V0395 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.472647d. P1/P0 = 0.74445.
V0398 Aps   According to [g0009], the star is a second-overtone pulsator.
V0401 Aps   P varies, the period in the Table is valid for 1990 - 1994.
V0403 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.477591d. P1/P0 = 0.744412.
V0404 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.480751d. P1/P0 = 0.74410.
V0405 Aps   Blazhko effect.
V0410 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.473375d. P1/P0 = 0.74416.
V0419 Aps   According to [g0010], the star is a second-overtone pulsator.
V0419 Aps   According to [g0009], the star is a second-overtone pulsator.
V0421 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.496065d. P1/P0 = 0.74449.
V0426 Aps   Blazhko effect?
V0431 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.48834d. P1/P0 = 0.74434.
V0432 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.474642d. P1/P0 = 0.74414.
V0440 Aps   The coordinates in the Table are uncertain.
V0444 Aps   The coordinates in the Table are uncertain.
V0445 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.480528d. P1/P0 = 0.74440.
V0446 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.486080d. P1/P0 = 0.74420.
V0447 Aps   According to [g0009], the star can be a double-mode pulsator with a low-amplitude fundamental mode.
V0448 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.473993d. P1/P0 = 0.74424.
V0449 Aps   The period in the Table is that of the first overtone (P1). P1 = 0.358943d is equally possible. The fundamental-mode period was not determined in [g0009].
V0454 Aps   The coordinates in the Table are uncertain.
V0458 Aps   According to [g0009], the star is a second-overtone pulsator.
V0461 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.477109d. P1/P0 = 0.74434.
V0463 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.480001d. P1/P0 = 0.74434.
V0466 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.474776d. P1/P0 = 0.74424.
V0469 Aps   Blended; the coordinates in the Table are uncertain.
V0470 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.493508d. P1/P0 = 0.74446.
V0483 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.485225d. P1/P0 = 0.74501.
V0488 Aps   The period in the Table is that of the first overtone (P1). Fundamental mode: P0 = 0.482485d. P1/P0 = 0.74431.
V0494 Aps   Cluster non-member?
V0496 Aps   P varies?
V0498 Aps   P varies?
V0504 Aps   P varies? [g0001].
V0384 Aqr   Blazhko effect?
V0387 Aqr   Blazhko effect?
V0398 Aqr   Blazhko effect?
V0399 Aqr   Blazhko effect.
V0409 Aqr   Blazhko effect?
V0413 Aqr   Blazhko effect.
V0425 Aqr   VB A (B sp). Blazhko effect?
V0427 Aqr   Field star? Blazhko effect? Another possible period: P = 0.746053d.
V0429 Aqr   Blazhko effect.
V0432 Aqr   P varies.
V0440 Aqr   Strong Blazhko effect [g0006]. P varies? [g0001].
V0457 Aqr   P varies, the light elements in the Table are for JD 2452433 - 2452445.
V0462 Aqr   P varies, the light elements in the Table are for JD 2452433 - 2452445.
V0477 Aqr   Period varies.
V1054 Ara   Cluster non-member.
V1055 Ara   Cluster non-member.
V1058 Ara   Cluster non-member.
V1059 Ara   Additional mode, P = 0.6285d [g0025].
V1060 Ara   Blazhko effect, P(Blazhko) = 57.710d [g0025].
V1060 Ara   Blazhko effect, P(Blazhko) = 35.2368d [g0025].
V1061 Ara   Cluster non-member. MinII - MinI = 0.26P.
V1063 Ara   Cluster non-member.
V1064 Ara   Cluster non-member.
V1065 Ara   Additional mode, P = 0.1707740d [g0025].
V1067 Ara   A second high-amplitude mode: P = 0.2509836d.
V1071 Ara   Blazhko effect, P(Blazhko) = 34.809d; additional period 216.34d [g0025].
V1072 Ara   A0 = 0.3771mV. P1 = 0.3266817d, A1 = 0.0275mV, P1/P0 = 0.7304 (abnormal ratio).
V1073 Ara   Blazhko effect, P(Blazhko) = 13.764d. Additional mode, P = 0.1897573d.
V1075 Ara   Cluster non-member.
V1077 Ara   Cluster non-member.
V1078 Ara   MinII - MinI = 0.75P.
V1080 Ara   Blazhko effect, P(Blazhko) = 82.267d [g0025].
V1083 Ara   Blazhko effect, P(Blazhko) = 66.917d [g0025].
V1084 Ara   A0 = 0.3089mV. P1 = 0.3596333d, A1 = 0.0177mV, P1/P0 = 0.7275 (abnormal ratio).
V1085 Ara   Blazhko effect, P(Blazhko) = 17.4043d [g0025].
V1088 Ara   Blazhko effect, P(Blazhko) = 41.191d [g0025].
V1090 Ara   Period varies.
V1092 Ara   Additional mode, P = 0.1688913d [g0025].
V1093 Ara   Blazhko effect, P(Blazhko) = 17.3010d [g0025].
V1094 Ara   Blazhko effect, P(Blazhko) = 73.332d [g0025].
V1095 Ara   Additional mode, P = 0.1715296d [g0025].
V1096 Ara   Cluster non-member.
V1097 Ara   Double-periodic Blazhko effect, P1(Blazhko) = 15.4504d, P2(Blazhko) = 13.771d.
V1100 Ara   Additional mode, P = 0.2002600d [g0025].
V1101 Ara   Additional mode, P = 0.1783040d [g0025].
V1103 Ara   Blazhko effect, P(Blazhko) = 56.190d [g0025].
V1105 Ara   Blazhko effect, P(Blazhko) = 78.036d [g0025].
V1108 Ara   Additional mode, P = 0.1730099d [g0025].
V1109 Ara   Cluster non-member.
V1113 Ara   Blazhko effect, P(Blazhko) = 8.52242d.
V1116 Ara   Additional modes, P = 0.1924287d, P = 0.1955796d, P = 0.1984818d [g0025].
V1117 Ara   Cluster non-member.
V1118 Ara   Additional modes, P = 0.187836d and 0.19332d.
V1119 Ara   According to [g0026], cluster non-member, in contradiction to Gaia DR2 proper motion.
V1121 Ara   Cluster non-member.
V1124 Ara   Cluster non-member.
V1126 Ara   Cluster non-member.
V1133 Ara   The Table presents the probable first-overtone period. P0 = 0.52d. Probable cluster non-member [g0023].
V1133 Ara   The suggested P0 gives P1/P0 = 0.66, not typical of first-overtone and fundamental-mode pulsators [g0001].
V1143 Ara   Chandra X-ray source.
V1144 Ara   Chandra X-ray source.
V1146 Ara   Optical counterepart of the millisecond pulsar PSR J1740-5340.