroscopic (STIS) | Cnc | SDSS J085623+310834 | spectrum of white dwarf primary visible | CQ Vel | | objects shows flickering | Lyn | SDSS J090016+430118 | period 0.221d (2004-45) is uncertain/unreliable | BP Lyn | Lyn1; PG 0859+415 | HST data is spectroscopic (STIS) | BI Lyn | PG 0900+401 | detached system | T Pyx | HV 3348 | HST data is imaging (WFPC2) | Hya | SDSS J090628+052656 | secondary star visible in spectrum | Lyn | NSV 4394* | also known as SN 1972 delta; no candidate, field map shown | GY Cnc | RX J0909.8+1849 | HST data is spectroscopic (STIS) | Cnc | SDSS J091137+084140 | not visible on POSS II plates, possible dwarf nova; secondary star visible in spectrum | Car | NGC 2808-397 | coordinates from HST image o60102f4q; HST data is imaging (STIS) | Car | NGC 2808-170 | coordinates from HST image o60102f4q; HST data is imaging (STIS) | Car | NGC 2808-222 | coordinates from HST image o60102f4q; HST data is imaging (STIS) | Pyx | | no candidate, field map shown | UMa | SDSS J091935+502825 | spectrum of secondary star visible | Cnc | SDSS J091945+085710 | spectrum of white dwarf primary visible | BK Lyn | PG 0917+342 | HST data is spectroscopic (STIS) | UMa | SDSS J092219+421256 | spectrum of white dwarf primary visible | Leo | SDSS J092444+080150 | spectrum of secondary star visible; period 0.88d (2005-32) uncertain/unreliable | Leo | HS 0922+1333 | magnitude unreliable due to peculiar spectral energy distribution | Leo | NSV 4498 | no candidate, field map shown; no flickering
reported by Haefner, R., Fielder, A., and Rau, S. (1996, IBVS,
4366) for stars in the field | MN Hya | Hya4; RX J0929-2404 | HST data is spectroscopic (FOS) | TU Leo | SVS 167 | object confused with minor planet (8) Flora | Lyn2 | KUV 09313+4052 | flagged object distinctly blue (2005-15) | Leo | NSV 4550 | no candidate, field map shown; object is possibly HD 83225 =
BD +15 2083 (1878-01) | Leo7 | NSV 18241 | also known as PG 0935+075 | Sex | RX J0944.5+0357 | HST data is spectroscopic (STIS) | Leo | HS 0943+1404 | period 0.174 (2005-51) is uncertain/unreliable | DV UMa | US 943 | HST data is spectroscopic (STIS) | LMi | FBS 0946+362 | G star | Sex1 | PG 0947+036 | white dwarf | RZ LMi | PG 0948+344 | period 0.0585d (1995-74) is estimated from the superhump period using the empirical relation given by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | KR UMa | standard 5 for QSO | G or K star | UMa2 | PG 1002+506 | binary with hot subdwarf; note that 1997-07X postulate the object as being a nearly pole-on CV | OY Car | S 6302 | HST data is spectroscopic (FOS, STIS, GHRS) | Sex | ROTSE3 J100932.2 | complete name is ROTSE3 J100932.2-020155 | CP Dra | | object blue on POSSII plate; period 0.0816d (2003-82) is estimated
from the superhump period using the empirical relation given by Stolz,
B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Car | NSV 18378 | no candidate, field map shown; object is No. 20
in reference 1978-01 | RW Sex | BD -7 3007 | HST data is spectroscopic (GHRS) | KS UMa | RX J1020+5304 | object is blue on POSSII plate; also known as SBS 1017+533;
HST data is spectroscopic (STIS) | HR Car | HD 90177 | S Dor type variable | UMa8 | NSV 4838 | object blue on POSS; spectrum (Thorstensen 2001, private communication) shows
broad H-alpha and H-beta emission | Sex | FIRST J102347+003841 | compact object in system may not be a white dwarf (2005-45) | U Leo | BD +14 2239 | missing BD star; variable object in Downes, R.A., and Szkody, P.
(1989, AJ, 97, 1729), marked on chart, has a G-type
spectrum (1990-29); the spectrum in 1996-14S is similar; period 0.2674d
(1998-46) is uncertain/unreliable | EP Car | | possible Mira variable | V411 Car | NSV 4884 | K1-2 III:e: star | DW UMa | PG 1030+590 | HST data is spectroscopic (STIS) | SS LMi | SVS 2506 | wrong target marked on chart in 2000-28 (which is inverted
mirror image) | RX Cha | S 6311 | period 0.081d (2001-38) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Car | NSV 18468 | object likely not real (1999-36); chart shown marks
Duerbeck's (1987-08X) candidate | Car | NSV 18473 | object not real, like an emulsion defect | RT Car | LSS 1855 | irregular variable | V382 Vel | | HST data is spectroscopic (STIS) and imaging (WFPC2) | V351 Car | BV 1543 | Mira variable | FH UMa | UMa9; WGA 1047+6335 | period 0.0556d (1996-10) is unreliable/uncertain | UMa5 | CW 1045+525 | HST data is spectroscopic (STIS) | Hya | RXS J105010-140431 | period 0.0615d (2001-55) is uncertain/unreliable | AG Car | PK 289-0 1 | S Dor type variable | CY UMa | SVS 2198 | object bright on POSS II plate (1995.234);
HST data is spectroscopic (STIS) | CN Vel | HD 95821 | the object is the east component of the faint optical double
(1996-01S); coordinates refer to combined light | AN UMa | PG 1101+453 | HST data is spectroscopic (STIS) | ST LMi | CW 1103+254 | HST data is photometric (HSP) and spectroscopic (FOS,STIS) | QU Car | HDE 310376 | HST data is spectroscopic (STIS) | FH Leo | HIP 54268 | late-F/early-G binary | Leo1 | PG 1104+022 | hot object; a spectrum by Li, Z.-Y., Liu, W., and Hu, J.-Y. (1999,
Chinese Astron. Astrophys., 23, 324) reveals strong Balmer absorptionm
with H-alpha partially filled-in | RS Car | HD 96830/HV 47 | period 0.0795d (2002-38) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V436 Cen | 1E 1111-3724 | HST data is spectroscopic (STIS) | UMa | SN 1985J; NSV 18704 | no candidate, field map shown | AR UMa | 1ES 1113+432 | HST data is spectroscopic (STIS) | CE UMa | | no candidate, field map shown; also SN 1966O (1995-42) | Leo2 | PG 1114+187 | precataclysmic variable | DP Leo | 1E 1114+182 | HST data is spectroscopic (FOS) | UMa3 | PG 1116+349 | hot object; Li, Z.-Y., Liu, W., and Hu, J.-Y. (1999, Chinese
Astron. Astrophys., 23, 324) classify the object as a binary | Leo6 | PG 1119+147 | no flickering reported by 1995-35; 1993-10S described the spectrum as having broad H-alpha and H-beta absorption with emission cores, while 1996-01S and 1999-09S shows only Balmer absorption | V442 Cen | HV 8364 | period 0.46d (1984-19) is uncertain/unreliable; HST data is spectroscopic (STIS) | Leo | 2QZ J112555.7-001639 | object is blue on POSS II plates | GU Mus | GRS 1121-68 | x-ray binary | AU Leo | S 8015 | galaxy | Leo3 | PG 1128+098 | hot object; Li, Z.-Y., Liu, W., and Hu, J.-Y. (1999, Chinese
Astron. Astrophys., 23, 324) classify the object as a binary
consisting of an early-F star and an O/B dwarf | UMa | 1RXP J113123+4322 | northern object of pair; period 0.0636d (2003-82) is estimated from
the superhump period using the empirical relation given by Stolz,
B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | TT Crt | FSV 1132-11 | HST data is spectroscopic (STIS) | T Leo | BD +4 2506a | HST data is spectroscopic (GHRS) | UMa4 | PG 1136+581 | starburst galaxy | Leo | | Star #6 in the field of RX J1142.7+2157
(ftp://ftp.hss.uni-hamburg.de/pub/outgoing/rass-id/rass2idv2_0.cat) | DO Dra | YY Dra? | HST data is spectroscopic (FOS) | MT Cen | | identification based on flickering data | Dra | SDSS J114628+675910 | period 0.067d (2003-22) is uncertain/unreliable | Leo | PG 1145+187 | DA White dwarf | Leo4 | PG 1146+228 | subdwarf B-O star; Li, Z.-Y., Liu, W., and Hu, J.-Y. (1999, Chinese
Astron. Astrophys., 23, 324) classify the object as a binary
consisting of an early-G star and an O/B component | EU UMa | RE 1149+28 | HST data is spectroscopic (FOS) | GQ Mus | | HST data is imaging (WFPC2), spectroscopy (FOS), and photometry (HSP) | BC UMa | GR 102 | HST data is spectroscopic (STIS) | SW Crt | SVS 2147 | A-star spectrum | UMa | SBS 1150+599A | halo planetary nebula; SBS 1150+599 is the bright galaxy to
the north of the marked object. The object with the PN spectrum, based
on positional coincidence, is marked on the chart. | LZ Mus | | no candidate, field map shown; period 0.1693d (1999-86) is
uncertain/unreliable | BE UMa | PG 1155+492 | detached binary with reflection effect | UMa | SN 1989Z? | near NGC 4013; object is visible projected against the disk of the galaxy | Vir | PG 1156-037 | subdwarf B star | Vir1 | PG 1157+004 | DA white dwarf | CP Cru | | HST data is imaging (WFPC2) | MU Cen | vG 41 | period 0.46d (1984-19) is uncertain/unreliable | EG UMa | Case 1 | detached white dwarf-red dwarf pair | CVn1 | NSV 5543 | object is very blue on POSS | Com | NSV 5550 | blue compact dwarf galaxy | Vir | PG 1217-067 | subdwarf B star | CG Mus | S 6398 | RR Lyrae star | Dra7 | FBS 1220+753 | the spectrum is that of an A star (1999-09S); 1995-12 claim the object shows emission. Either the object is not a CV, or is mis-identified (there is no published chart). | Cru | N Cru 2003 | no candidate, field map shown; object may be a nova, a
post-asymtotic-giant-branch star in flare-up, a V4332 Sgr-type object,
