Table C.2.
New eclipsing binaries identified with ASTEP South and known objects with improved classification and parameters.
| ID | RA | Dec | fmag | Period | T0 | Depth | Type |
|---|---|---|---|---|---|---|---|
| (UCAC3) | (J2000) | (J2000) | (mag) | (d) | (BJD) | (mmag) | |
| 003-001765a | 06:53:22.343 | −88:34:04.28 | 10.04 | 0.4574110 (48) | 4627.4151 (34) | 2.6 (0.4) | EB |
| 002-002671 | 16:04:20.122 | −89:00:40.74 | 10.99 | 13.4892 (25) | 4627.70 (13) | 5.7 (0.4) | EB |
| 002-003763 | 23:23:51.240 | −89:25:17.62 | 11.25 | 23.3853 (53) | 4636.35 (18) | 8.6 (0.4) | EB |
| 004-006956 | 18:03:31.003 | −88:16:36.79 | 11.86 | 36.263 (24) | 4634.18 (23) | 5.9 (0.4) | EB |
| 004-000272b | 00:45:26.547 | −88:25:21.03 | 11.98 | 34.559 (19) | 4627.69 (19) | 15.0 (0.7) | EB |
| 001-000823c | 14:50:14.729 | −89:46:58.96 | 12.18 | 0.28891080 (20) | 4627.2346 (02) | 479 (8) | EW |
| 001-000701 | 12:41:48.571 | −89:42:30.30 | 12.69 | 54.133 (15) | 4668.37 (20) | 38 (2) | EB |
| 002-003056d | 18:36:30.712 | −89:11:02.84 | 12.76 | 75.57626 (20) | 4629.9895 (60) | 30 (2) | EA |
| 001-001090 | 20:37:01.418 | −89:44:34.88 | 12.82 | 23.7052 (70) | 4632.38 (10) | 10 (1) | EW |
| 001-000120 | 02:26:38.190 | −89:31:31.72 | 14.45 | 81.051070 (20) | 5058.9223 (24) | 335 (5) | EA |
| 001-000682 | 12:27:06.862 | −89:48:58.91 | 14.59 | 1.048938 (30) | 4627.2738 (97) | 28.0 (0.8) | EB |
Notes. The ID, coordinates, and magnitudes fmag are extracted from the UCAC3 catalog. For each object, we report the period, the mid-eclipse date of the first detected eclipse, the depth of the primary eclipse (or of the secondary eclipse in the potential case of eccentric binaries with no primary eclipses), and the type of eclipsing binary. Numbers in parentheses indicate the 3σ uncertainties on the last two digits for the periods and ephemerides, and the 3σ uncertainties for the depths.
This object was reported as a rotating ellipsoidal variable by Wang et al. (2015).
This object was reported as a variable of unknown type by Wang et al. (2011) and was not identified by Wang et al. (2013).
This object is EN Oct: we improved its period and eclipse depth compared to previous studies by Knigge & Bauernfeind (1967); Otero (2004).
This object is discussed in Sect. 7.2.5.
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