Table 1: Point source fluxes.

ID		     2MASS designation         Spitzer fluxes and uncertaintiesa         SCUBA peakb
  RA Dec J, H & $K_{\rm s}$ bands 3.6 $\mu $m $\sigma_{3.6}$ 4.5 $\mu $m $\sigma_{4.5}$ 5.8 $\mu $m $\sigma_{5.8}$ 8.0 $\mu $m $\sigma_{8.0}$ 24 $\mu $m $\sigma_{24}$ 70 $\mu $mc $\sigma_{70}$ sub-millimeter
  (J2000) (J2000)   (mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (Jy) (Jy)  
S1 19$^{\rm h}$21$^{\rm m}$50 $\hbox{$.\!\!^{\rm s}$ }$1 +13$^\circ$47 $\hbox{$^\prime$ }$57 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 <0.500 0.250 <2.000 1.000 <2.000 1.000 26.647 3.033 - - -
S2 19$^{\rm h}$21$^{\rm m}$50 $\hbox{$.\!\!^{\rm s}$ }$2 +13$^\circ$48 $\hbox{$^\prime$ }$19 $\hbox{$^{\prime\prime}$ }$ 19215022+1348185 2.994 0.518 6.248 0.854 8.012 1.115 3.862 1.107 101.585 7.051 - - P3
S3 19$^{\rm h}$21$^{\rm m}$53 $\hbox{$.\!\!^{\rm s}$ }$0 +13$^\circ$48 $\hbox{$^\prime$ }$19 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 <0.500 0.250 <2.000 1.000 <2.000 1.000 23.254 2.999 - - -
S4 19$^{\rm h}$21$^{\rm m}$34 $\hbox{$.\!\!^{\rm s}$ }$4 +13$^\circ$49 $\hbox{$^\prime$ }$12 $\hbox{$^{\prime\prime}$ }$ 19213444+1349122 234.100 8.137 161.000 6.024 148.499 10.147 75.078 5.725 32.944 2.963 - - -
S5 19$^{\rm h}$21$^{\rm m}$49 $\hbox{$.\!\!^{\rm s}$ }$6 +13$^\circ$49 $\hbox{$^\prime$ }$31 $\hbox{$^{\prime\prime}$ }$ - 3.741 0.622 4.808 0.720 29.020 2.581 58.549 4.542 109.226 7.936 2.4 1.4 part of P1
S6 19$^{\rm h}$21$^{\rm m}$50 $\hbox{$.\!\!^{\rm s}$ }$2 +13$^\circ$49 $\hbox{$^\prime$ }$39 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 4.237 0.682 8.802 1.291 4.214 1.213 295.503 16.843 4.5 1.4 part of P1
S7 19$^{\rm h}$21$^{\rm m}$40 $\hbox{$.\!\!^{\rm s}$ }$7 +13$^\circ$51 $\hbox{$^\prime$ }$17 $\hbox{$^{\prime\prime}$ }$ 19214073+1351176 1.233 0.314 1.581 0.352 <2.000 1.000 <2.000 1.000 90.409 6.485 - - -
S8 19$^{\rm h}$21$^{\rm m}$37 $\hbox{$.\!\!^{\rm s}$ }$3 +13$^\circ$51 $\hbox{$^\prime$ }$23 $\hbox{$^{\prime\prime}$ }$ 19213739+1351238 4.448 0.662 9.188 1.140 9.272 1.200 13.316 1.768 31.222 2.877 - - -
S9 19$^{\rm h}$21$^{\rm m}$35 $\hbox{$.\!\!^{\rm s}$ }$9 +13$^\circ$52 $\hbox{$^\prime$ }$01 $\hbox{$^{\prime\prime}$ }$ 19213593+1352007 4.001 0.653 3.637 0.609 4.461 0.779 9.529 1.468 87.157 6.167 - - -
S10 19$^{\rm h}$21$^{\rm m}$52 $\hbox{$.\!\!^{\rm s}$ }$1 +13$^\circ$52 $\hbox{$^\prime$ }$24 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 0.639 0.196 <2.000 1.000 <2.000 1.000 67.752 5.307 - - -
S11 19$^{\rm h}$21$^{\rm m}$36 $\hbox{$.\!\!^{\rm s}$ }$2 +13$^\circ$52 $\hbox{$^\prime$ }$21 $\hbox{$^{\prime\prime}$ }$ - 0.201 0.122 1.109 0.293 1.206 0.429 1.988 0.959 24.073 2.446 - - -