or a V838 Mon-type object | V373 Cen | vG 19 | object is a double | CQ Dra | 4 Dra b | CQ Dra is a Mira-type variable with a spectroscopic CV companion. It is not clear whether the system is triple (with the period quoted being the orbital period of a CV binary) or double (with the period quoted being the rotation period of an accreting magnetic white dwarf; coordinates are for the star 4 Dra (GSC 4394-01871); HST data is astrometric (FGS); 2003-72 claim the object is a symbiotic variable rather than a cv based on the x-ray properties | GT Com | | minor planet (679) Pax | IM Com | SVS 2819 | featureless continuum | AP Cru | 615.1936 | spectrum shows very narrow H-alpha emission | AL Com | Zw SN 106 | finding chart from J. Thorstensen; HST data is spectroscopic (FOS,STIS) | AM CVn | HZ 29/EG 91 | HST data is spectroscopic (GHRS, STIS) and astrometric (FGS) | V1025 Cen | RX 1238-38 | period 0.05876d (1998-14S) is uncertain/unreliable | IR Com | Com1; S 10932 | also known as RX J1239.5+2108 | Hya | NSV 19451 | this object is distinct from EW Hya; a spectrum of the flagged object shows that it is a late-G star (2004-23S), so the identification is likely incorrect | V591 Cen | HV 10172 | G5-8 V star | Vir5 | 1E 1240.8+0312 | also known as SDSS J124325+025548 (2003-22), NSV 19466 | TX CVn | BD +37 2318 | Z And type variable | FY Com | LV 13 | no candidate, field map shown; flagged object (12h 49m 19.14s,
+27d 24' 35.2'') is blue and is consistent with the discovery position | Dra | SDSS J125023+665526 | period 0.233d (2003-112) is uncertain/unreliable | EX Hya | 1E 1249-2858 | HST data is spectroscopic (FOS, STIS) and astrometric (FGS) | LW Hya | Hya3; Abell 35 | planetary-nebula nucleus | Com | NSV 19553 | also known as RE J1255+266; period 0.0830d (2005-60) uncertain/unreliable | V485 Cen | HV 10231 | HST data is spectroscopic (STIS) | RX Com | HV 3627 | Mira variable | Vir | PG 1257+010 | subdwarf B-O star | Cen | CTCV J1300-3052 | period 0.08898d (2004-58) is uncertain/unreliable | V888 Cen | | coordinates are centroid of close double, nova is the southern object | GP Com | G 61-29/Gr 389 | HST data is spectroscopic (FOS, GHRS) and astrometric (FGS) | BM Cha | S 6445 | T Tauri star | UMi | RX J1308+7026 | quasar | AU CVn | SVS 1254 | BL Lac | V396 Hya | CE 315 | HST data is spectroscopic (STIS) | V1043 Cen | RX J1313-3259 | HST data is spectroscopic (STIS) | NN Cen | HV 6432 | the object is a north-south double, with the CV being the north object | Oct | NSV 6101 | no candidate, field map shown | Vir2 | PG 1314+041 | subdwarf B star | Vir | PG 1315-123 | subdwarf B star | Dra1 | PG 1316+678 | DA+Me | V840 Cen | | Z And variable | V1047 Cen | Nova Centauri 2005 | no candidate, field map shown | HV Vir | NSV 6201 | a second outburst was recorded in 1992; HST data is spectroscopic (STIS) | V803 Cen | AE1 | period 0.01865d (1990-40) is uncertain/unreliable; HST data is spectroscopic (STIS) and astrometric (FGS) | Vir | SDSS J132411+032050 | magnetic CV with low accretion rate | Cen | NGC 5139-NV408 | object seen in outburst | Cen | NGC 5139-31 | type based on Chandra X-ray data only | Cen | NGC 5139-A | HST data is imaging (WFPC) | Cen | NGC 5139-B | HST data is imaging (WFPC2) | Cam | FBS 1330+837 | spectrum is that of a G star | CVn2 | NSV 6278 | M star spectrum, possible flare star | Mus | NSV 19878 | chart in 1984-01 incorrect; spectrum is Me, likely a symbiotic star | UMa | NSV 19892/GD 325 | DB white dwarf | UX UMa | SVS 365 | HST data is spectroscopic (GHRS, FOS) | UMa | SDSS J133941+484727 | spectrum of white dwarf primary visible | CVn | 1RXS J134210+282250 | in globular cluster NGC 5272; also known as 1E
1339.8+2837; HST data is imaging (WFPC2,ACS) | CVn | NGC 5272-7290 | HST data is imaging (WFPC2) | HS Vir | PG 1341-079 | period 0.0769 (2003-81) is uncertain/unreliable | CR Boo | PG 1346+082 | HST data is astrometric (FGS) | V890 Cen | Cen4; V1349-4754 | no candidate, field map shown | V868 Cen | | nova is southern object of close pair | V1039 Cen | | identification based on image in decline | BW Cir | 1354-64 | low mass X-ray binary | DR UMa | GR 296 | no confirmed candidate, field map shown; flagged object
is extremely blue [(U-B)=-0.7, V=19.9], although it is 25'' north
of the nominal position (J. Thorstensen, private communication) | Vir3 | PG 1403-111 | F-G star | Z Aps | HV 5060 | pulsating variable, possible a Cepheid | AB Boo | BD +21 2606? | no candidate, field map shown; the discovery (Schwab, 1901, Astr. Nachr., 155, 219)
was published 23 years after the fact, and gives a position to a precision of probably no
better than 0.5 degrees; there are no subsequent confirmed sightings | V834 Cen | 1E 1405-451 | HST data is photometric (HSP) and spectroscopic (STIS) | Cir | CG X-1 | may be a ULX in Circinus galaxy; period 0.304d uncertain/unreliable (2004-91) | T Boo | BD +19 2768a | 1990-29 note that the spectrum of candidate 2 of Downes, R.A. and Szkody, P. (1989, AJ, 97, 1729) is quite red, while the spectrum of candidate 5 is a featureless, blue continuum. 1996-14S also observed candidates 2 and 5, and found object
2 to be a K5-M4 star, while object 5 is that of an F2-9 star; candidate 1 was found to be a K3-5 dwarf | Vir | 2QZ J142256.3-022108 | period 0.1404 (2002-01) is uncertain/unreliable; also
known as SDSS J142256-022108 | DD Cir | | object not visible on image shown | Vir | 2QZ J142438.9-022739 | object blue on POSS II plates; period 0.1555 (2002-01)
is uncertain/unreliable | V895 Cen | Cen2; EUVE J1429-38 | HST data is spectroscopic (STIS) | Boo | SDSS J142955+414516 | period 0.059d (2005-32) uncertain/unreliable | Vir | SN 2001bn | blue variable with narrow Balmer absortion | HY Lup | | HST data is imaging (WFPC2) | OU Vir | Vir4/1432-0033 | object blue on POSS | V842 Cen | | HST data is imaging (WFPC2) | Boo | 1RXS J143704+234236 | object is very faint on GSC plate | X Cir | | identification based on flickering data; object is northeast
of bright star; spectrum of 2002-56 candidate in 2003-15S reveals a
red continuum with no emission | Boo | S 10808 | double exposure | UZ Boo | HV 10426 | period 0.125d (1987-05) is uncertain/unreliable | Boo | PG 1443+337 | DA white dwarf | Dra2 | PG 1445+583 | subdwarf B star | AR Cir | HV 2954 | nova is slightly NW of the bright object flagged, and is not resolved on this image; coordinates are for the companion star | AI Cir | HV 5121 | no candidate, field map shown | KV Dra | RX J1450.5+6403 | HST data is spectroscopic (STIS) | Lib3 | Preston 874124 | the spectrum is that of an B star (Liu, Hu, Li, and Cao (1999)). Either the object is not a CV, or is mis-identified (there is no published chart) | BZ Cir | Cir1; 1E 1449.8-6803 | period 0.0784d (1998-46) is uncertain/unreliable | TT Boo | HV 3681 | period 0.077d (1988-23) is uncertain/unreliable | Boo | SDSS J145758+514807 | spectrum of white dwarf primary visible | Lib1 | PG 1459-026 | subdwarf B star | Boo | SDSS J150722+523039 | spectrum of white dwarf primary visible | Dra8 | SN 1964O; SN s1964a | identification uncertain; although classified as a possible
supernova, there is no host galaxy visible on the POSS, so if
real, the object may be a nova. The coordinates of object B are
RA(2000) = 15h 8m 49s, Dec(2000) = +55 degrees 27' 51''. The
coordinates given by 1965-03 are RA(2000) = 15h 08m 50s,
Dec(2000) = 55 degrees 28' 07''. The spectrum of both candidate
objects are those of K stars (1999-09S) | Lib4 | IRAS 15075-0144 | a low redshift (z=0.037) AGN (= IRAS 15075-0144) | NY Ser | Ser1; NSV 6990 | HST data is spectroscopic (STIS) | EK TrA | S 5005 | close companion, object marked in D+S is incorrect, as true object is
brighter star to the southwest; HST data is spectroscopic (STIS) | Boo | SDSS J151413+454911 | spectrum of white dwarf primary visible | Ser | ROTSE3 J151453 | full name is ROTSE3 J151453.6+020934.2 | DE Cir | | no candidate, field map shown | CrB | PG 1517+265 | binary with hot subdwarf | GW Lib | | minimum magnitude is based on pre-outburst observations, while post-outburst observations show (as of 2004) that the object has faded to V~17; HST data is spectroscopic (STIS) | TrA1 | 1E 1516.6-6827 | north object of pair | Lib2 | PG 1520-050 | subdwarf B star | Ser2 | PG 1522+122 | subdwarf B star | IL Nor | HD 137677/HV 25 | no candidate, field map shown; our coordinates
are 1.1s west and 5'' south of Duerbeck | DM Dra | SVS 2426 | period 0.087d (1990-37) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | HP Lib | Lib5; EC 15330-1403 | HST data is astrometric (FGS) | Lib | ASAS 153616-0839.1 | period 0.0636d (2004-14) is estimated from the superhump period using the empirical relation by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Boo | SDSS J153817+512338 | period 0067d (2004-45) is uncertain/unreliable | IM Nor | HV 3532 | identification based on outburst observations; second outburst
detected on 2002.027 | V344 Nor | | possible Mira variable | AB Nor | HV 4908 | the object is the northernmost star in a small triangle, and is
slightly above quiescence on the SERC-J plate of 3 June 1975; period
0.0813d (2003-71) is estimated from the superhump period using the
empirical relation given by Stolz, B. and Schoembs, R. 1984, Astron.
