V0735 And  | Magnitudes in the Table can be influenced by surrounding bright stars.
V0736 And  | VB AB (AB 11.03mV; 0.1", 115deg, 1973; A and B estimated equally bright). Magnitudes in the Table can be influenced by a 10.60mV star BD +36 0159 (50", 252deg, 1999).
V0744 And  | Porb = 0.02608d.
V0751 And  | A twice shorter period is not excluded.
V0762 And  | Studied in [81025] (SAVS 023548+491758) but erroneously identified with GSC 03303-01008.
CH    Ant  | Multiperiodic, 4 harmonics. P1 is given in the Table.
CI    Ant  | VB A (B 13.1m, 1", 306deg, 1991).
CN    Ant  | P strongly varies. The elements in the Table are for JD 2453569 - 2454298.
V0367 Aps  | VB B (A 11.3m; AB 8", 58deg, 2000).
V0380 Aps  | VB (several companions).
V0919 Ara  | SB2.
V0927 Ara  | VB A (B 13.3m, 14", 121deg, 1999). The magnitude in minimum is influenced with the companion.
V0943 Ara  | Similarity to FG Sge is not excluded.
V0952 Ara  | Multiperiodic, 5 frequencies detected.
V0969 Ara  | VB A (B 13.8m, 16", 148deg, 1999).
V0978 Ara  | P=46.5d is superposed.
V0981 Ara  | Blazhko effect, P = 58.66d.
V0982 Ara  | VB B (A 13.9mpg, B 14.3mpg; AB 13", 351deg, 2000). The magnitudes in the Table are influenced by the companion.
CP    Ari  | VB A (B 7", 149deg, 1997).
CR    Ari  | Type ELL with the light elements Min = 2455181.6141 + 0.361849d x E is also possible.
V0674 Aur  | P = 0.29779d is not excluded. Type EW, with periods 0.59563d or 0.63533d, is also possible.
V0681 Aur  | Blazhko effect.
V0695 Aur  | Running numbers and USNO-B1.0 numbers in [81080] are mixed up; corrected by GCVS compilers.
V0696 Aur  | Running numbers and USNO-B1.0 numbers in [81080] are mixed up; corrected by GCVS compilers.
V0697 Aur  | VB A (B 6", 70deg, 1997).
V0698 Aur  | Eccentric binary. Running numbers and USNO-B1.0 numbers in [81080] are mixed up; corrected by GCVS compilers.
V0707 Aur  | O'Connell effect.
V0708 Aur  | O'Connell effect.
V0716 Aur  | MinII - MinI = 0.47P.
V0742 Aur  | DSCTC type with P=0.132695d is also possible.
V0744 Aur  | VB A (B 5", 9deg, 2000). P = 0.362922d is also possible.
V0746 Aur  | P = 0.086921d is also possible.
V0750 Aur  | Multiperiodic, P2 = 0.069397.
V0754 Aur  | P = 0.33285d is also possible.
V0765 Aur  | VB A (B 4", 91deg, 1997).
V0786 Aur  | VB A (B 3", 183deg, 1989).
V0790 Aur  | Type EW with a twice longer period is not excluded.
V0798 Aur  | VB A (12.4mV; B 14.7:mV, 7", 286deg, 1998).
V0803 Aur  | Multiperiodic. P2 = 0.05503008d, P3 = 0.04250400d.
V0808 Aur  | Eclipses: Min = 2455126.8960 + 0.081376d x E, range 17.8 - 21.4 V, D = 0.06P.
V0815 Aur  | VB A (B 16.5mpg, 5", 75deg, 2000).
V0817 Aur  | MinII - MinI = 0.32P.
V0823 Aur  | Secondary period P2 = 0.2980d.
V0349 Boo  | P strongly varies. The coordinates in [81005] refer to a brighter neighbor.
V0352 Boo  | Multiperiodic. The period of the first-overtone radial mode is given in the Table. Two non-radial modes: P2 = 0.347051d, P3 = 0.342383d.
V0524 Cam  | Distortion wave: P = 0.499464d.
V0525 Cam  | Distortion wave: P = 0.461208d.
V0534 Cam  | MinII - MinI = 0.545P.
