Figure 1: HD 32918 = YY Men V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2444155.64 + 9.5476 
E (Collier 1982a)
Figure 2: HD 36705 = AB Dor V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2444296.575 + 0.51423 E (Pakull 1981)
Figure 3: HD 37847 = TW Lep V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2444155.64 + 28.22 E (Henry et al. 1982)
Figure 4: HD 39917 = SZ Pic V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2443931.54 + 4.905 E
Figure 5: HD 61245 = V 344 Pup V-band light curve and
colors. Phases are reckoned from the spectroscopic ephemeris
24448331.5 + 11.761 E (Balona 1987)
Figure 6: HD 81410 = IL Hya V-band light curve and colors.
Phases are reckoned from the spectroscopic ephemeris
2441466.213 + 12.86833 E (Raveendran et al. 1982)
Figure 7: HD 81410 = IL Hya V-band long-term variability.
The vertical bars indicate the peak-to-peak amplitude of the light curve
Figure 8: HD 82558 = LQ Hya V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2445275.64 + 1.5978 E (Strassmeier & Hall 1988)
Figure 9: HD 98712 = SZ Crt V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2448331.5.5 + 11.58 E (Torres et al. 1985)
Figure 10: HD 101309 = V 829 Cen V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2448331.5 + 11.65 E (Cutispoto 1993)
Figure 11: HD 101309 = V 829 Cen V-band long-term
variability. The vertical bars indicate the peak-to-peak amplitude of
the light curve
Figure 12: HD 102077 = V 838 Cen V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2448331.5 + 1.847 E
Figure 13: HD 106225 = HU Vir V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2448331.5 + 10.353 E (Strassmeier et al. 1997)
Figure 14: HD 119285 = V 851 Cen V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2448331.5 + 12.05 E (Lloyd Evans & Koen 1987)
Figure 15: HD 119285 = V 851 Cen V-band long-term
variability. The vertical bars indicate the peak-to-peak amplitude of
the light curve
Figure 16: HD 127535 = V 841 Cen V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2445804.1 + 5.929 E (Cutispoto 1990). The flares data are represented
by the symbol (
)
Figure 17: HD 127535 = V 841 Cen V light long-term
variability. The vertical bars indicate the peak-to-peak amplitude of
the light curve
Figure 18: HD 136905 = GX Lib V-band light curve and
colors. Phases are reckoned from the spectroscopic ephemeris
2445061.901 + 11.13448 E (Kaye et al. 1995)
Figure 19: HD 136905 = GX Lib V-band long-term variability.
The vertical bars indicate the peak-to-peak amplitude of the light curve
Figure 20: HD 139084 = V 343 Nor V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2448331.5 + 4.24 E
Figure 21: HD 155555 = V 824 Ara V-band light curve and
colors. Phases are reckoned from the photometric ephemeris
2448331.5 + 1.694 E
Figure 22: HD 174429 = PZ Tel V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2448331.5 + 0.9447 E
Figure 23: HD 197481 = AU Mic V-band light curve and colors.
Phases are reckoned from the photometric ephemeris
2448331.5 + 4.865 E (Torres et al. 1972)
Figure 24: HD 197481 = AU Mic V-band long-term variability.
The vertical bars indicate the peak-to-peak amplitude of the light curve