1 Variable in NSVS data.
 2 P=55.6d (from NSVS data).
 3 A twice shorter period and type RRC are possible.
 4 P=39.7d (NSVS data).
 5 A small-amplitude variable in NSVS data.
 6 P=60d (NSVS data).
 7 P~50d (NSVS data) is possible.
 8 A twice longer period is possible.
 9 A twice longer period and type EW are possible.
10 P~51d (NSVS data) is possible.
11 A CCD study following this discovery was announced in 
11  Antipin et al. (2007PZ.....27....8A).
12 A white or yellow star, J-H=0.529 (2MASS).
13 P~62d (NSVS data) is possible.
14 NSVS data show variations with the same period.
15 1-day aliases of a twice shorter period are strong.
16 P=45d (NSVS data).
17 Variable in ASAS-3 data, not included into the ASAS-3 catalog of 
17  variable stars.
18 Not identical to V568 Oph (17:59:44.09, +4:59:55.6, J2000).
19 1-day aliases (0.399278d and 0.285235d) are also quite possible.
20 The periods 83.8d or 92.5d are possible (NSVS data).
21 A double star.
22 P~63.5d (NSVS data) is possible.
23 P=75d (NSVS data).
24 The period 0.286864d (type EW) is also quite possible.
25 O'Connell effect.
26 A 1-day alias, P=0.49813d, is possible.
27 P~78d (NSVS data) is possible.
28 P~150d (NSVS data) is possible.
29 P~130d (NSVS data) is possible.
30 A twice shorter period and type HADS are possible.
31 P=58d (NSVS data).
32 P=48d (NSVS data).
33 P=62d (NSVS data).
34 P=0.305252d is also possible.
35 P~250d (NSVS data) is possible.
36 P~60d (NSVS data) is possible.
37 P~54d (NSVS data) is possible.
38 P~85d (NSVS data) is possible.
39 A 1-day alias, P=0.397451d, is possible.
40 A twice shorter period and type RRAB are possible.
41 The coordinates are from the USNO-A2.0 catalog.
42 P=81d (NSVS data).
43 Possibly, the minima are deeper.
44 P~82d (NSVS data) is possible.
45 A 1-day alias, P=0.081429d, is possible.