V0782 And | MinII - MinI = 0.383P.
V0784 And | P1 is presented in the Table. P0 = 0.534895d; P1/P0 = 0.7465.
V0787 And | P1 is presented in the Table. P0 = 0.542396d; P1/P0 = 0.7465.
V0788 And | P1 is presented in the Table. P0 = 0.529664d; P1/P0 = 0.7461.
V0796 And | P1 is presented in the Table. P0 = 0.470490d; P1/P0 = 0.7442.
V0797 And | Additional non-radial pulsation, Pnr = 0.18776d.
            P1 is presented in the Table; Pnr/P1 = 0.9162.
V0799 And | VB (A 10.3m; B 10.9m, 6", 320deg, 2016). The magnitudes in the Table are for combined brightness.
V0800 And | Biperiodic, P2 = 71.2d.
V0806 And | MinII - MinI = 0.494P.
V0807 And | d = 0.08P. The elements in the table are for planet transits. Superposed DSCT
          | oscillations: P = 0.0476d [023].
DN    Ari | P1 is presented in the Table. P0 = 0.547871d; P1/P0 = 0.7466.
DO    Ari | P1 is presented in the Table. P0 = 0.564048d; P1/P0 = 0.7455.
DP    Ari | P1 is presented in the Table. P0 = 0.492409d; P1/P0 = 0.7449.
DQ    Ari | P1 is presented in the Table. P0 = 0.480781; P1/P0 = 0.7441.
DS    Ari | VB B (A 15.3mV, const, at the coordinates of 1SWASP J022727.03+115641.7;
          | B varies, AB 12", 309deg, 2000; C 17.3mV, AC 14", 348deg, 2000). The data in
          | in [82030] are for combined brightness. The magnitudes in the Table also seem
          | to be somewhat influenced with the companions.
DT    Ari | P1 is presented in the Table. P0 = 0.561570d; P1/P0 = 0.7455.
DV    Ari | P1 is presented in the Table. P0 = 0.481500d; P1/P0 = 0.7448.
V0829 Aur | Possible BY variations outside flares: P = 1.04098d, 16.4m - 16.6m.
V0830 Aur | VB A (B 6", 176deg, 2000). The range in the Table is for combined brightness.
V0837 Aur | VB A (B 13.4m, 19", 94deg, 2000; C 5", 281deg, 2000).
V0838 Aur | MinII - MinI = 0.330P.
V0839 Aur | MinII - MinI = 0.438P.
V0841 Aur | VB B (A 10.8mV; AB 16", 351deg, 2007).
V0849 Aur | Two systems of eclipses. The Table presents the light elements for system A.
          | MinII - MinI = 0.52P. System B: MinI = 2455968.3398 + 0.806931 x E; D = 0.14P.
V0856 Aur | VB A (B 13.3m, 17", 345deg, 1998).
V0860 Aur | The data for 1SWASP J070953.45+364417.3 in [82030] are combined measurementss for a
          | non-variable star (V = 12.8) near the SuperWASP position and the real variable.
V0861 Aur | P1 is presented in the Table. P0 = 0.555912d; P1/P0 = 0.7464.
V0381 Boo | P1 is presented in the Table. P0 = 0.534137d; P1/P0 = 0.7457.
V0383 Boo | P1 is presented in the Table. P0 = 0.472061d; P1/P0 = 0.7439.
V0384 Boo | P1 is presented in the Table. P0 = 0.532235d; P1/P0 = 0.7460.
V0386 Boo | P1 is presented in the Table. P0 = 0.555941d; P1/P0 = 0.7457.
V0388 Boo | P1 is presented in the Table. P0 = 0.527220d; P1/P0 = 0.7460.
V0392 Boo | Additional non-radial mode, P = 0.2909421d; P(Blazhko) = 27.6d.
V0394 Boo | P1 is presented in the Table. P0 = 0.478545d; P1/P0 = 0.7449.
V0395 Boo | P0 is presented in the Table. P1 = 0.345662d; P1/P0 = 0.7433.
V0396 Boo | P1 is presented in the Table. P0 = 0.536540d; P1/P0 = 0.7464.