V0542 Cam  | Multiperiodic. P1 is presented in the Table; P0 = 0.174773d. VB A (11.70mV; B 13.55mV, 17", 191deg, 1999).
V0549 Cam  | MinII - MinI = 0.543P. O'Connell effect.
V0565 Cam  | VB A (B 14.9mF, 7", 139deg, 2000); the amplitude in the Table is too low because of the companion.
MR    Cnc  | Pulsates in the first overtone (see Table) and fundamental (Max = 2454701.537 + 0.536525d x E) modes. P1/P0 = 0.7462.
MY    Cnc  | Double-mode, with a radial and a none-radial modes excited. The second light elements: Max = 2454700.652 + 0.281995d x E. P2/P1 = 0.9824.
GP    CVn  | Light elements for eclipses: Min = 2453796.248245 + 0.062959041d x E [81139].
GR    CVn  | The Table presents the period of first-overtone pulsations; P0 = 0.486651d. P1/P0 = 0.7443.
V0432 CMa  | MinII - MinI = 0.53P.
V0835 Car  | SB2.
V0845 Car  | SB2.
V0846 Car  | Multiperiodic, 3 harmonics.
V0865 Car  | MinII - MinI = 0.605P.
V0867 Car  | VB B (A 12.6mV; AB 4.5", 194deg, 2000).
V0869 Car  | MinII - MinI = 0.45P.
V0887 Car  | MinII - MinI = 0.445P.
V0889 Car  | MinII - MinI = 0.370P.
V0890 Car  | A twice shorter period is also possible.
V0899 Car  | Double-mode pulsations. The Table gives the fundamental-mode elements. For the first overtone, P1 = 0.0858512d.  P1/P0 = 0.7748.
V0901 Car  | Large scatter outside eclipses; intrinsic variability?
V1255 Cas  | Twice shorter period and type RRC are possible.
V1271 Cas  | MinII - MinI = 0.525P.
V1276 Cas  | Light curve shape varies.
V1277 Cas  | Multiperiodic, P2 = 0.0876987d.
V1280 Cas  | Multiperiodic.
V1375 Cen  | Porb = 0.3604d? [81150].
V1389 Cen  | SB2?
V1393 Cen  | Double-mode pulsations. P1 is given in the Table. P0 = 0.1177831. P1/P0 = 0.7712.
V1397 Cen  | Blazhko effect, P = 146d.
V1400 Cen  | Starspots rotational modulation with P = 3.219d. One deep minimum, with secondary fadings before and after it, was observed. Probably a pre-main sequence star.
IO    Cet  | VB A (12.1mV; B 13mV, 14", 173deg, 1998). The range in the Table is for combined magnitudes.
IQ    Cet  | P1 is presented in the Table; P1/P0 = 0.7438.
IU    Cet  | P1 is presented in the Table; P1/P0 = 0.7425.
IZ    Cet  | SB, Porb = 8.1194d.
KM    Cet  | P1 is presented in the Table. P0 = 0.542695d.
KN    Cet  | Eclipsing variability outside outbursts: 17.2m*-19.9m*, Min = 2455202.5579 + 0.05298466 x E [81196].
KR    Cet  | P1 is presented in the Table; P1/P0 = 0.7434.
FG    Cir  | VB A (B 13.9mpg, 19", 339deg, 2000); B is in 3" sf to AR Cir, Nova Cir 1906.
FH    Cir  | Multiperiodic. Light elements with P1 are given in the Table. P2 = 0.1260864. P2/P1 = 0.8279.
BI    Col  | Type EW with a twice longer period is not excluded, having in mind association with an X-ray source [81001].
BK    Col  | P varies strongly [80001].
BL    Col  | Blazhko effect, P = 40.5d.
BQ    Col  | Blazhko effect, P = 15.33d?
QQ    Com  | P strongly varies.
CZ    CrB  | P strongly varies.
YZ    Crv  | VB B (A 16.2mpg, B 16.2mpg; AB 27", 192deg, 2000). The coordinates in [81005] refer to the A component.
AA    Crv  | VB B (A 12.7mpg, B 15.9mpg; AB 28", 220deg, 1998). The coordinates in [81005] refer to the brighter star.
V0458 Dra  | The light elements could not be confirmed [81001] using the Catalina Surveys data.