Astrophys., 132, 187 | SS UMi | PG 1551+719 | HST data is spectroscopic (STIS) | MR Ser | PG 1550+191 | HST data is spectroscopic (STIS) | NN Ser | PG 1550+131 | precataclysmic variable (Ritter, H. 1986, Astron. Astrophys., 169,
139) | Dra | SDSS J155331+551615 | magnetic CV with low accretion rate | CrB | RX J1554.2+2721 | HST data is spectroscopic (STIS) | QZ Ser | HadV4 | HST data is spectroscopic (STIS) | VW CrB | CrB1; Antipin V21 | period 0.0707 (2003-94) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Nor | ASAS 160048-4846.2 | period 0.06338 (2005-36) is uncertain/unreliable | V345 Nor | NSV 7429 | Mira or Z And variable | Ser | SDSSp J161033-010223 | HST data is imaging (ACS) and spectroscopic (ACS) | V794 Sco | Plaut 1-53 | D from variable star group at Shternberg Astr Inst, Moscow State University, which holds Plaut's original charts; observations by 1990-09S (a reddened A-star) are of the wrong object | Ser | ROTSE3 J161304+01212 | probably in decline from outubrst on chart (1987.338) | Oph | NSV 7542 | ID uncertain | V341 Nor | | no candidate, field map shown | UMi1 | FBS 1614+711 | DAB white dwarf | V893 Sco | SVS 1772 | HST data is spectroscopic (STIS) | Sco | NGC 6093-CX5 | object in outburst on finding chart | Sco | NGC 6093-CX3 | type based on Chandra X-ray data only; HST data is imaging (WFPC2) | Sco | NGC 6093-CX4 | type based on Chandra X-ray data only; HST data is imaging (WFPC2) | Sco | NGC 6093-CX15 | type based on Chandra X-ray data only; HST data is imaging (WFPC2) | Sco | NGC 6093-CX2 | type based on Chandra X-ray data only; HST data is imaging (WFPC2) | T Sco | | in NGC 6093; possibly observed by Chandra (2003-80); HST
data is imaging (WFPC, WFPC2) and spectroscopic (STIS) | V382 Nor | Nova Normae 2005 | no candidate, field map shown | Her1 | PG 1617+150 | subdwarf B star | V589 Her | S 10296 | period 0.0905 (2002-130) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | U Sco | BD -17 4554 | HST data is spectroscopic (STIS) and imaging (WFPC2) | Sco | NGC 6121-CX1 | HST data is imaging (WFPC2) | Sco | NGC 6121-CX4 | object not visible on image; HST data is imaging (WFPC2) | Sco | NGC 6121-CX2 | object is likely a QSO; HST data is imaging (WFPC2) | PZ Nor | S 5733 | Mira variable | V844 Her | Antipin V43 | HST data is spectroscopic (STIS) | V699 Oph | HV 10577 | a spectrum of the new (DWS) candidate by 1999-09S is that of a
K star. However, astrometry in outburst (Sumner, B. 1999, VSNET chat
1810) shows the star marked is the correct identification; period
0.0685d (9999-01) is estimated from the superhump period using the
empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | TU Oph | HV 1068 | M-star spectrum, possible flare star | KQ Nor | S 5752 | K3 III star | UMi | NSV 7956 | photometric observations by Bennert, N. et. al. (1999, IBVS, 4779)
shows no evidence of flickering, and a spectrum by 2000-35 is that
of a late G star; = BD +86 252 | FL TrA | S 5770 | object in outburst on plate shown (1979.27); spectrum in 2003-15 is of
previous candidate (star to southwest of flagged object); period 0.05886
(2005-122) is estimated from the superhump period using the empirical
relation given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V592 Her | S 10376 | period 0.05592d (2002-107) is estimated from the superhump period
using the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | UMi | RX J1630.9+6950 | candidate on the edge of the circle is much brighter than the
quoted magnitude of the object | Dra | RX J1631.4+7354 | flagged object blue on POSS II plates | LR Nor | S 5796 | G2 II: star | V849 Her | PG 1633+115 | period 0.1409d (1999-89) is uncertain/unreliable | Oph | SDSSp J163722-001957 | north component of pair | V544 Her | S 9789 | period 0.069d (1998-46) is uncertain/unreliable | OY Ara | HD 149990 | object may be one of the fainter, nearby stars | Her3 | PG 1639+338 | subdwarf B star | Her | NGC 6205-23081 | ROSAT source; HST data is imaging (WFPC) | Her | NGC 6205-21429 | ROSAT source; object likely the bottom object in the circle;
HST data is imaging (WFPC2) | V610 Her | S 10311 | in the 1968-03 reference, this object and V611 Her are confused. The coordinates for V610 Her are those of variable S 10312, while the chart is that of S10311. For V611 Her, the coordinates are those of variable S 10311, while
the chart is that of S 10312 | AH Her | SVS 32 | HST data is spectroscopic (GHRS) | V611 Her | S 10312 | in outburst on POSSII plate (shown above) | AC Sco | HV 1095 | originally classified as a UG:, the flagged object is a G star; unless the object appears in outburst on the POSS I and II plates, and the UK-F plate shown here, it may be misidentified | V663 Ara | S 5893 | faint on 4 of 5 NOFS scans, bright on GSC 2.2 | RW UMi | SVS 1359 | object is bright on Guide Star Survey plate (1983.349); HST data is imaging (WFPC2) | AF Sco | HV 1108 | Mira variable | V840 Oph | HV 3522 | finding chart from C. Tappert | Dra | PG 1657+656 | subdwarf B-O star; catalog coordinates in 1986-06 are
40'' N of true position, listed here | V422 Ara | S 5989 | early-A V + K7 V binary | V1195 Oph | Plaut 2-71 | object blue on SERC plate | V1235 Oph | Plaut 2-111 | ID from variable star group at Shternberg Astr Inst,
Moscow State University, which holds Plaut's original charts | V598 Sco | HV 10836 | semiregular, late-type giant (K5 III) | V1326 Oph | Plaut 2-202 | ID from variable star group at Shternberg Astr.