V0397 Boo | P1 is presented in the Table. P0 = 0.506502d; P1/P0 = 0.7440.
V0398 Boo | Additional non-radial mode, P = 0.2645555d; P(Blazhko) = 14.1d.
V0399 Boo | P1 is presented in the Table. P0 = 0.492554d; P1/P0 = 0.7453.
V0401 Boo | P1 is presented in the Table. P0 = 0.493517d; P1/P0 = 0.7444.
V0403 Boo | P1 is presented in the Table. P0 = 0.564890d; P1/P0 = 0.7457.
V0405 Boo | P1 is presented in the Table. P0 = 0.546206d; P1/P0 = 0.7453.
V0407 Boo | VB A (14.1mV; B 14.5mV, 22", 113deg, 1998).
V0411 Boo | P1 is presented in the Table. P0 = 0.476987d; P1/P0 = 0.7442.
V0412 Boo | P1 is presented in the Table. P0 = 0.483115d; P1/P0 = 0.7444.
V0413 Boo | P1 is presented in the Table. P0 = 0.480226d; P1/P0 = 0.7440.
V0414 Boo | Additional non-radial mode, P = 0.324200d; P(Blazhko) = 36.6d.
V0415 Boo | P1 is presented in the Table. P0 = 0.552367d; P1/P0 = 0.7457.
V0588 Cam | Period varies.
V0602 Cam | Type SR with P = 92d is not excluded.
V0609 Cam | VB B (A 11.7m; AB 26", 239deg, 2000; C 14.2m, AC 38", 302deg, 2000).
V0610 Cam | P1 is presented in the Table. P0 = 0.47921d6; P1/P0 = 0.7443.
NN    Cnc | P1 is presented in the Table. P0 = 0.478318d; P1/P0 = 0.7448.
NP    Cnc | P1 is presented in the Table. P0 = 0.498566d; P1/P0 = 0.7449.
NU    Cnc | P1 is presented in the Table. P0 = 0.472146d; P1/P0 = 0.7432.
NW    Cnc | P1 is presented in the Table. P0 = 0.481136d; P1/P0 = 0.7446.
OO    Cnc | P1 is presented in the Table. P0 = 0.505835d; P1/P0 = 0.7443.
PR    Cnc | P1 is presented in the Table. P0 = 0.482865d; P1/P0 = 0.7450.
PS    Cnc | P1 is presented in the Table. P0 = 0.478487d; P1/P0 = 0.7442.
PU    Cnc | P1 is presented in the Table. P0 = 0.489181d; P1/P0 = 0.7443.
PW    Cnc | VB A (B = NEXT STAR IN THE LIST, 12", 171deg, 1997).
PX    Cnc | A twice longer period is not excluded. VB B (A = PREVIOUS STAR IN THE LIST; AB 12", 171deg, 1997).
QQ    Cnc | P1 is presented in the Table. P0 = 0.483002d; P1/P0 = 0.7441.
QU    Cnc | P1 is presented in the Table. P0 = 0.542956d; P1/P0 = 0.7456.
HK    CVn | P1 is presented in the Table. P0 = 0.478824d; P1/P0 = 0.7442.
HL    CVn | P1 is presented in the Table. P0 = 0.555276d; P1/P0 = 0.7462.
HM    CVn | P1 is presented in the Table. P0 = 0.526289d; P1/P0 = 0.7459.
HP    CVn | P1 is presented in the Table. P0 = 0.479250d; P1/P0 = 0.7446.
HQ    CVn | Strong O'Connell effect.
HS    CVn | P1 is presented in the Table. P0 = 0.531760d; P1/P0 = 0.7451.
HU    CVn | The mean brightness slowly varies by about 0.1mV. The depths of MinI and MinII are about 0.1mV.
HV    CVn | P1 is presented in the Table. P0 = 0.514168d; P1/P0 = 0.7450.
HX    CVn | P1 is presented in the Table. P0 = 0.513224d; P1/P0 = 0.7452.
V0436 CMa | The data for 1SWASP J061236.44-281553.0 in [82030] are combined measurements for a
          | non-variable star (V = 14.8m) near the SuperWASP position and the real variable.