S12 19$^{\rm h}$21$^{\rm m}$45 $\hbox{$.\!\!^{\rm s}$ }$6 +13$^\circ$49 $\hbox{$^\prime$ }$21 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 0.260 0.133 <2.000 1.000 <2.000 1.000 13.778 2.018 - - EP
S13 19$^{\rm h}$21$^{\rm m}$40 $\hbox{$.\!\!^{\rm s}$ }$7 +13$^\circ$50 $\hbox{$^\prime$ }$55 $\hbox{$^{\prime\prime}$ }$ 19214066+1350547 4.342 0.695 4.106 0.659 2.650 0.578 <2.000 1.000 16.289 2.513 - - -
S14 19$^{\rm h}$21$^{\rm m}$42 $\hbox{$.\!\!^{\rm s}$ }$3 +13$^\circ$50 $\hbox{$^\prime$ }$21 $\hbox{$^{\prime\prime}$ }$ 19214228+1350212 3.269 0.589 2.934 0.526 3.189 0.594 3.125 0.746 7.466 1.673 - - -
S15 19$^{\rm h}$21$^{\rm m}$47 $\hbox{$.\!\!^{\rm s}$ }$9 +13$^\circ$49 $\hbox{$^\prime$ }$20 $\hbox{$^{\prime\prime}$ }$ - <0.500 0.250 0.726 0.222 <2.000 1.000 <2.000 1.000 2.757 0.918 - - P2
S16 19$^{\rm h}$21$^{\rm m}$50 $\hbox{$.\!\!^{\rm s}$ }$5 +13$^\circ$47 $\hbox{$^\prime$ }$28 $\hbox{$^{\prime\prime}$ }$ - 3.303 1.331 2.624 1.304 6.388 0.908 2.290 0.687 5.544 1.381 - - -
S17 19$^{\rm h}$21$^{\rm m}$48 $\hbox{$.\!\!^{\rm s}$ }$7 +13$^\circ$51 $\hbox{$^\prime$ }$02 $\hbox{$^{\prime\prime}$ }$ 19214875+1351034 212.300 7.346 111.500 4.275 81.086 6.043 41.064 3.503 7.142 1.262 - - -
S18 19$^{\rm h}$21$^{\rm m}$48 $\hbox{$.\!\!^{\rm s}$ }$1 +13$^\circ$51 $\hbox{$^\prime$ }$24 $\hbox{$^{\prime\prime}$ }$ 19214807+1351249 436.200 18.300 240.600 14.500 87.205 6.401 87.228 6.439 13.605 1.598 - - -
S19 19$^{\rm h}$21$^{\rm m}$49 $\hbox{$.\!\!^{\rm s}$ }$4 +13$^\circ$51 $\hbox{$^\prime$ }$58 $\hbox{$^{\prime\prime}$ }$ 19214945+1351581 416.400 18.690 233.300 9.739 69.551 5.225 88.545 6.542 12.832 1.589 - - -
S20 19$^{\rm h}$21$^{\rm m}$40 $\hbox{$.\!\!^{\rm s}$ }$8 +13$^\circ$52 $\hbox{$^\prime$ }$36 $\hbox{$^{\prime\prime}$ }$ - 14.478 1.442 14.110 1.531 12.216 1.410 6.380 1.035 22.614 2.258 - - -
a A ``<'' sign indicates that the corresponding flux value is an upper limit. The IRAC 3.6 $\mu $m and 4.5 $\mu $m fluxes and uncertainties for S4, S17 and S18 are taken from GLIMPSE.
b Sub-millimeter peaks P1, P2 and EP are listed in Table 3 of Ormel et al. (2005). See text in Sect. 3.2.1 for details of P1's subdivision. P3 is not defined in Ormel et al. (2005), its flux at 450 $\mu $m is estimated in Sect. 3.2.1 of the present study.
c The MIPSGAL mosaic shows one emission core of 6.9 Jy at the position of S5 and S6. See Sect. 3.2.1 for details of the subdivision of the MIPS 70 $\mu $m flux and Sect. 2.3 for the upper limit used for other sources.

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