Inst. Moscow State University, which holds Plaut's
original charts | Her | | near UGC 10700 | V992 Sco | | object blue on POSS | V455 Sco | HV 7869 | Z And variable | FQ Sco | HV 4389 | shown in outburst | V2051 Oph | | HST data is spectroscopic (FOS) | V2101 Oph | BV 1694 | semiregular, late-type giant (M5 II-III) | Dra | PG 1710+567 | subdwarf B star | V1548 Oph | Plaut 2-429 | minor planet (336) Lacadiera | V2214 Oph | | HST data is imaging (WFPC2) | V2400 Oph | Oph3;RX J1712.6-2414 | period 0.142d (1995-13) is uncertain/unreliable | Dra | SDSSp J171247+604603 | south component of pair | V1186 Sco | ASAS 171251-3056.6 | no candidate, field map shown; period 0.058d (2004-84) is uncertain/unreliable | V795 Her | PG 1711+336 | HST data is spectroscopic (FOS) | UMi | FBS 1719+834 | no candidate, field map shown; the object is detected
on a plate obtained on 26 June 1976, while the object is not seen
on the POSS I plate (11 August 1953) nor on a plate obtained
26 May 1974; in Henden's sequence
(ftp://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/fbs1735.dat) there
is a blue star (V=18.55, B-V=+0.17) at 17h 13m 13.69s, +83d 19' 08.7'',
which is under a diffraction spike on this chart | Her4 | PG 1712+493 | planetary nebula | V360 Her | | double exposure | V877 Ara | NSV 8383 | identification based on outburst observation; period 0.08106 (2003-11)
is estimated from the superhump period using the empirical relation
given by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Her | NGC 6341-8203 | ROSAT source; HST data is imaging (WFPC2, ACS, FOC, WFPC) | V825 Her | PG 1717+413 | HST data is spectroscopic (STIS) | V2573 Oph | Nova Oph 2003 | no candidate, field map shown | V2264 Oph | | no candidate, field map shown | V2527 Oph | Oph2/1E1719.5-1946 | finding chart from J. Thorstensen; object very blue | RY Ser | Ross 19 | the object was misidentified in DWS, the correct object (detected
during an outburst) is south of the DWS candidate | V2109 Oph | | north object of pair | V2295 Oph | | no candidate, field map shown | V902 Sco | He 3-1401 | identification uncertain | V906 Oph | | Circle indicates nominal position of the object; identification
in Duerbeck's atlas based on poor position and finding chart, and
should be discarded | V809 Her | S 10875 | quasar | V908 Oph | | no candidate, field map shown | V1187 Sco | Nova Sco 2004 No. 2 | no candidate, field map shown (although object in circle
is possible counterpart) | UMi | FBS 1735+825 | no candidate, field map shown; the object is not
seen on the POSS I plate (11 August 1953) | Dra | SDSSp J173008+624754 | HST data is spectroscopic (STIS) | MM Sco | HV 6553 | identification uncertain (2003-71); period 0.06024 (2004-32) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V1063 Oph | S 9807 | tentative identification | EK Aps | | RR Lyrae star | V2313 Oph | | no candidate, field map shown | Ara | NSV 9208 | cool DA white dwarf | V2540 Oph | | no candidate, field map shown | Oph | M14 Nova 1938 | HST data is both imaging (WFPC, FOC, WFPC2) and spectroscopy (FOS) | V2574 Oph | | no candidate, field map shown | BF Ara | HV 6576 | period 0.0845 (2003-45) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V794 Oph | | 1996-14S note that spectrum of the marked object is
featureless; 2003-07 find no evidence of rapid variability
in the marked object or any field stars; identification
uncertain | V728 Sco | N Ara 1862 | confirmation of candidate is necessary; the chart in
Duerbeck's atlas is inverted | Her | NSV 9445 | no candidate, field map shown; flagged star (17:39:30.44,
21:08:51.7) is a blue object possibly linked with a ROSAT source
(1RXS J173930.9+210847), which is also possibly slightly variable,
and could be a candidate for the nova (Skiff, B. and Kinnunen, T.
2005, private communication) | V733 Sco | | Tentative identification | RT Ser | He 3-1452 | Z And variable | Ara | NGC 6397-U28 | type based on Chandra X-ray data only | Ara | NGC 6397-CV1 | HST data is imaging (WFPC2) and spectroscopic (FOS) | Ara | NGC 6397-CV4 | HST data is spectroscopic (FOS) | Ara | NGC 6397-DP1 | HST data is imaging (FOC, WFPC2) | Ara | NGC 6397-DP3 | HST data is imaging (FOC, WFPC2, STIS) | Ara | NGC 6397-DP2 | HST data is imaging (FOC, WFPC2) | Ara | NGC 6397-CV3 | HST data is imaging (WFPC2, STIS) and spectroscopic (FOS) | Ara | NGC 6397-DP4 | HST data is imaging (FOC, WFPC2) | Ara | NGC 6397-U13 | type based on Chandra X-ray data only | Ara | NGC 6397-U11 | type based on Chandra X-ray data only | Ara | NGC 6397-U10 | type based on Chandra X-ray data and variability | V810 Oph | HV 11017 | slow irregular variable | AE Ara | HV 5491 | Symbiotic star | V1012 Oph | SVS 1308 | no candidate, field map shown | V660 Her | SVS 2120 | chart in D+S is of the wrong field; no revised chart provided in DWS | V2024 Oph | | Circle indicates nominal position of the object, while the flagged object is indicated in the Duerbeck atlas | V721 Sco | He 3-1458 | object is at the center of the circle, and is the corner of an
inverted 'L' | V553 Oph | | a faint star is visible in Duerbeck's atlas at the
indicated position; ID is uncertain | V2290 Oph | | no candidate, field map shown | V2110 Oph | AS 239 | 2MASS source (K=7.62); object likely a Z And variable | V916 Sco | | Z And variable; 2MASS source (K=12.12) | KP Sco | HV 4716 | nova is probably a star of 21m, NE of a bright
visual double star; tentative identification | V1188 Sco | Nova Sco 2005 | no candidate, field map shown | V734 Sco | IRAS 17416-3537 | in outburst; 2MASS source (K=6.89); likely a Mira variable | Sgr | K5-15 | object visible on 1980 May 19, May 23, and June 17 | Sgr | CXOGC J174532-290552 | no candidate, field map shown; type based on Chandra X-ray data only | V719 Sco | He 3-1473 | object not visible | Sco | NSV 9663 | candidate revised by Duerbeck; coordinates
given are for this candidate | V4744 Sgr | N Sgr 2002 No. 4 | no candidate, field map shown | Sgr | Terzan 5 - W7 | type based on Chandra X-ray data only | Sgr | Terzan 5 - W10 | type based on Chandra X-ray data only | Sgr | Terzan 5 - W9 | type based on Chandra X-ray data only | Sgr | Terzan 5 - W6 | type based on Chandra X-ray data only | Sgr | Terzan 5 - W5 | type based on Chandra X-ray data only | Her | | near UGC 10990 | V707 Sco | HV 3618 | confirmation of candidate is necessary; not
visible on finding chart | V722 Sco | | no candidate, field map shown | Sgr | NGC 6440-CX13 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX8 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX23 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX15 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX24 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX14 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX18 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX17 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX19 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX16 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX6 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX10 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX11 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX20 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX9 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX12 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX21 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX22 | type based on Chandra X-ray data only | Sgr | NGC 6440-CX4 | type based on Chandra X-ray data only | V1274 Sgr | SN s1954a | no candidate, field map shown; although classified as a possible
supernova, there is no host galaxy visible on the POSS, so if real, the
object may be a nova | V378 Ser | | no candidate, field map shown | V723 Sco | | circle designates nominal outburst position,
while flagged object is Duerbeck candidate | RS Oph | BD -6 4661 | HST data is imaging (WFPC2) | V380 Oph | 159.1929 | HST data is spectroscopic (STIS) | V759 Sgr | HV 10285 | originally classified as an Irregular variable (Swope, H.H. 1940, Harvard Ann., 109, No. 1); bright in the 2MASS survey (K = 9.72 at 17 50 19.708, -27 25 02.46). Swope gives a note saying, ''there is one observation at 13.6 on J.D. 2424402, one at 14.4 on J.D. 2413083; otherwise the star varies between 15.0 and 16.0.'' In light of its IR brightness, this is probably a long-period or irregular red giant, possibly a symbiotic star, but very unlikely to be a CV | V1172 Sgr | | 2MASS source (K = 11.04) | Sgr | Bul_sc5_2859 | outburst not observed | Her6 | NSV 9787 | G star | V977 Sco | | object in outburst on 1989.67 plate, which confirms
identification; HST data is imaging (WFPC2) | V382 Sco | HV 7006 | no candidate, field map shown | V720 Sco | He 3-1503 | no candidate, field map shown | KW Sgr | HDE 316496 | semiregular variable | V4334 Sgr | Sakurai's var. | final helium flash object | V2415 Sgr | | no candidate, field map shown | V744 Sco | | tentative identification | Sco | NSV 9808 | no candidate, field map shown | V711 Sco | HV 3061 | unambiguous identification not possible | Sco | NSV 24027 | does not exist | V1141 Sco | | likely identical to Bul_sc4_1367 (2003-09) | V4643 Sgr | | no candidate, field map shown | Sgr | NSV 9828 | no candidate, field map shown; there is a bright, extremely
red star (not in the GSC) a few arcseconds away (2MASSI
J1754428-284136 (K=7.86 at 17h 54m 42.836s, -28d 41' 36.21''). If
this is the counterpart, then NSV 9828 is likely a long-period
variable | Sgr | m403.47614.3183 | no candidate, field map shown | V745 Sco | | a second outburst was recorded in 1989.58; in decline on POSS II plate
(epoch 1989.67) shown above; 2MASS source (K=8.23); HST data is imaging (WFPC2) | V1142 Sco | | object is northwest object of pair | MU Ser | | no candidate, field map shown | V732 Sgr | HDE 316633 | identification uncertain | V960 Sco | | HST data is imaging (WFPC2) | V1178 Sco | HadV92 | tentative identification | Sgr | NSV 24048 | symbiotic star | V3889 Sgr | | object not visible on chart | V2435 Sgr | | long-period variable | Sgr | NSV 9923 | possible ROSAT ID is 1RXS-F J175914.5-423529 period 0.0796d (2003-82)
is estimated from the superhump period using the empirical relation
given by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V4338 Sgr | | no candidate, field map shown; there is a bright 2MASS source
(K = 12.66, at 17h 59m 18.252s, -29d 09' 52.61'') near the outburst
position of this nova | V2446 Sgr | | Mira variable | V4683 Sgr | NSV 24062 | Mira or symbiotic star | V4135 Sgr | | in decline on GSS plate 067O; HST data is imaging (WFPC2) | V2468 Sgr | | bright on 2MASS - LPV? | V4741 Sgr | N Sgr 2002 No. 1 | no candidate, field map shown | Sgr | m113.18676.5195 | no candidate, field map shown | V787 Sgr | HDE 316917 | no candidate, field map shown | V999 Sgr | HD 163982 | 1996-14S note the spectrum is featureless | V394 CrA | N Sco 1949 | nova is the southern object in a triple; a second outburst was recorded in 1987.59;
