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Table 1:

Targets of the present observations.

Number
ID Obs. ID Obs. Date RA[J2000] Dec[J2000] Reference
ST1 IRAS 05400-7013 5126560 2008 Apr. 12 05:39:31.15 -70:12:16.8 1, 2
ST2 NGC 1936 5126562 2008 May 25 05:22:12.56 -67:58:32.2 1
ST3 ......a 3410003 2008 Dec. 11 05:25:46.69 -66:14:11.3 1, 3
ST4 IRAS F05148-6715 3410004 2008 Dec. 27 05:14:49.41 -67:12:21.5 1, 3
ST5 IRAS 05311-6836 5126561 2008 May 11 05:30:54.27 -68:34:28.2 1, 2
ST6 05394112-6929166b 5126563 2008 Apr. 19 05:39:41.08 -69:29:16.8 1
ST7 IRAS 05240-6809 5126567 2008 May 23 05:23:51.15 -68:07:12.2 1, 3
ST8 MSX LMC 1786 5126573 2008 May 2 05:37:28.17 -69:08:47.0 3, 4, 5, 6
ST9 IRAS 05237-6755 5126568 2008 May 26 05:23:35.53 -67:52:35.5 2, 4
ST10 MSX LMC 1229 5200384 2008 Dec. 21 04:56:40.80 -66:32:30.4 2, 4, 5
ST11 IRAS05270-6851 5126571 2008 May 11 05:26:46.63 -68:48:47.1 2, 5
ST12 IRAS 05328-6827 5126566 2008 May 12 05:32:38.59 -68:25:22.2 3, 6

Notes. (a) The source is in a cluster; (b) 2MASS ID.

References. (1) Shimonishi et al. (2008); (2) Seale et al. (2009); (3) Oliveira et al. (2009); (4) Whitney et al. (2008); (5) Gruendl & Chu (2009); (6) van Loon et al. (2010a).


Source LaTeX | All tables | In the text

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