V0462 Dra  | P = 0.21157d is not excluded.
V0472 Dra  | VB B (A 13.7m; B 14.5m, 19", 199deg, 1999). The tabulated variability range is influenced with the companion.
V0485 Dra  | Type ELL is not excluded.
V0486 Dra  | The coordinates in [81005] refer to a neighbor star.
V0506 Dra  | P varies.
NN    Eri  | Blazhko effect, P = 335.29d.
NP    Eri  | Blazhko effect [81005].
NX    Eri  | P0 is presented in the Table; P1 = 0.354824d.
BF    For  | VB A (B 11.0m, 2", 170deg, 1991).
BI    For  | P varies? Light elements for JD 2454000 - 2455165 are presented in the Table.
V0439 Gem  | A twice longer period is not excluded.
V0455 Gem  | Multiperiodic.
V1366 Her  | P strongly varies, current elements after JD 2456000 are given in the Table.
V1373 Her  | Period varies.
V1377 Her  | Period varies.
V1390 Her  | MinII - MinI = 0.46P.
V1396 Her  | Blazhko effect.
V0571 Hya  | Blazhko effect, P = 11.80d.
V0575 Hya  | Blazhko effect, P = 8.52d.
V0588 Hya  | Blazhko effect, P = 87.73d [81056].
V0592 Hya  | Possibly Blazhko effect with P = 14.2d.
V0598 Hya  | VB A (15.4mpg; B 15.6mpg, 18", 43deg, 2000). The coordinates in [81005] refer to the companion.
V0599 Hya  | VB B (A 15.1mpg, B 16.6mpg; AB 29", 152deg, 2000). The coordinates in [81005] refer to the brighter star.
V0603 Hya  | Double-mode pulsations. The Table contains the period for the first overtone. Fundamental mode: P0 = 0.4867803. P1/P0 = 0.7449.
LR    Leo  | Pulsates in the first overtone (see Table) and fundamental (Max = 2454701.577 + 0.557447d x E) modes. P1/P0 = 0.7469. A nonradial mode with P = 0.559369d may also be present.
LU    Leo  | O'Connell effect.
LY    Leo  | O'Connell effect.
LZ    Leo  | VB A (13.6mV; B 15.7mV, 9", 258deg, 2000).
MV    Leo  | Porb = 0.14608d.
NV    Leo  | Double-mode pulsations. The Table gives the first-overtone light elements. For the fundamental mode, Max = 2454800.541 + 0.483098d x E. P1/P0 = 0.7441.
OX    Leo  | Multiperiodic. P2 = 0.89405d.
BL    Lep  | VB (6", 19deg, 1999); the variable is probably the southern component. Combined magnitudes are presented in the Table.
BN    Lep  | P varies strongly.
BO    Lep  | VB A (11.4mV; B 11.6mV, 19", 163deg, 1998).
V0364 Lib  | Two outbursts were observed. Porb = 0.70242d.
V0366 Lib  | P varies. The light elements in the Table are for JD 2453639 - 2455100.
V0368 Lib  | Double-mode pulsations. The Table contains light elements for the first overtone. Fundamental mode: Max = 2455000.800 + 0.57857d x E. P1/P0 = 0.7443.
HS    Lyn  | A twice shorter period is not excluded.
IW    Lyn  | VB A (B 7", 349deg, 1999).
IZ    Lyn  | Probably a VB unresolved in the photometry.
KX    Lyn  | [Fe/H] = -1.9.
LO    Lyn  | Blazhko effect, P=9.763d.
LR    Lyn  | Blazhko effect? [81001].
V0960 Mon  | In a nebula.
V0962 Mon  | SB2, Porb = 5.32d; the F2V component varies. Multiperiodic; other periods are P2 = 0.77214d and P3 = 0.68432d.
V0964 Mon  | VB AB (12.5m, 13.0m, 2".7, 213deg, 2000).
V0965 Mon  | Blazhko effect, P=37.24d.
V0966 Mon  | Pulsates in the first (see Table) and second (Max = 2453761.54 + 0.85905d x E) overtone modes. P2/P1 = 0.8043.
V0972 Mon  | A period of 0.948d was also detected.