V0441 CMa | Multiperiodic.
V0442 CMa | Multiperiodic.
V0445 CMa | MinII - MinI = 0.56P.
V0450 CMa | MinII - MinI = 0.73P.
V0451 CMa | For SRD light elements, see the Table. Eclipses: Min = 2453707.98 + 8.2958d x E, amplitude 0.2m.
V0911 Car | Epoch of minimum brightness is given in the Table. Secondary minimum at about 11.4m. P = 44.9d is superposed.
V0914 Car | MinII - MinI = 0.90P.
V1315 Cas | Type DCEPS is also possible.
V1316 Cas | VB B (A 14.3mV; AB 23", 165deg, 1998). The object 1SWASP
            J011732.10+525204.9, announced variable in [82030], is a blend
            of the non-variable component A near the SuperWASP position and
            the really variable component B.
V1345 Cas | Type EW with a twice longer period is also possible.
V1355 Cas | VB (companion: 6", 259deg, 1999).
V1378 Cas | Type RRC with a twice shorter period is also possible.
V1386 Cas | MinII - MinI = 0.465P.
V1406 Cen | The data for 1SWASP J111501.66-361254.2 in [82030] are combined measurements for a
          | non-variable star (V = 15.4m) near the SuperWASP position and the real variable.
V1411 Cen | The data for 1SWASP J121359.79-414742.7 in [82030] are combined measurements for a
          | non-variable star (V = 13.2m) near the SuperWASP position and the real variable.
V1415 Cen | In the field of the globular cluster NGC 5139 = Omega Cen.
V1418 Cen | P = 60.7d is superposed.
V1419 Cen | P = 45.0d is superposed.
V1425 Cen | P = 14.896d is superposed.
V1429 Cen | A secondary wave (possibly nonradial) with P = 0.103095d.
V1024 Cep | Eclipses: Min = 2451859.2468 + 0.14872385d x E, amplitude 1.4m.
KS    Cet | P1 is presented in the Table. P0 = 0.564845d; P1/P0 = 0.7456.
KY    Cet | Period strongly varies. The light elemens in
            the Table are for JD 2455600 - 56600.
LN    Cet | P1 is presented in the Table. P0 = 0.530534d; P1/P0 = 0.7459.
LQ    Cet | P1 is presented in the Table. P0 = 0.465495d; P1/P0 = 0.7433.
LT    Cet | Additional non-radial mode, P = 0.2820182d, or Blazhko effect, P = 231d.
LU    Cet | Multiperiodic. P2 = 0.8488154d, P3 = 0.4776334d.
FO    Cir | The maximum could be earlier and brighter, no observations during the ascending branch.
FP    Cir | Double-mode pulsations. P = 0.0976718 is superposed.
QU    Com | P1 is presented in the Table. P0 = 0.541781d; P1/P0 = 0.7456.
QW    Com | P1 is presented in the Table. P0 = 0.547401d; P1/P0 = 0.7455.
QX    Com | P1 is presented in the Table. P0 = 0.544233d; P1/P0 = 0.7454.
QY    Com | P1 is presented in the Table. P0 = 0.490349d; P1/P0 = 0.7446.
QZ    Com | Additional non-radial mode, P = 0.2687276d; P(Blazhko) = 13.7d.
V0335 Com | P1 is presented in the Table. P0 = 0.515253d; P1/P0 = 0.7460.
V0336 Com | P1 is presented in the Table. P0 = 0.480562d; P1/P0 = 0.7439.
V0337 Com | P1 is presented in the Table. P0 = 0.478242d; P1/P0 = 0.7439.
V0338 Com | P1 is presented in the Table. P0 = 0.485204d; P1/P0 = 0.7440.
V0340 Com | P1 is presented in the Table. P0 = 0.460448d; P1/P0 = 0.7425.
V0341 Com | P1 is presented in the Table. P0 = 0.476173d; P1/P0 = 0.7443.
V0342 Com | P1 is presented in the Table. P0 = 0.488314d; P1/P0 = 0.7447.
V0343 Com | P1 is presented in the Table. P0 = 0.486854d; P1/P0 = 0.7443.