HST data is imaging (WFPC2); period 0.7577d (1990-41) is uncertain/unreliable | FL Sgr | HV 4003 | no candidate, field map shown; an object is identified
on the SERC-J plate in Duerbeck's atlas | V2301 Oph | Oph1; 1H 1752+081 | HST data is spectroscopic (FOS) | V1944 Sgr | SVS 1397 | our coordinates are 0.3s east and 4'' north of Duerbeck | V2493 Sgr | | Mira variable | V551 Sgr | HV 7095 | from outburst image; period 0.0659d (2003-105) is estimated from the
superhump period using the empirical relation given by Stolz, B. and
Schoembs, R. 1984, Astron. Astrophys., 132, 187 | DZ Ser | | no candidate, field map shown | KY Sgr | HV 4480 | tentative identification | V1174 Sgr | | no candidate, field map shown | V2561 Oph | SN 1999bs | no candidate, field map shown | Sgr | MACHO pec var | in outburst on POSS II plate (1991.68225) | V884 Her | Her5; WGA 1802+1804 | object is the southwest star in double | V4742 Sgr | N Sgr 2002 No. 2 | no candidate, field map shown; period 0.225d (2004-36) is
uncertain/unreliable | Sgr | m119.19707.2379 | no candidate, field map shown | V4027 Sgr | | no candidate, field map shown | Sgr | m114.19842.2283 | no candidate, field map shown | Sgr | m104.19991.1951 | no candidate, field map shown | V5099 Sgr | MACHO SU UMa var | object is visible on chart in 1999-91 | V2104 Oph | | ID uncertain | V1431 Sgr | | revised identification based on the new chart reference;
star is the middle object in chain of three | AT Sgr | HV 1149 | object not visible | V4579 Sgr | NSV 24159 | the object is still partially in outburst on an HST Guide Star survey plate obtained on 1987.59, while is in quiescence on a second epoch SERC-ER plate obtained on 1992.42. | EX Dra | Dra5; HS 1804+6753 | HST data is spectroscopic (FOS) | V1502 Sgr | | semiregular variable | Sgr | NSV 10158 | no candidate, field map shown;
position is 17'' north of Duerbeck's position (from X1953-02) | V1572 Sgr | | no candidate, field map shown | Sgr | m105.21291.7441 | no candidate, field map shown | V1012 Sgr | HV 3531 | nova is blend of 2 stars | V1014 Sgr | HV 3312 | no candidate, field map shown | V737 Sgr | V908 Sgr | ID is unresolved clump | V908 Sgr | V737 Sgr | duplicate GCVS designation, retired in favor of V737 Sgr | Sgr | CPD -22 6701 | spurious nova, the results of omission of this star on an
AAVSO chart | DQ Her | 452.1934 | HST data is imaging (WFPC2), spectroscopy (FOS), and photometry (HSP) | Sgr | OGLE MM3 I 58214 | single outburst observed; no candidate, field map shown | V927 Sgr | | no candidate, field map shown | V4121 Sgr | | object appears to be in outburst on SERC-J plate shown in the
Duerbeck atlas; HST data is imaging (WFPC2) | Sgr | MOA-ngb10-1-211 | no candidate, field map shown | KY Ara | HV 7987 | no candidate, field map shown | V631 Her | S 10422 | no candidate, field map shown | Sgr | | M star, long period variable | V1015 Sgr | HV 3529 | no candidate, field map shown | V1148 Sgr | | tentative identification | Sgr | m115.22695.3361 | no candidate, field map shown | V4157 Sgr | | no candidate, field map shown | PU Her | S 4248 | a spectrum of the candidate object in DS93 is that of
a G star (1999-09S). 2000-31 has identified a new candidate based on an outburst
observation. | Sgr | Bul_sc16_2143 | possibly 1RXS J180957.5-262158 | V5113 Sgr | N Sgr 2003 No. 2 | no candidate, field map shown | Sgr | MOA-ngb11-2-1146 | no candidate, field map shown | V2506 Sgr | AS 282 | Z And variable | V4740 Sgr | N Sgr 2002 No. 3 | no candidate, field map shown | Sgr | MOA-ngb11-2-1011 | no candidate, field map shown | Sgr | m125.23850.4190 | no candidate, field map shown | IX Dra | Dra6; KUV 18126+6704 | spectrum in Wegner, G. and McMahan, R.K. (1988, AJ, 96, 1993) could
be in outburst; HST data is spectroscopic (STIS) | V4327 Sgr | | no candidate, field map shown | V1830 Sgr | | in outburst on SERC V plate shown | V4160 Sgr | | no candidate, field map shown | V1175 Sgr | | no candidate, field map shown;
there is an object at RA(2000) = 18h 14m 20.8s, Dec(2000) = -31
degrees 06' 36'' which is much fainter on the Guide Star plate (a V
image) than Duerbeck's (a J image) published chart. This object
(flagged) is either very blue or variable, and is a candidate for the
nova | V533 Her | | HST data is imaging (WFPC2) | V3909 Sgr | | M3 III star (Mira variable?) | V3914 Sgr | | Mira variable | V1583 Sgr | HV 12320 | no candidate, field map shown | V2323 Sgr | | semi-regular or Mira variable | V4074 Sgr | AS 295B | nova is in a visual triple;
object is 3'' south of the brighter star ADS 295 | Sgr | m306.36059.752 | no candidate, field map shown | V370 CrA | HV 11880 | Mira variable | AM Her | 3A 1815+498 | HST data is photometric (HSP) and spectroscopic (FOS, GHRS, STIS) | V2839 Sgr | Plaut 3-281 | identification based on low-level variability | V2329 Sgr | NSV 8428 | Mira variable | Sgr | MOA-ngb13-2-1170 | no candidate, field map shown | V5115 Sgr | Nova Sagittarii 2005 | no candidate, field map shown | FM Sgr | HV 3994 | no candidate, field map shown | DV Dra | SVS 2704 | position from outburst observation; no candidate visible; period 0.06
(2005-123)is estimated from the superhump period using the empirical
relation given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V5116 Sgr | Nova Sgr 2005 No. 2 | no candidate, field map shown | V1149 Sgr | | tentative identification; object not visible | Sgr | m311.37730.4143 | no candidate, field map shown | V1150 Sgr | AS 300? | no candidate, field map shown | V928 Sgr | | no candidate, field map shown;
position is the midpoint between Duerbeck's candidates 1 and 2 | GM Sgr | HV 4048 | long period variable (Luyten's variable) | V4641 Sgr | SAX J1819.3-2525 | flaring x-ray transient (Goranskij's variable) | V5114 Sgr | Nova Sgr 2004 | no candidate, field map shown | V726 Sgr | HDE 315532 | no candidate, field map shown | V4065 Sgr | | object possibly in decline from outburst on UK-F plate shown | V441 Sgr | HDE 315574 | no candidate, field map shown | Sgr | m153.28398.2677 | no candidate, field map shown | GR Sgr | HV 4012 | nova is brightest component of blend of 3 stars | Sct | Lanning 17 | single outburst observed | V4169 Sgr | | no candidate, field map shown | Sgr | NGC 6624 CV2 | HST data is imaging (WFPC2) | V4171 Sgr | | no candidate, field map shown; HST data is imaging (WFPC2) | Sgr | NGC 6624 CV1 | the object may not be real (1999-17S);
HST data is imaging (WFPC2) | IR Lyr | S 4267 | strong Balmer absorption, recent outburst unlike a CV | WW Tel | HV 9884 | chart reference not unambiguous, field map shown; the flagged object
in D+S is a G0 V star | Sgr | NGC 6626 V7 | Mira variable | V655 CrA | | object is a member of a close triplet | V4739 Sgr | N Sgr 2001 No. 2 | no candidate, field map shown | V1151 Sgr | | object is north object of close pair | V4019 Sgr | | A7e star | V909 Sgr | | no candidate, field map shown; period 0.140d (1997-58) is
uncertain/unreliable | V3941 Sgr | | lose companion to the southwest; 2MASS source (K = 11.25) | DP Pav | S 7111 | A2-3 V star | BS Sgr | INN 4a | object is bright component of close visual pair; 1996-14S note the colors as a reddened K star?; 2MASS source (K = 12.10) | V1988 Sgr | IRC -30385 | possible Z And variable | HS Sgr | HV 4011 | 1996-14S note the colors of Duerbeck's candidate is that of a K3-6 star? | V391 Sct | M 64 | there is a red companion 4'' to the southwest | Sct | NSV 10848 | no candidate, field map shown | LQ Sgr | HV 4475 | Symbiotic star | V366 Sct | | no candidate, field map shown | V3462 Sgr | Plaut 3-1047/INN 114 | no candidate, field map shown | V4362 Sgr | | no candidate, field map shown | V3890 Sgr | GS 1826-24 | a second outburst was recorded in 1990.32; HST data is imaging (WFPC2) | FH Ser | | HST data is imaging (WFPC2) | Sgr2 | NGC 6637 CV | - position is computed by offset from star II-35 (cf 1986-12S)); HST
data is imaging (WFPC2) | V2359 Sgr | NGC 6637-V7 | measurement is of the center of a clump, the object is
possibly the east object in the clump; object observed in 2003-15S is
a G-type star | V2572 Sgr | BV 1262 | nova is a blend of 3 stars | V1017 Sgr | HV 3519 | 1987-08X lists the object as a possible symbiotic star or recurrent nova | V476 Sct | Nova Scuti 2005 | no candidate, field map shown | Sct | AX J183220-0840 | no candidate, field map shown; period 0.017929d
(2000-88) is uncertain/unreliable | V3876 Sgr | IRC -20494 | Mira variable | Sgr | m173.33002.479 | no candidate, field map shown | V1905 Sgr | | our coordinates are 0.1 east and 5'' south of Duerbeck; 1996-14S note the colors of Duerbeck's candidate is that of a K3-5 star | AG Ser | Ross 48 | extremely red object, Mira variable or flare star | YY Tel | HV 9962 | classification in doubt (no emission lines in the spectrum
(1996-01S) nor flickering (2001-79)) | V463 Sct | HadV46 | object incipently visible on DSS image | V939 Sgr | INN 25 | Mira variable | V4077 Sgr | | HST data is imaging (WFPC2); period 0.16d (1997-58) is uncertain/unreliable | V941 Sgr | INN 27 | Mira variable | V1310 Sgr | | revised identification based on the original chart reference in 1987-08X; possible Mira variable | Sgr | NGC 6656-35 | UV candidate in XMM-Newton error circle | V662 CrA | Plaut 3-1235 | ID from variable star group at Shternberg Astr Inst,
Moscow State University, which holds Plaut's original charts | Sgr | NGC 6656-78 | UV candidate in XMM-Newton error circle | Sgr | NGC 6652 C | could also be a quiescent low-mass x-ray binary; HST data is imaging (WFPC2) | V3645 Sgr | SVS 1728 | most likely candidate flagged | Sgr | m145.34015.1280 | no candidate, field map shown | Her | | Near UGC 11289 | Sgr | NGC 6656 CV2 | object not visible, field map shown; period 0.0852 (2005-90)
is estimated from the superhump period using the empirical relation
given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132,
187 | Sgr | NGC 6656-44 | UV candidate in XMM-Newton error circle | Sgr | NGC 6656-32 | UV candidate in XMM-Newton error circle | Sgr | NGC 6656 CV1 | HST data is imaging (WFPC2) | Sgr | NGC 6656-39 | UV candidate in XMM-Newton error circle; 2 possible candiates; coordinates
are for the southern object; northern object has end figures 25.5, 13.7, and
U=19.1 | Sgr | NGC 6656-23 | UV candidate in XMM-Newton error circle | Sgr | NGC 6656-21 | UV candidate in XMM-Newton error circle | V2012 Sgr | | slow irregular variable | V4021 Sgr | | chart in Duerbeck atlas is incorrect due to labelling problem.