V0973 Mon  | The amplitude of periodic variations (see Table) is 0.08m; a single flare was observed.
V0975 Mon  | Light elements for eclipses are tabulated. Outside eclipses, P = 3.25d, amplitude 0.03m. VB A (B = NSV 03138, 16.1 - 16.7mV, 7", 357deg, 1999).
V0979 Mon  | The light elements for the first overtone are given in the Table. Second overtone: Max = 2453800.32 + 1.03153 x E. P2/P1 = 0.8005.
V0982 Mon  | VB A (B 14.35mF, 10", 256deg, 1998).
V0985 Mon  | Pulsates in the first (see Table) and second (Max = 2453674.01 + 0.70772d x E) overtone modes. P2/P1 = 0.8046.
V0988 Mon  | P = 0.36319d is also possible.
V0989 Mon  | VB A (B 6", 264deg, 1998).
V0355 Mus  | SB2.
V0356 Mus  | Double-mode pulsations. The Table gives the first-overtone light elements. For the second overtone, Max = 2453693.12 + 0.734376d x E. P2/P1 = 0.8043.
V0495 Nor  | SB2.
V0498 Nor  | VB B (A 9.25mV; B 9.72mV, A6V, 7", 160deg, 1998). Combined magnitudes are presented in the Table.
V0501 Nor  | VB A (B 5", 99deg, 20000). Combined magnitudes are presented in the Table.
V2837 Oph  | The period in the Table is that of spot variability. SB2, Porb = 591d. VB A (B = V2252 Oph, 13", 123deg, 1998).
V2857 Oph  | O'Connell effect.
V2862 Oph  | VB A (B 19.7m, 2.5", 289deg).
V2897 Oph  | P = 129d is superposed.
V2918 Oph  | A twice shorter period is not excluded.
V2925 Oph  | P varies [81101].
V2930 Oph  | Blazhko effect.
V2947 Oph  | VB A (B 14.0m, 12", 93deg, 1998). The magnitude at minimum in the Table can be influenced by the companion.
V2797 Ori  | Multiperiodic.
V0966 Per  | MinII - MinI = 0.33P. e = 0.284.
V0982 Per  | MinII - MinI = 0.38P.
V1024 Per  | VB A (B 4", 168deg, 1989).
V1035 Per  | Type DSCT with P = 0.1441d is also possible.
V1036 Per  | Type SR with P = 71d is not excluded.
V1041 Per  | Type SR with P = 160d is not excluded.
V1043 Per  | The epoch in the Table corresponds to the eclipse-like feature of the light curve but not to the overall brightness minimum.
DN    Phe  | Blazhko effect?
DP    Phe  | P probably varies.
DR    Phe  | Blazhko effect, P=40.17d [81056].
AW    Pic  | Blazhko effect. P(Bl) = 756d [81001].
AX    Pic  | P varies.
AY    Pic  | SB2.
V0707 Pup  | P varies strongly.
V0711 Pup  | VB A (B 5", 128deg, 1999).
V0714 Pup  | Blazhko effect, P=116.96d.
V0716 Pup  | P varies strongly.
V0719 Pup  | Pulsates in the first (see Table) and second (Max = 2453455.40 + 0.593216d x E) overtone modes. P2/P1 = 0.8057. VB A (B 11.0m, 6", 42deg, 1999); the tabulated range is for the combined brightness.
V0722 Pup  | SB2.
V0725 Pup  | VB A (B 10.3m, 1", 47deg, 1991).
V0732 Pup  | Pulsates in the first (see Table) and second (Max = 2453456.065 + 0.333105d x E) overtone modes. P2/P1 = 0.8007.
V0733 Pup  | Pulsates in the fundamental mode (see Table) and in the first overtone (Max = 2453600.055 + 0.1742342d x E). P1/P0 = 0.7618.
V1537 Sco  | Multiperiodic. VB A (8.1mV; B 12.6mV, 1.9", 231deg, 1939).
V1544 Sco  | It is assumed that there is a typo in the star's declination in [81021].
V1547 Sco  | Simultaneous presence of two periods. P1 is given in the Table. P2 = 2.27816d.
V1552 Sco  | VB A (B 16.0m, 11", 111deg, 2000).