DE    CrB | P1 is presented in the Table. P0 = 0.554870d; P1/P0 = 0.7460.
DG    CrB | P1 is presented in the Table. P0 = 0.539078d; P1/P0 = 0.7456.
DH    CrB | P1 is presented in the Table. P0 = 0.551550d; P1/P0 = 0.7464.
DI    CrB | P1 is presented in the Table. P0 = 0.508196d; P1/P0 = 0.7452.
DK    CrB | MinII - MinI = 0.482P.
DL    CrB | Time-variable O'Connell effect.
AD    Crv | Additional non-radial mode, P = 0.2691307d; P(Blazhko) = 185d.
AG    Crv | P1 is presented in the Table. P0 = 0.537739d; P1/P0 = 0.7465.
AH    Crv | P1 is presented in the Table. P0 = 0.488888d; P1/P0 = 0.7450.
AV    Crt | A period about 3497d is possibly superposed.
AX    Crt | P1 is presented in the Table. P0 = 0.521023d; P1/P0 = 0.7454.
AY    Crt | P1 is presented in the Table. P0 = 0.483101d; P1/P0 = 0.7446.
V0546 Dra | P0 is presented in the Table. P1 = 0.351671d; P1/P0 = 0.7438.
V0552 Dra | Double-mode pulsations, also P = 0.0475034d.
V0555 Dra | P1 is presented in the Table. P0 = 0.551274d; P1/P0 = 0.7461.
V0556 Dra | O'Connell effect.
V0557 Dra | P1 is presented in the Table. P0 = 0.510745d; P1/P0 = 0.7459.
V0558 Dra | P1 is presented in the Table. P0 = 0.472239d; P1/P0 = 0.7436.
V0560 Dra | P1 is presented in the Table. P0 = 0.469194d; P1/P0 = 0.7432.
V0561 Dra | P1 is presented in the Table. P0 = 0.484660d; P1/P0 = 0.7447.
OX    Eri | Repeated outbursts in 2014, with intervals increasing approximately
          | from 10 to 20 days.
V0483 Gem | P0 is presented in the Table. P1 = 0.1173070d; P1/P0 = 0.7685.
V0487 Gem | The magnitude range in the Table is for BY-type brightness variations. Five flares were also detected.
V0506 Gem | P1 is presented in the Table. P0 = 0.551687d; P1/P0 = 0.7465.
V0512 Gem | The ephemeris of eclipses is presented in the Table. Pulsations: peak-to-peak amplitude 0.36mV,
          | P = 0.08494573d, M - m = 0.40P.
V0514 Gem | VB A (B 10.33m, 8", 358deg, 2012).
V0517 Gem | P1 is presented in the Table. P0 = 0.481358d; P1/P0 = 0.7452.
V0520 Gem | P1 is presented in the Table. P0 = 0.540394d; P1/P0 = 0.7468.
V1452 Her | P1 is presented in the Table. P0 = 0.547662d; P1/P0 = 0.7462.
V1457 Her | P1 is presented in the Table. P0 = 0.531662d; P1/P0 = 0.7465.
V1458 Her | The data for 1SWASP J161858.05+261303.5 data [82030] are combined measures for a
          | non-variable star (V = 13.2m) near the SuperWASP position and the real variable.
V1460 Her | Outside outburst, type EW with light elements Min = 2456560.640 + 0.2078522d x E,
          | V = 15.08m - 15.55m, MinII 15.45mV. Near outburst maximum, type EA with the depth
          | of MinI reaching 1.2mV and the depth of MinII of only about 0.1mV.
V1461 Her | P1 is presented in the Table. P0 = 0.559638d; P1/P0 = 0.7461.
V1466 Her | P1 is presented in the Table. P0 = 0.545187d; P1/P0 = 0.7460.
V1467 Her | Additional non-radial mode, P = 0.2737529d; P(Blazhko) = 112d.
V1468 Her | P1 is presented in the Table. P0 = 0.570831d; P1/P0 = 0.7459.
V1472 Her | P1 is presented in the Table. P0 = 0.506715d; P1/P0 = 0.7448.