Spectrum in 1996-14S (K0-3 star) is of old candidate | V651 Oph | 271.1936 | possible ROSAT ID is 1RXS-F J1837+0922 | V477 Sct | Nova Sct 2005 No. 2 | no candidate, field map shown | Her | OT_J183926+260410 | northwest component of double (separation 0.99'') with the
bright star in the circle (2MASS 18392629+2604087); also known as
1RXS J183927.1+260409 | V4745 Sgr | N Sgr 2003 | no candidate, field map shown | Oct | NSV 10934 | ROSAT ID is 1RXS J184050.3-834305; period 0.0726d (2004-32) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V949 Sgr | INN 46 | Mira or semiregular variable | V3774 Sgr | Plaut 3-1453 | object is bright on the Palomar Observatory Sky Survey O print, not as bright on the Palomar Observatory Sky Survey E print, SRC J film, or Guide Star Survey V plate (1987.633) | V693 CrA | | no candidate, field map shown; HST data is imaging (WFPC2) | Pav | NSV 11181/LTT 7406 | DC white dwarf | V2383 Sgr | | Mira variable | V1709 Sgr | HV 12404 | semiregular variable | V427 Sct | CSV 7917 | Mira variable? | BD Pav | HV 10031 | HST data is spectroscopic (STIS) | V492 Lyr | LHS 3406 | dMe star | V827 Her | | HST data is imaging (WFPC2) | V2032 Sgr | | Mira variable | AK Tel | HV 10036 | very red colors, small-amplitude variations (1.2 mag) | AY Lyr | 330.1928 | period 0.0737d (1988-29) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Aql | NSV 11280 | no candidate, field map shown | V344 Lyr | S 9329 | in outburst on plate; period 0.0876d (1998-46) is estimated from the
superhump period using the empirical relation given by Stolz, B. and
Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V347 Pav | RE J1844-741 | HST data is spectroscopic (STIS) | Aql2 | NSV 11297 | a spectrum of the candidate object is that of a late-K star (1999-09S), so the object is likely mis-identified | V2038 Sgr | | Mira variable | GL Sct | | Duerbeck's quoted position is not consistent with his chart.
The object is located 0.64s east and 6.4'' south of Duerbeck's
position | V838 Her | | the object is 1.4'' west and 1.0'' north of the star at 18h 46m 31.6s and +12 degrees 14' 00.8''; HST data is imaging (WFPC2) | V444 Sct | | no candidate, field map shown | V522 Sgr | | Duerbeck's candidate (due north) has the colors of a G2-G5
star (1996-14S) | V603 Aql | HD 174107 | HST data is spectroscopic (FOS, GHRS) | V475 Sct | N Sct 2003 | no candidate, field map shown | V443 Sct | | a measurement of a possible prenova (0.02s west and 0.3'' north of the
position presented here) can be found in Anupama, G.C., Duerbeck,
H.W., Prabhu, T.P. and Jain, S.K. (1992, Astron. Astrophys., 263, 87);
no candidate, field map shown | V4332 Sgr | | M-giant star | CI Aql | 23.1925 | a quiescent spectrum of the object shows He II 4686 and N III/C II 4650 emission (Greiner, J., Alcala, J.M., and Wenzel, W. 1996, IBVS, 4338); a second outburst was recorded in 2000.33 | Sct | NGC 6712 V9 | 1988-11 reports a B-V color of +1.23 (wrong ID?), while
1966-06 report that the object is extremely blue; flagged object
is very blue in the USNO-A2.0 catalog | Sct | NGC 6712 10261 | HST data is imaging (WFPC2) | Lyr | NSV 11494 | no candidate, field map shown | V4368 Sgr | Pec Var in Sgr | symbiotic star | V1223 Sgr | 3A 1851-312 | HST data is astrometric (FGS) | Sgr | NGC 6715-CX4 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX7 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX6 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX1 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX2 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX5 | type based on Chandra X-ray data only | Sgr | NGC 6715-CX3 | type based on Chandra X-ray data only | EL Aql | 60.1927 | chart in Duerbeck atlas is incorrect due to labelling problem | EU Sct | | 2003-07 note that the marked object is red, and shows no evidence
of rapid variability. A 19.1 mag companion 4'' south may show
variability | V800 Aql | S 4376 | Cepheid | Sct | NSV 11561 | K4 V star | V446 Her | | nova has 3 close companions; HST data is imaging (WFPC2) and
spectroscopic (STIS) | FS Sct | | 1996-14S note the spectrum of Duerbeck's candidate is featureless | V358 Lyr | S 9649 | no candidate, field map shown | V447 Lyr | GR 247 | in outburst on the Palomar Observatory Sky Survey (1951.672) | V4743 Sgr | N Sgr 2002 No. 3 | no candidate, field map shown | V1059 Sgr | HD 176654 | nova is brightest of a blend of 3 stars | Aql | NSV 24663 | observed to flare once, at 11 September 1960; published chart
not useful; no candidate, field map shown | Aql | | in decline on POSS II red image shown (1987.410) | Aql | NSV 24667 | observed to flare once, at 18 July 1964; published chart not useful;
no candidate; field map shown | CM Aql | | Symbiotic star | QV Vul | | HST data is imaging (WFPC2, NICMOS) | V1663 Aql | ASAS 190512+0514.2 | object could be a symbiotic nova | V1425 Aql | | faint blue star on POSS I plate (1998-77); HST data is
imaging (WFPC2) | Aql | NSV 24685 | observed to flare once, at 8 September 1948; published
chart not useful; no candidate, field map shown | MV Lyr | Mac +43 1 | HST data is spectroscopic (STIS) | V1548 Aql | TAV J1907+117 | no candidate, field map shown | CG Dra | S 9370 | period 0.1893d (1997-41) is uncertain/unreliable | V1493 Aql | | candidate not visible | V841 Aql | | object in decline on POSS I; a spectrum of the Duerbeck
candidate by 1999-09S reveals a late-type star, consistent with the
report of 1996-14S | V1089 Sgr | vG 136 | north object of blended pair shown; observations in outburst
reveal that the object marked in previous editions is incorrect. The
object observed by 1996-01S (K3-5 II star)is the wrong target | V419 Lyr | SVS 1584 | a spectrum by 1999-09S shows only Mgb absorption in a low
signal-to-noise spectrum; period 0.0864d (2003-82) is estimated from
the superhump period using the empirical relation given by Stolz,
B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | Pav | NGC 6752-CX3 | HST data is imaging (WFPC2) | Pav | NGC 6752-CX13 | HST data is imaging (WFPC2) | Pav | NGC 6752-CX6 | HST data is imaging (WFPC2) | Pav | NGC 6752-CX1 | HST data is imaging (WFPC2) | Pav | NGC 6752-CX5 | may be BY Dra star; HST data is imaging (WFPC2) | Pav | NGC 6752-CV2 | HST data is imaging (WFPC2) and spectroscopy (FOS);
period 0.154 (1996-12) is uncertain/unreliable | Pav | NGC 6752-CV1 | HST data is imaging (WFPC2) and spectroscopy (FOS);
period 0.213 (1996-12) is uncertain/unreliable | Pav | NGC 6752-CX11 | may be a galaxy; object not visible, + marks approximate location;
HST data is imaging (WFPC2) | Pav | NGC 6752-CX10 | HST data is imaging (WFPC2) | Pav | NGC 6752-CX15 | may be a galaxy; HST data is imaging (WFPC2) | Pav | NGC 6752-CX2 | HST data is imaging (WFPC2) | V363 Sgr | | no candidate, field map shown | V369 Lyr | SVS 1512 | no candidate, field map shown | V1419 Aql | | HST data is imaging (WFPC2) | V352 Aql | PK 37-3 3 | planetary nebula nucleus (PK 37-3.3 = K3-25) | V585 Lyr | TK 4 | there is a companion to the northwest; object possibly in outburst on
image; period 0.0593d (2003-90) is estimated from the superhump period
