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Table 1:

YSO candidates projected onto the infrared extended sources B and C (near RA, Dec(J2000) = [13$^{\rm h}$34$^{\rm m}$30$^{\rm s}$, -62$^\circ $25$^\prime $]).
$\char93 $ l[h m s] b[ $^\circ\ \hbox{$^\prime$ }\ \hbox{$^{\prime\prime}$ }$] IRAS source Fluxes[Jy]     Class.
        12 $\mu $m 25 $\mu $m 60 $\mu $m 100 $\mu $m      
1 13 34 11.4 -62 27 03 13307-6211 0.8 2.0 20.5 85.4     YSO/Class 0
$\char93 $ l[h m s] b[ $^\circ\ \hbox{$^\prime$ }\ \hbox{$^{\prime\prime}$ }$] MSX source Fluxes[Jy]      
        $\mu $m 12 $\mu $m 14 $\mu $m 21 $\mu $m     Class.
2 13 34 13.0 -62 25 07 G307.8603+00.0439 0.2261 1.809 1.118 1.391     CH  II, HD 117797
3 13 35 03.6 -62 25 77 G307.9563+00.0163 0.7808 0.7287 0.5542 3.093     CH  II
4 13 34 10.2 -62 25 00 G307.8561+00.0463 0.2149 1.144 2.191 4.793     MYSO, HD 117797
5 13 34 13.8 -62 25 29 G307.8620+00.0399 0.1614 1.146 1.726 4.996     MYSO
$\char93 $ l[h m s] b[ $^\circ \ \hbox{$^\prime$ }$] GLIMPSE source Fluxes[mag]  
        H $K_{\rm s}$ [3.6] [4.5] [5.8] [8.0] Class.
6 13 34 14.4384 -62 26.5794 G307.8597+00.0185 13.244 11.95 11.237 11.137 10.873 10.895 II
7 13 34 17.9136 -62 25.9506 G307.8680+00.0277 12.459 11.257 10.338 10.419 10.242 10.243 II
8 13 34 19.4304 -62 25.506 G307.8721+00.0345 11.202 9.599 7.489 7.385 6.928 6.641 I-II
9 13 34 21.564 -62 26.6934 G307.8729+00.0143 13.959 12.913 12.267 12.144 12.116 11.853 II
10 13 34 47.6856 -62 26.9472 G307.9219+00.0018 13.37 12.553 11.859 11.738 11.713 11.68 II
11 13 34 48.9096 -62 25.4874 G307.9283+00.0254 14.267 12.681 11.796 11.655 11.204 11.654 II
12 13 34 50.1048 -62 25.6944 G307.9300+00.0216 13.767 12.546 11.785 11.7 11.347 11.414 II
13 13 34 54.0384 -62 26.2866 G307.9358+00.0106 12.596 11.773 11.018 10.92 10.938 10.933 II
14 13 34 54.8448 -62 25.3746 G307.9399+00.0253 13.319 12.117 11.293 11.152 10.792 10.611 I-II
15 13 34 56.6544 -62 25.7538 G307.9422+00.0185 14.487 12.589 11.331 10.94 10.732 10.827 II
16 13 34 58.644 -62 26.6052 G307.9436+00.0039 13.376 12.672 12.142 11.819 11.508 11.403 I-II
17 13 35 0.6672 -62 25.641 G307.9502+00.0190 11.013 9.211 8.089 7.925 7.462 7.366 I-II
18 13 35 0.8784 -62 26.061 G307.9494+00.0121 13.54 12.424 11.79 11.598 11.264 11.535 II
19 13 35 4.7112 -62 25.1676 G307.9592+00.0255 13.87 12.348 11.382 11.22 10.892 10.994 II
20 13 35 5.0928 -62 24.3822 G307.9621+00.0383 14.298 13.186 12.453 12.352 12.217 12.064 II
21 13 35 5.5032 -62 26.2302 G307.9577+00.0078 12.143 10.783 9.836 9.826 9.511 9.568 II
22 13 35 7.9968 -62 25.6524 G307.9641+00.0165 14.241 12.207 10.879 10.721 10.298 10.135 I-II


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