V1473 Her | The NSVS data for ROTSE1 J164316.86+264815.8 are combined measurements for a
          | non-variable star (V = 12.4m) near the ROTSE position and the real variable.
V1474 Her | P1 is presented in the Table. P0 = 0.536720d; P1/P0 = 0.7464.
V1477 Her | P1 is presented in the Table. P0 = 0.532323d; P1/P0 = 0.7454.
V1478 Her | P1 is presented in the Table. P0 = 0.502498d; P1/P0 = 0.7443.
V1480 Her | P1 is presented in the Table. P0 = 0.473596d; P1/P0 = 0.7442.
V1481 Her | P1 is presented in the Table. P0 = 0.472265d; P1/P0 = 0.7441.
V1482 Her | P1 is presented in the Table. P0 = 0.532921d; P1/P0 = 0.7460.
V1483 Her | P1 is presented in the Table. P0 = 0.537739d; P1/P0 = 0.7460.
V1484 Her | P1 is presented in the Table. P0 = 0.530745d; P1/P0 = 0.7460.
V1486 Her | P1 is presented in the Table. P0 = 0.489858d; P1/P0 = 0.7447.
V1487 Her | The data for 1SWASP J165734.53+274827.7 in [82030] are combined measurements for a
          | non-variable star (V = 14.7m) near SuperWASP position and this variable (18"S).
V1488 Her | P1 is presented in the Table. P0 = 0.502028d; P1/P0 = 0.7459.
V1489 Her | P1 is presented in the Table. P0 = 0.550905d; P1/P0 = 0.7462.
V1490 Her | VB A (B 12.5mV, 16", 110deg, 2000).
V1491 Her | P1 is presented in the Table. P0 = 0.555957d; P1/P0 = 0.7456.
V1492 Her | P1 is presented in the Table. P0 = 0.478660d; P1/P0 = 0.7446.
V1499 Her | P1 is presented in the Table. P0 = 0.503175d; P1/P0 = 0.7457.
V1503 Her | Additional non-radial mode, P = 0.340686d; P(Blazhko) = 17.2d.
V1507 Her | P1 is presented in the Table. P0 = 0.480341d; P1/P0 = 0.7438.
V0621 Hya | P1 is presented in the Table. P0 = 0.467934d; P1/P0 = 0.7434.
V0623 Hya | P1 is presented in the Table. P0 = 0.545078d; P1/P0 = 0.7461.
V0624 Hya | P1 is presented in the Table. P0 = 0.528738d; P1/P0 = 0.7465.
V0627 Hya | Period varies.
V0635 Hya | P1 is presented in the Table. P0 = 0.558754d; P1/P0 = 0.7462.
V0638 Hya | The data for 1SWASP J090758.16-153811.8 in [82030] are combined measurements for the
          | a non-variable star (V = 13.6m) near the SuperWASP position and the real variable.
V0659 Hya | P1 is presented in the Table. P0 = 0.447456d; P1/P0 = 0.7412.
V0664 Hya | P1 is presented in the Table. P0 = 0.520738d; P1/P0 = 0.7461.
V0677 Hya | [Fe/H] = -1.16.
V0678 Hya | [Fe/H] = -1.37.
DS    Hyi | In the region of the SMC galaxy, probable non-member.
PS    Leo | P1 is presented in the Table. P0 = 0.509437d; P1/P0 = 0.7443.
PW    Leo | P1 is presented in the Table. P0 = 0.503529d; P1/P0 = 0.7454.
PX    Leo | P1 is presented in the Table. P0 = 0.521624d; P1/P0 = 0.7456.
PY    Leo | P1 is presented in the Table. P0 = 0.530969d; P1/P0 = 0.7455.
PZ    Leo | P1 is presented in the Table. P0 = 0.536083d; P1/P0 = 0.7462.
QQ    Leo | P1 is presented in the Table. P0 = 0.502380d; P1/P0 = 0.7456.
QR    Leo | P1 is presented in the Table. P0 = 0.561943d; P1/P0 = 0.7460.
QS    Leo | P1 is presented in the Table. P0 = 0.471002d; P1/P0 = 0.7440.
