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Table 2
Stars showing close, unresolved peaks near f0 that were marked as PC.
ID | PPuls [d] | Pm [d] | S/N | N | TS [d] | Rem |
|
||||||
DI Aps | 0.519187(6) | 2700(300) | 7.7 | 509 | 3212 | |
ASAS J204705-0919.2 | 0.508809(6) | 2500(200) | 6.7 | 369 | 3146 | + |
ASAS J083815-6025.9 | 0.465751(5) | 2400(400) | 5.9 | 550 | 3293 | b |
QZ Cen | 0.502052(6) | 2200(200) | 6.1 | 634 | 3188 | b |
V0584 Cen | 0.459032(2) | 3200(600) | 5.0 | 418 | 3153 | |
RS Crv | 0.536834(6) | 2200(200) | 6.0 | 727 | 3169 | |
BK Eri | 0.548148(4) | 1900(100) | 4.9 | 363 | 3243 | + |
SV Eri | 0.713861(4) | 2800(100) | 10.0 | 536 | 3296 | |
NSV 14009 | 0.563985(6) | 3000(200) | 6.4 | 585 | 3256 | |
ASAS J054843-1627.0* | 0.376709(4) | 3000(200) | 7.9 | 544 | 3299 | b |
PS Lup | 0.471878(2) | 3200(400) | 5.7 | 663 | 3191 | + |
V0898 Mon | 0.541493(12) | 2200(200) | 5.0 | 316 | 3078 | b |
ASAS J160612-4319.2 | 0.356944(2) | 2800(200) | 8.0 | 639 | 3194 | b |
ASAS J165834-8458.6 | 0.549312(6) | 3200(500) | 5.1 | 561 | 3241 | |
V0455 Oph | 0.453893(2) | 2200(400) | 3.6 | 377 | 2586 | b |
KV Pav | 0.527929(6) | 4000(600) | 6.9 | 528 | 3289 | |
V0338 Pav | 0.530827(6) | 2600(400) | 4.4 | 330 | 3273 | b |
ASAS J075127-4136.3 | 0.335716(2) | 3000(300) | 6.8 | 610 | 3296 | b |
V0687 Pup | 0.575194(8) | 2500(300) | 5.8 | 483 | 3246 | b |
ASAS J200147-2153.8 | 0.546631(14) | 2500(400) | 4.3 | 562 | 3144 | b |
ASAS J190713-5205.7 | 0.526724(2) | 3100(600) | 4.0 | 725 | 3173 | |
GR Tel | 0.611916(4) | 2900(400) | 4.9 | 696 | 3134 | b |
Notes. The notation of the columns is the same as in Table 1. The star with “*” is known to the literature as a BL star. Blended stars are marked with “b” and stars with additional peaks are marked with “+” in the column Rem.
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