using the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V407 Vul | RX J1914+2456 | a blend of 3 stars; object could also be a unipolar-inductor
(2002-25) | Aql3 | NSV 11855 | a plate flaw | V344 Pav | | in outburst on plate shown (1995.65); period 0.077d (2004-72) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | FO Aql | 3.1905 | may be blended with a red star 0.525 arcsec to SSW at minimum (Sumner, B. 1999, ftp://ftp.nofs.navy.mil/pub/outgoing /aah/sequence/sumner/foaql.seq) | V587 Lyr | TK 5 | period 0.06 (2005-124) is estimated from the superhump period using the
empirical relation given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V605 Aql | 7.1920 | final helium flash object | V1336 Aql | SVS 2270 | Mira variable | V528 Aql | | north object of pair | V606 Aql | BD -0 3708a | object blue on POSS II plates | V523 Lyr | NGC 6791 B7 | red dwarf plus hot subdwarf | V1113 Cyg | S 9382 | period 0.0766d (1998-46) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V1494 Aql | | east object of close pair | BF Cyg | He 3-1747 | Z And type | V1229 Aql | | nova is the southern object in a triple (Della Valle, M. and Duerbeck,
H.W. 1993, Astron. Astrophys., 275, 239); HST data is imaging (WFPC2) | Aql | NSV 12006 | no candidate, field map shown | PW Vul | | object is the middle object in a chain of three; HST
data is imaging (WFPC2); period 0.2137d (1998-46) is uncertain/unreliable | DH Aql | HV 3899 | period 0.07738d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V368 Aql | 668.1936 | north object of pair | V2176 Cyg | BAO 01 | period 0.0553d (1997-43) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | Aql | NSV 24785 | in error box of GRBS 790311 | Tel | CTCV J1928-5001 | object is northeast star of close pair | V868 Cyg | VV 137 | very crowded field | NQ Vul | | HST data is imaging (WFPC2) | V1505 Cyg | SVS 1532 | south star of merged double | HN Cyg | 294.1929 | Mira variable | KX Aql | HV 5428 | finding chart from J. Thorstensen | V795 Cyg | VV 63 | western member of pair; finding chart from J. Thorstensen;
spectrum shows broad Balmer and He I 5876 emission | V2289 Cyg | 1H 1933+510; Cyg2 | period 0.138d (1992-40) is uncertain/unreliable | V607 Aql | 31.1905/IRC 00445 | Mira variable | BZ Aql | HV 3799 | Mira variable | V991 Aql | S 8125 | near NGC 4013 | V1141 Aql | 36.1905 | period 0.06202d (2004-95) is uncertain/unreliable | Cyg3 | NSV 12245 | both objects in double are late-type stars | QS Tel | RE 1938-461 | HST data is spectroscopic (FOS) | EM Cyg | 185.1928 | HST data is astrometric (FGS) and spectroscopic (STIS) | V1289 Aql | 67.1903 | originally classified as a NL:, the flagged object is an early-mid G
star, indicating a possible misidentification; the object due south appears to
be slightly blue on the POSSII plate | SS Sge | SVS 81 | Z And variable | HS Sge | | ID is a blend | Cyg | NSV 24843 | a plate defect | Sgr | NGC 6809 CV1 | finding chart from 2005-21 | V1432 Aql | Aql1; RX J1940-1025 | HST data is spectroscopic (FOS) | V890 Aql | | does not exist | Sgr1 | NSV 12329 | no candidate, field map shown; Suspected nova, based on
Fleming's (1896, Harvard Circ. No. 9) classification of the K0 star
CoD -40 13448 = HD 186058 at the center of the error circle as a B5p
star with H-beta emission | V1285 Cyg | VV 255 | semiregular variable | LU Vul | | no candidate, field map shown | CK Vul | BD +26 3670a | no candidate, field map shown; may be final helium flash
object instead of classical nova | V3885 Sgr | CD -42 14462 | HST data is spectroscopic (FOS, STIS) | V1449 Cyg | GR 217 | new identification based on blue color on POSSII
plate, east object of pair | CI Cyg | HV 3625 | Z And type | V1050 Aql | S 8194 | Mira variable | V1452 Cyg | GR 220 | very crowded; 2MASS source (K=15.26) | DO Vul | 25.1928 | finding chart from J. Thorstensen; period
0.064 (2005-123) is estimated from the superhump period using the empirical
relation given by Stoltz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V500 Aql | S 3542 | object in decline on POSS I | V465 Cyg | VV 67 | candidate not visible, field map shown | V405 Vul | S 10943 | period 0.112d (1998-45) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | PQ Aql | HV 5482 | in outburst on POSS; ID could be object to northwest | CK Cyg | SVS 26 | no candidate, field map shown; the coordinates in 1923-01 do not match
the finding chart | V1454 Cyg | GR 221 | in outburst on POSS II J plate shown; the spectrum in 1999-09S is of the
wrong object | EY Cyg | 200.1928 | HST data is spectroscopic (STIS) | V1819 Cyg | | HST data is imaging (WFPC2) | Sgr3 | NSV 12560/LTT 7873 | DA white dwarf | V476 Cyg | 26.1920 | HST data is imaging (WFPC2) | AW Sge | 151.1905 | period 0.0724d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187; spectrum is that of a G-type star,
which implies that either the wrong candidate was observed, or the
flagged object is not the correct identification | Vul | Var. Star near M27 | positionally near the planetary nebula M27; no candidate,
field map shown; period 0.0580 (2005-123) is estimated from the
superhump period using the empirical relation given by Stoltz, B. and
Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V337 Cyg | 101.1928 | object is one of 2 candidates in circle | V1028 Cyg | S 7854 | period 0.06041d (1998-46) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | V823 Cyg | VV 66 | identification based on outburst observation; object
is in outburst on POSS II-J plate (1989.49) shown above | V362 Vul | E2000+223 | low redshift AGN | RZ Sge | 157.1905 | finding chart from J. Thorstensen; HST data is
spectroscopic (STIS) | RR Tel | HV 3181 | Z And variable | V550 Cyg | S 3847 | ID from outburst astrometry (VSNET alert 5210); period 0.0672d
(2003-82) is estimated from the superhump period using the empirical
relation given by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys.,
132, 187; finding chart from J. Thorstensen | Cyg4 | NSV 12778 | late-G or early-K star | QQ Vul | 1E 2003+225 | HST data is photometric (HSP) | Sgr | CTCV J2005-2934 | period 0.06289d (2004-58) is uncertain/unreliable | V2274 Cyg | N Cyg 2001 No.1 | no candidate, field map shown; period 0.3d (2001-115) is uncertain/unreliable | WZ Sge | HV 3518 | HST data is spectroscopic (FOS, GHRS, STIS) and astrometric (FGS) | GS Pav | S 7040 | HST data is spectroscopic (STIS) | AX Cap | Cap4; 2006-1725 | in outburst on POSS II-F plate shown; period 0.110d (2004-82) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | V2361 Cyg | Nova Cygni 2005 | no candidate, field map shown | V1316 Cyg | GR 141 | revised identification from D+S | Cyg | MGHT 4 | object in outburst on POSSII-J plate (06/30/89) | V1377 Cyg | GR 166 | no candidate, field map shown; flagged object
is bluest in the area | V794 Aql | 499.1936 | shown in faint state; period 0.1533d (1998-86) is
uncertain/unreliable; HST data is spectroscopic (STIS) | V Sge | He 3-1879 | HST data is spectroscopic (GHRS) | Del | NSV 13022 | equinox of the coordinate
systems in the discovery notice (1953-01) is ambiguous.