QU    Leo | P1 is presented in the Table. Additional non-radial mode, P = 0.359842d.
          | P0 = 0.490181d; P1/P0 = 0.7441.
QV    Leo | P1 is presented in the Table. P0 = 0.560076d; P1/P0 = 0.7455.
QY    Leo | P1 is presented in the Table. P0 = 0.469265d; P1/P0 = 0.7432.
V0335 Leo | P1 is presented in the Table. P0 = 0.481418d; P1/P0 = 0.7445.
V0338 Leo | P1 is presented in the Table. P0 = 0.553220d; P1/P0 = 0.7466.
V0340 Leo | P1 is presented in the Table. P0 = 0.489670d; P1/P0 = 0.7450.
V0342 Leo | VB A (B 11.9m, 35", 300deg, 2011).
V0343 Leo | P1 is presented in the Table. P0 = 0.465896d; P1/P0 = 0.7435.
V0344 Leo | P1 is presented in the Table. P0 = 0.533747d; P1/P0 = 0.7461.
V0345 Leo | P0 is presented in the Table. P1 = 0.358597d; P1/P0 = 0.7442.
V0350 Leo | P1 is presented in the Table. P0 = 0.547015d; P1/P0 = 0.7460.
V0351 Leo | P1 is presented in the Table. P0 = 0.472132d; P1/P0 = 0.7438.
AR    LMi | P1 is presented in the Table. P0 = 0.493881d; P1/P0 = 0.7448.
AV    LMi | P1 is presented in the Table. P0 = 0.547379d; P1/P0 = 0.7460.
AW    LMi | Additional non-radial mode, P = 0.3056288d; P(Blazhko) = 25d.
AX    LMi | P1 is presented in the Table. P0 = 0.487467d; P1/P0 = 0.7445.
AY    LMi | Additional non-radial mode, P = 0.313789d; P(Blazhko) = 13.4d.
AZ    LMi | P1 is presented in the Table. P0 = 0.571772d; P1/P0 = 0.7459.
BB    LMi | P1 is presented in the Table. P0 = 0.535953d; P1/P0 = 0.7463.
V0377 Lib | P1 is presented in the Table. P0 = 0.544401d; P1/P0 = 0.7455.
V0379 Lib | P1 is presented in the Table. P0 = 0.483137d; P1/P0 = 0.7447.
LV    Lyn | P0 is presented in the Table. P1 = 0.360108d; P1/P0 = 0.7460.
LW    Lyn | P1 is presented in the Table. P0 = 0.477799d; P1/P0 = 0.7442.
MM    Lyn | P1 is presented in the Table. P0 = 0.480261d; P1/P0 = 0.7442.
MQ    Lyn | Additional non-radial mode, P = 0.2534778d; P(Blazhko) = 22.7d.
MR    Lyn | P1 is presented in the Table. P0 = 0.485654d; P1/P0 = 0.7451.
MS    Lyn | Porb = 0.080d.
MT    Lyn | P1 is presented in the Table. P0 = 0.501434d; P1/P0 = 0.7447.
MV    Lyn | P1 is presented in the Table. P0 = 0.478181d; P1/P0 = 0.7442.
MW    Lyn | Period varies.
V1014 Mon | VB (A 9.52m, B 10.56m; AB 3", 194deg, 2001). The magnitude range in the Table is for combined brightness.
V0558 Nor | VB A (B 11.4m, 3", 183deg, 1933; C 11.4m, 6", 159deg, 1972).
V3673 Oph | Cluster non-member.
V3677 Oph | P = 72d is also possible.
V3694 Oph | Possible additional pulsation with P = 0.294286d.
V2834 Ori | P1 is presented in the Table. P0 = 0.488575d; P1/P0 = 0.7428.
V2846 Ori | According to [82044], a flare to 15.7mpg from 17.4 mpg was observed on 1996 November 17.
V2853 Ori | P1 is presented in the Table. P2 = 0.2653979d; P2/P1 = 0.7990.
V2855 Ori | Double-mode pulsator, P2 = 0.0448278d. VB A (B 5", 99deg, 1999).
V2856 Ori | MinII - MinI = 0.52P.
