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Table D.1

Candidate hot luminous stars in the census as selected by the criteria explained in Sect. 3. Stars are listed in order of increasing right ascension.

ID α δ V B − V Ref. VFTS HSH95 S99 P93 ST92 Sk
# (h m s) (°   ′   ′′) (mag) (mag)

1 05 36 51.12 − 69 05 12.20 16.63 0.67 W
2 05 36 53.82 − 69 04 30.13 17.00 0.32 W
3 05 36 55.98 − 69 07 36.70 17.36 0.61 W
4 05 36 56.85 − 69 05 59.36 17.98 0.68 W
5 05 36 57.18 − 69 08 47.40 15.85 0.04 W
6 05 36 57.22 − 69 07 23.33 18.33 0.80 W
7 05 36 57.26 − 69 05 00.01 15.11 0.69 W
8 05 36 57.62 − 69 03 44.04 14.56 0.61 W
9 05 36 58.95 − 69 08 21.66 15.33 0.01 W
10 05 37 03.59 − 69 10 22.32 16.71 0.32 W
11 05 37 03.91 − 69 10 03.60 13.01 0.20 Z
12 05 37 04.01 − 69 08 23.83 14.36 0.80 W
13 05 37 04.26 − 69 08 05.46 16.18 0.11 W 009
14 05 37 04.47 − 69 04 00.08 15.56 0.20 W
15 05 37 05.63 − 69 09 12.20 15.83 0.15 W 012
16 05 37 06.29 − 69 04 41.20 16.36 0.13 W 013
17 05 37 08.72 − 69 04 45.51 17.36 0.47 W
18 05 37 08.88 − 69 07 20.39 13.55 0.04 Z 016
19 05 37 09.68 − 69 02 21.39 15.88 −0.02 W
20 05 37 10.17 − 69 05 24.10 17.29 0.37 W

Notes. The first 20 candidate stars are given here, see online data for full census. References for the photometry are as follows: dM – De Marchi et al. (2011); S – Selman; W – WFI; P – Parker; C – CTIO; Z – Zaritsky et al. (2004) and Wal – Walborn et al. (1999). Popular aliases are also included from the following catalogues: VFTS – Paper I; HSH95 – Hunter et al. (1995); S99 – Selman et al. (1999); P93 – Parker (1993); ST92 – Schild & Testor (1992) and Sk – Sanduleak (1970) catalogues.

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