V1553 Sco  | Double-mode pulsations. The period for the fundamental mode is given in the Table. P1 = 0.1470447d. P1/P0 = 0.7978.
V1560 Sco  | VB A (B 15.0m, 6", 147deg, 1999).
V1611 Sco  | MinII - MinI = 0.65P.
V1614 Sco  | Several close companions.
CY    Scl  | Blazhko effect.
DE    Scl  | P1 is presented in the Table; P1/P0 = 0.7448.
DI    Scl  | SB2.
V0562 Ser  | d = 0.07P.
V0575 Ser  | Double-mode pulsations. The Table contains light elements for the first overtone. Fundamental mode: Max = 2454700.867 + 0.475615d x E. P1/P0 = 0.7446.
V0579 Ser  | Double-mode pulsations. The Table contains light elements for the first overtone. Fundamental mode: Max = 2454800.609 + 0.479144d x E. P1/P0 = 0.7444.
V0585 Ser  | SiO maser.
V0592 Ser  | VB A (B 14.0mpg, 13", 80deg, 1998).
V0595 Ser  | VB A (B 5" p).
BY    Sex  | Pulsates in the first overtone (see Table) and fundamental (Max = 2454801.000 + 0.581288d x E) modes. P1/P0 = 0.7473.
CF    Sex  | P strongly varies. The elements in the Table are for JD 2455900 - 2456500.
V1384 Tau  | Multiperiodic. P1 is presented in the Table; P0 = 0.1397914d.
V1392 Tau  | Multiperiodic. P0 is presented in the Table; P1 = 0.0579031d.
V1403 Tau  | Close VB.
V1412 Tau  | P=0.3409505d is also possible.
V1414 Tau  | P = 0.195018d is also possible.
DE    Tri  | P = 30.6d is not excluded.
V0347 TrA  | Blazhko effect, P=118.05d.
V0348 TrA  | Double-mode pulsations. The Table contains light elements for the first overtone. Second overtone: Max = 2453600.091 + 0.1224057d x E. P2/P1 = 0.8279.
V0351 TrA  | P = 49.5d is superposed.
V0374 UMa  | Multiperiodic, 4 harmonics.
V0379 UMa  | P1 is given in the Table. P0 = 0.494909d, P1/P0=0.7446.
V0380 UMa  | Pulsates in the first overtone (see Table) and fundamental (Max = 2454876.9243 + 0.47451d x E) modes. P1/P0 = 0.743.
V0384 UMa  | Type EW with a twice longer period is also possible.
V0389 UMa  | Double-mode pulsations. The Table gives the first-overtone light elements. For the fundamental mode, Max = 2454847.9552 + 0.47119d x E. P1/P0 = 0.744.
V0415 UMa  | P = 1.56575d is also possible.
V0417 UMa  | O'Connell effect.
V0430 UMa  | Other detected periods are 0.0037005d and 0.0024173d.
AN    UMi  | VB A (14.4mV; B 15.8mV, 8", 63deg, 2000). The variability range in the Table is for combined light.
V0519 Vel  | Pulsates in the first (see Table) and second (Max = 2453426.48 + 0.939354d x E) overtone modes. P2/P1 = 0.8052.
V0526 Vel  | Double-mode pulsation. For the fundamental-mode period, see the Table. P1 = 0.0624889d, P1/P0 = 0.8062.
V0528 Vel  | Multiperiodic, 4 harmonics.
V0533 Vel  | SB2.
V0540 Vel  | Double-mode pulsation. P2 = 0.1765777d.
V0547 Vel  | SB2.
V0548 Vel  | Multiperiodic. P2 = 0.0482189d.
V0613 Vir  | P strongly varies.
V0630 Vir  | The Table presents the light elements for the first overtone. For the fundamental mode, Max = 2454800.650 + 0.524429d x E. P1/P0 = 0.7453.
V0644 Vir  | Double-mode pulsations. The Table gives the first overtone light elements. For the fundamental mode, Max = 2454800.145 + 0.455977d x E. P1/P0 = 0.7426.
V0659 Vir  | Double-mode pulsations. The Table contains light elements for the first overtone. Fundamental mode: Max = 2454800.750 + 0.505828d x E. P1/P0 = 0.7450.