V1056 Per | VB A (B 6", 80deg, 2000; other companions). The magnitudes in
            the Table are for combined brightness; if corrected for
            neighbors, the approximate range is 11.75 - (12.4m*.
V1057 Per | Type ELL with a twice longer period is not excluded.
V1058 Per | O'Connell effect.
V1060 Per | VB A (B 6", 1deg, 1999).
V1066 Per | O'Connell effect.
V1078 Per | Multiperiodic. P0 is presented in the Table. P1 = 0.143832d.
LM    Psc | VB A (B 4", 305deg, 1997).
LO    Psc | VB A (B 12.2m, 5", 299deg, 2012).
LQ    Psc | VB A (B 10.5m, 5", 314deg; C 10.5m, 9", 57deg, 2015).
V0743 Pup | VB A (B 10", 211deg, 1999); magnitudes in the Table are for combined brightness.
          | P1 is presented in the Table. P2 = 0.328118d; P2/P1 = 0.8000.
V0751 Pup | VB A (B 12.8m, 0.6", 166deg, 2015).
V5860 Sgr | P0 is presented in the Table. P1 = 3.37986d; P1/P0 = 0.7009.
V5864 Sgr | Blended. P0 is presented in the Table. P1 = 0.832980d; P1/P0 = 0.7051.
V5867 Sgr | P = 215.3d is superposed.
V5874 Sgr | P = 161.7d is superposed.
V5875 Sgr | The depth of eclipses varies strongly.
V1679 Sco | P = 38.8d is superposed.
V1695 Sco | VB A (15.5mV; B 15.6mV, 9", 204deg, 1999).
V0637 Ser | P1 is presented in the Table. P0 = 0.541556d; P1/P0 = 0.7460.
V0638 Ser | Double-mode pulsations. P = 0.04191053d is superposed.
V0640 Ser | The data for 1SWASP J151652.90+004835.8 in [82030] are combined measurements for a
          | non-variable star (V = 14.3m) near the SuperWASP position and the real variable.
V0641 Ser | Type EB with a twice longer period is not excluded.
V0646 Ser | P1 is presented in the Table. P0 = 0.596277d; P1/P0 = 0.7450.
V0647 Ser | Double-mode pulsations. P = 0.042667 is superposed.
V0649 Ser | P1 is presented in the Table. P0 = 0.481733d; P1/P0 = 0.7438.
V0654 Ser | P1 is presented in the Table. P0 = 0.491922d; P1/P0 = 0.7456.
CW    Sex | P1 is presented in the Table. P0 = 0.475673d; P1/P0 = 0.7443.
CX    Sex | P1 is presented in the Table. P0 = 0.563212d; P1/P0 = 0.7459.
CY    Sex | P1 is presented in the Table. P0 = 0.488334d; P1/P0 = 0.7446.
DI    Tri | P1 is presented in the Table. P0 = 0.559708d; P1/P0 = 0.7459.
DK    Tri | VB B (A = GCVS NAME!!!; AB 14", 211deg, 2016).
DL    Tri | VB A (B = GCVSNAME!!!, 14", 211deg, 2016).
V0362 TrA | Several close companions.
EY    Tuc | In the region of the SMC galaxy, non-member.
V0441 UMa | VB A (B = V442 UMa, 2.0", 136deg, 2002). The range in the Table is for combined brightness.
V0442 UMa | VB B (A = V441 UMa; AB 2.0", 136deg, 2002). O'Connell effect.
V0448 UMa | P1 is presented in the Table. P0 = 0.481662d; P1/P0 = 0.7445.
V0452 UMa | VB A (A 14.0mV; B 15.7mV, 18", 233deg, 2000).
V0460 UMa | Distortion wave: P = 3.697d.
V0462 UMa | P1 is presented in the Table. P0 = 0.484580d; P1/P0 = 0.7441.
V0464 UMa | P1 is presented in the Table. P0 = 0.483830d; P1/P0 = 0.7450.
V0465 UMa | The mean brightness varies.
V0470 UMa | P1 is presented in the Table. P0 = 0.516157d; P1/P0 = 0.7464.
V0471 UMa | P1 is presented in the Table. P0 = 0.548171d; P1/P0 = 0.7455.