B1953.3 (the epoch of discovery) is assumed; no candidate,
field map shown | PU Vul | Kuwano's NL | Z And variable | Cap1 | StHA 176 | this star is red (B-V=1.28) in Henden's photometry (ftp.nofs.navy.mil/pub/outgoing/aah/sequence/cap1.dat) | V1776 Cyg | Lanning 90 | HST data is spectroscopic (STIS) | V404 Cyg | 100.1938 | x-ray binary; a second outburst was recorded in 1989 | CM Del | 147.1930 | HST data is spectroscopic (GHRS) | EZ Del | S 4505 | the object identified in the first edition is incorrect. The correct identification (1997-28 and Liu, W., Hu, J.Y., Zhu, X.H., and Li, Z.Y. 1999, Ap.J. Supp., 122, 243) is the star to the southeast of the original ID (the middle
star in the triple). | V374 Vul | LD 171 | late M star, semi-regular variable | V2276 Sgr | S 6738 | spectrum of the flagged object is that of a hot white dwarf;
identification may be in error | QU Vul | | HST data is imaging (WFPC2, NICMOS) | IO Del | S 10693 | no candidate, field map shown | V503 Cyg | S 4524 | HST data is spectroscopic (STIS) | V1974 Cyg | | HST data is imaging (WFPC, WFPC2,
NICMOS, FOC), spectroscopy (FOS, GHRS), and photometry (HSP) | Cyg1 | NSV 25181 | also known as KPD 2032+5037 | AE Aqr | 342.1931 | HST data is both imaging (WFPC2) and spectroscopy (FOS) | TY Vul | 38.1923 | object barely visible to east of brighter star; period 0.0777d
(2003-102) is estimated from the superhump period using the empirical
relation by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132,
187 | HR Del | | HST data is imaging (WFPC2, FOC) | V1697 Cyg | SVS 2272 | no candidate, field map shown; object in the center of the
circle is a 2MASS source (K=14.47) | V751 Cyg | SVS 1202 | HST data is spectroscopic (STIS) | V1330 Cyg | | 1996-14S note the color of Duerbeck's candidate is that of a K1-4 star | UY Vul | 150.1904 | M-star spectrum | UZ Vul | 151.1904 | M-star spectrum | V450 Cyg | 85.1942 | object in decline on POSS I | V407 Cyg | AS 453 | Z And variable | Aqr | SDSS J210241-004408 | likely a white dwarf | EV Aqr | SVS 615 | object is not visible; position marked is that indicated by
1991-15, but differs from the bright star to the NW (GSC 0526-01562)
marked by 1971-05, whom they cite as their nominal reference | HU Aqr | RX J2107.9-0518 | HST data is spectroscopic (FOS, GHRS) | V1062 Cyg | S 9110 | there is a blue object to the northeast (end figures
12.3s, 31.0''), which could be the dwarf novae (which would
imply that the stated amplitude is in error) | V1065 Cyg | S 9113 | north object of pair | V1500 Cyg | RX J2111.6+4809 | object bright on 1990.6 POSS II plate; HST data is both imaging (WFPC2) and spectroscopy (FOS) | VY Aqr | Ross 88 | HST data is spectroscopic (STIS) | V364 Peg | BAO 02 | period 0.085d (2004-87) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | EF Peg | 143.1935 | object is 5'' away at 305 degrees from the star at RA(2000) = 21h 15m
04.45s, Dec(2000) = 14 degrees 03' 47.5''; HST data is spectroscopic
(STIS); period 0.0837d (2002-45) is estimated from the superhump
period using the empirical relation given by Stolz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | CD Ind | Ind1; EUVE J2115-586 | HST data is spectroscopic (STIS) | V2151 Cyg | HIP 105230 | spurious variable | CV Aqr | HV 6262 | minor planet (52) Europa | V1075 Cyg | S 8393 | a spectrum by 1997-07S shows a featureless blue continuum | Peg | NGC 7078 C | HST data is imaging (WFPC2) | Peg | NGC 7078 CCZ-V1 | 0.3" northeast of M15 center; HST data is imaging (WFPC2, FOC, ACS, and STIS) | Peg | NGC 7078 B | could also be a soft queiscent X-ray transient; HST data is imaging (WFPC2) | Cyg | RX J2130.3+4709 | object lost in glare of bright star (HD 204906);
see original reference for clear identification | CI Gru | Gru1; Hawkins V6 | period 0.056d (1995-73) is uncertain/unreliable | Cyg | RX J2133.7+5107 | coordinates measured on DSS plate 07WE | V630 Cyg | S 4556 | period 0.0764d (2001-85) is estimated from the superhump period using
the empirical relation by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | LQ Peg | Peg6; PG 2133+115 | period 0.121d (1993-10) is uncertain/unreliable | Cap2 | NGC 7089 V4; NSV 257 | southwest object of pair | V1570 Cyg | S 9726 | G-star spectrum | V1251 Cyg | Wr 160 | finding chart from J. Thorstensen; period 0.07376 (1998-46) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | CF Gru | Gru3; 2138-453 | period 0.069d (1995-73) is uncertain/unreliable | SS Cyg | BD +42 4189a | HST data is astrometric (FGS), imaging (STIS), and spectroscopy (GHRS,STIS) | V1760 Cyg | | Mira variable | Cyg | NSV 25747 | no candidate, field map shown | V2209 Cyg | Antipin V66 | southeast component of pair is blue; finding chart from J.
Thorstensen | Aqr | ROTSE3 214850-020622 | no candidate, field map shown | Cyg5 | NSV 13904 | early-G star | Peg | Antipin V79 | also known as 1RXS J215434.4+355023; period 0.0637d (2004-87) is
estimated from the superhump period using the empirical relation given
by Stolz, B. and Schoembs, R. 1984, Astron. Astrophys., 132, 187 | BG Lac | BD +42 4267 | Cepheid variable | Cep | Lanning 420 | single outburst observed; tentative identification | PS Lac | VV 442 | a spectrum of the candidate object is that of a early-K star (1999-09S), so the object is likely mis-identified | Peg | SDSS J220553+115554 | HST data is imaging/spectroscopy (ACS) | Cep | NSV 25861 | no candidate, field map shown | KM Lac | VV 347 | close pair | RU Peg | 142.1904 | HST data is astrometric (FGS) | Aqr | ROTSE3 J221519 | full name is ROTSE3 J221519.8-003257.2 | CP Lac | 605.1936 | period 0.127d (2005-05) is uncertain/unreliable | V381 Lac | LD 197 | the (tentative) ID is based on the finding chart, but the
coordinates are off from the nominal position (2.9s west and 20'' south);
object somewhat bright on V plate; 2MASS source (K=7.78); likely a
long-period variable or slow irregular red giant | FO Aqr | H 2215-086 | HST data is spectroscopic (FOS) | AY Lac | 207.1928 | field map shown; the faint object in the center of the circle
may be the CV | MN Lac | VV 381 | object blue on POSS II plates | Lac | NSV 25894 | aircraft (Duerbeck, private communication) | MR Lac | VV 386 | a spectrum of the candidate object is that of a G star (1999-09S), so the object is likely mis-identified | IK Aqr | Aqr2; NSV 14152 | BL Lac | NQ Lac | VV 403 | subdwarf O star | BS Cep | 569.1936 | Herbig emission-line star | DI Lac | HD 214239 | HST data is spectroscopic (STIS) | Cep | HS 2237+8154 | object could be a pre-CV, a CV that terminated mass-transfer, or a
hibernating nova | Aqr1 | 2236+0052 | period 0.1344d (2004-10) is uncertain/unreliable | KQ Peg | PG 2240+193 | subdwarf B-O star | RZ Gru | S 5150 | period 0.360d (1998-87) is uncertain/unreliable | DK Lac | | object in decline on POSS I; HST data is imaging (WFPC2) | EG Lac | S 4617 | N. Samus (private communication) states that the object is bright on
POSS II infrared plates. Kinnunen and Skiff (2000, IBVS, 4906) suggest a
possible symbiotic classification | Cep1 | GD 552; NSV 25966 | HST data is spectroscopic (STIS) and astrometric (FGS) | AO Psc | H 2252-035 | HST data is spectroscopic (STIS) | V709 Cep | MisV1181 | no candidate, field map shown | Aqr | SDSS J225831-094932 | period 0.080 (2005-113) is estimated from the superhump
period using the empirical relation given by Stoltz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | V368 Peg | Antipin V63 | period 0.073d (2003-82) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | MS Peg | GD 245 | pre-cataclysmic variable; plate epoch = 1983.774 | Peg3 | NSV 26002 | also known as PG 2300+166; originally classified as a
cv, the spectrum is that of a hot object | V369 Peg | NSV 26006 | period 0.0817 (2001-39) is estimated from the superhump period using
the empirical relation given by Stolz, B. and Schoembs, R. 1984,
Astron. Astrophys., 132, 187 | AN Gru | S 6526 | RR Lyrae star | And | NSV 14443 | no candidate, field map shown; existence doubtful | OS And | | HST data is imaging (WFPC2) | LM Cas | S 4633 | object slightly in outburst on plate shown | Peg | RX J2313+2117 | M-dwarf | EZ Peg | BD +24 4742 | RS CVn variable | Psc2 | PG 2315+071 | binary with hot subdwarf | Scl1 | GD 1555; NSV 26056 | white dwarf | Peg5 | KUV 23182+1007 | quasar | IP Peg | SVS 2549 | HST data is spectroscopic (FOS) | AY Oct | S 6613 | RR Lyrae star | VY Scl | GD 1662/PHL 538 | HST data is spectroscopic (STIS); period 0.2323d (2000-107) is uncertain/unreliable | EI Psc | 1RXS J2329+0628 | HST data is spectroscopic (STIS) | And | HS 2331+3905 | HST data is spectroscopic (STIS) | EH Aqr | BV 5/PHL 563 | object blue on POSSII plate | Peg | NSV 14652 | ID based on POSS plates; possible ROSAT ID is 1RXS-F
J2338+2820; period 0.079 (2005-112) is estimated from the superhump
period using the empirical relation given by Stoltz, B. and Schoembs,
R. 1984, Astron. Astrophys., 132, 187 | V705 Cas | | object is the north component with the measured
object; period 0.2280d (1995-51) is uncertain/unreliable | And | LD 317 | also known as RXS J2344.9+4331? | Aqr | | no candidate, field map shown | VZ Scl | Ton S 120 | HST data is spectroscopic (STIS) | BC Cas | SVS 254 | see the spectrum in 1994-07S which does not show emission | BW Scl | RX J2353.0-3852 | HST data is spectroscopic (STIS) | V379 Peg | Peg7; NSV 26158 | also known as FBS 2351+228; object A is the original, red
identification (2002-93), while object B is the new, blue candidate
(coordinates above are for this object); object may be white dwarf-red
dwarf pair, or low mass-transfer rate CV | Peg4 | PG 2357+125 | composite spectrum of a white dwarf and a mid-M star with no evidence of interaction | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |