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Table 1

Observational properties of our sample.

Name Coordinates Host ESO ESO MJD Flux (J − Ks) Group 1.53 μm
(J2000) Period OBid notea [mag]b c featured
Cl* NGC 121 T V8 00:26:48.52 −71:32:50.5 SMC P89 723477 56 090.41 N 1.06 1
2MASS J00490032-7322238 00:49:00.33 −73:22:23.8 SMC P84 389528 55 110.07 N 1.50 2
2MASS J00493262-7317523 00:49:32.62 −73:17:52.3 SMC P84 389526 55 110.09 N 1.44 2
2MASS J00530765-7307477 00:53:07.65 −73:07:47.8 SMC P84 389511 55 116.12 N 1.43 2
2MASS J00542265-7301057 00:54:22.66 −73:01:05.7 SMC P84 389505 55 119.07 N 1.92 3
2MASS J00553091-7310186 00:55:30.91 −73:10:18.6 SMC P84 389503 55 119.09 N 2.11 3
2MASS J00563906-7304529 00:56:39.06 −73:04:53.0 SMC P84 389499 55 114.12 N 1.37 2
2MASS J00564478-7314347 00:56:44.78 −73:14:34.7 SMC P84 389497 55 119.11 N 1.77 3
2MASS J00570070-7307505 00:57:00.70 −73:07:50.6 SMC P84 389495 55 111.07 N 1.66 3
2MASS J00571214-7307045 00:57:12.15 −73:07:04.6 SMC P84 389493 55 111.08 N 1.53 2
2MASS J00571648-7310527 00:57:16.48 −73:10:52.8 SMC P84 389489 55 111.11 N 1.31 2
2MASS J01003150-7307237 01:00:31.51 −73:07:23.7 SMC P84 389481 55 111.12 N 1.33 2
Cl* NGC 419 LE 35 01:08:17.49 −72:53:01.3 SMC P90 804029 56 213.20 V 2.09 3
Cl* NGC 419 LE 27 01:08:20.67 −72:52:52.0 SMC P90 804024 56 213.18 V 1.98 3
T Cae 04:47:18.92 −36:12:33.5 MW P84 389 388 55 142.19 N/S 1.63 3
SHV 0500412-684054 05:00:29.71 −68:36:37.4 LMC P90 804254 56 213.29 1.84 3 Y
SHV 0502469-692418 05:02:28.86 −69:20:09.7 LMC P90 804257 56 213.31 1.98 3 Y
SHV 0504353-712622 05:03:55.96 −71:22:22.1 LMC P84 389445 55 119.26 N 2.17 3
SHV 0517337-725738 05:16:33.31 −72:54:32.1 LMC P90 804263 56 213.36 1.13 1
SHV 0518222-750327 05:16:49.73 −75:00:22.7 LMC P84 389433 55 142.28 N 2.52 4 Y
SHV 0518161-683543 05:18:02.47 −68:32:39.1 LMC P90 804266 56 234.29 N 1.16 1
SHV 0520505-705019 05:20:15.02 −70:47:26.1 LMC P84 389428 55 142.32 N 2.37 4 Y
SHV 0520427-693637 05:20:20.19 −69:33:44.8 LMC P90 804284 56 240.35 2.11 3
SHV 0528537-695119 05:28:27.73 −69:49:01.8 LMC P84 389414 55 226.19 V/N 3.23 4 Y
SHV 0525478-690944 05:25:28.21 −69:07:13.2 LMC P84 389421 55 142.36 N 3.02 4 Y
SHV 0527072-701238 05:26:37.82 −70:10:11.6 LMC P90 804300 56 261.34 2.55 4 Y
SHV 0536139-701604 05:35:42.81 −70:14:16.3 LMC P84 389406 55 226.23 N 3.12 4 Y
[ABC89] Pup 42 08:04:57.56 −29:51:25.5 MW P90 804003 56 292.25 2.30 4
IRAS 09484-6242 09:49:49.40 −62:56:09.0 MW P92 998 138 56 617.34 2.02 3
[W65] c2 11:22:05.06 −59:38:45.2 MW P90 804 322 56 320.35 1.71 3
[ABC89] Cir 18 13:55:26.20 −59:22:19.0 MW P89 814763 56 319.37 2.45 4
MW P91 929 000 56383.31 2.52 4
HE 1428-1950 14:30:59.39 −20:03:41.9 MW P91 929514 56 383.33 0.71 1
V CrAc 18:47:32.31 −38:09:32.3 MW P89 723829 56 144.17 – –
HD 202851 21:18:43.48 −01:32:03.3 MW P89 723822 56 144.31 N 0.83 1

Notes.

(a)

The letter indicates for which X-Shooter arm no absolute flux-calibration was possible: V=visible, N=near-infrared. The S letter indicates that the spectrum is saturated in the K-band.

(b)

The (J − Ks) colors are derived from the spectra using the 2MASS filters (Cohen et al. 2003), see Sect. 5.1.

(c)

The group sharing is discussed in Sect. 4.

(d)

The Y letter indicates the presence of the 1.53 μm absorption band (see Sect. 4).

(e)

See Appendix A for more details about V CrA.

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