V0473 UMa | P1 is presented in the Table. P0 = 0.497336d; P1/P0 = 0.7456.
V0474 UMa | Double-mode pulsations. The other period is 0.0496142d.
V0475 UMa | P1 is presented in the Table. P0 = 0.557528d; P1/P0 = 0.7462. Additional non-radial mode, P = 0.433241d.
V0477 UMa | P1 is presented in the Table. P0 = 0.474709d; P1/P0 = 0.7440.
V0479 UMa | P1 is presented in the Table. P0 = 0.524939d; P1/P0 = 0.7463.
V0486 UMa | Type EW with a twice longer period is also possible.
V0497 UMa | Double-mode pulsations. For the P0 period, see the Table. P1 = 0.0526002d; P1/P0 = 0.77418.
V0498 UMa | Period varies?
BD    UMi | MinII - MinI = 0.544P.
BE    UMi | d = 0.05P. The mean brightness outside eclipses strongly varies. Quasi-periodic variations
          | outside eclipses with P1 = 0.0402525d, P2 = 0.0352080d and four other periods.
V0551 Vel | Multiperiodic.
V0674 Vir | P1 is presented in the Table. P0 = 0.485546d; P1/P0 = 0.7444.
V0675 Vir | P0 is presented in the Table. P1 = 0.347029d; P1/P0 = 0.7415.
V0679 Vir | P1 is presented in the Table. P0 = 0.481836d; P1/P0 = 0.7436.
V0680 Vir | P1 is presented in the Table. P0 = 0.496630d; P1/P0 = 0.7451.
V0681 Vir | P1 is presented in the Table. P0 = 0.494004d; P1/P0 = 0.7453.
V0684 Vir | P1 is presented in the Table. P0 = 0.478307d; P1/P0 = 0.7433.
V0685 Vir | P1 is presented in the Table. P0 = 0.495555d; P1/P0 = 0.7447.
V0686 Vir | P1 is presented in the Table. P0 = 0.494463d; P1/P0 = 0.7445.
V0691 Vir | P1 is presented in the Table. P0 = 0.539888d; P1/P0 = 0.7461.
V0693 Vir | The data for 1SWASP J130711.90+084159.9 in [82030] are combined measurements for a
          | non-variable star (V = 14.9m) near the SuperWASP position and the real variable.
V0694 Vir | P1 is presented in the Table. P0 = 0.464667d; P1/P0 = 0.7430.
V0696 Vir | P1 is presented in the Table. P0 = 0.469383d; P1/P0 = 0.7433.
V0698 Vir | P1 is presented in the Table. P0 = 0.516959d; P1/P0 = 0.7452.
V0699 Vir | P1 is presented in the Table. P0 = 0.559293d; P1/P0 = 0.7468.
V0703 Vir | P1 is presented in the Table. P0 = 0.476683d; P1/P0 = 0.7441.
V0704 Vir | P1 is presented in the Table. P0 = 0.476846d; P1/P0 = 0.7446.
V0705 Vir | P1 is presented in the Table. P0 = 0.477771d; P1/P0 = 0.7438.
V0707 Vir | P1 is presented in the Table. P0 = 0.486191d; P1/P0 = 0.7437.
V0708 Vir | P1 is presented in the Table. P0 = 0.483093d; P1/P0 = 0.7438.
V0711 Vir | P1 is presented in the Table. P0 = 0.545077d; P1/P0 = 0.7457.
V0723 Vir | Additional non-radial mode, P = 0.2702020d; P(Blazhko) = 10.7d.
V0730 Vir | Type EW with a twice longer period is also possible.
V0734 Vir | P1 is presented in the Table. P0 = 0.462283d; P1/P0 = 0.7428.
V0735 Vir | P1 is presented in the Table. P0 = 0.545647d; P1/P0 = 0.7468.
V0737 Vir | P1 is presented in the Table. P0 = 0.485785d; P1/P0 = 0.7439.
V0740 Vir | Period varies?
V0742 Vir | P1 is presented in the Table. P0 = 0.552328d; P1/P0 = 0.7459.
          | A close VB.
AO    Vol | A close VB.