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Table 2:

Multiwavelength results for the intermediate-mass YSOs in the star-forming region IRAS 00117+6412.

Wavelength
  Beam PA rms $I_\nu^{\rm peak}$a $S_\nu$a Deconv. size PA
(cm) Instrument ( $\hbox{$^{\prime\prime}$ }\times\hbox{$^{\prime\prime}$ }$) ( $\hbox{$^\circ$ }$) ($\mu$Jy beam-1) (mJy beam-1) (mJy) ( $\hbox{$^{\prime\prime}$ }\times\hbox{$^{\prime\prime}$ }$) ( $\hbox{$^\circ$ }$)

UCH II region
$\alpha(J2000.0)=00^{\rm h}14^{\rm m}28\hbox{$.\!\!^{\rm s}$ }23$b            
  $\delta(J2000.0)=+64\hbox{$^\circ$ }28\hbox{$^\prime$ }46\hbox{$.\!\!^{\prime\prime}$ }6$b            

6.0
VLA-C $5.2\times4.0$ -4 30 $1.21\pm0.03$ $\phantom{0}1.72\pm0.08$ $3.1\pm0.5\times2.7\pm0.4$ $95\pm50$
3.6 VLA-CD $3.8\times3.7$ +45 30 $1.03\pm0.03$ $\phantom{0}1.88\pm0.09$ $3.7\pm0.4\times3.1\pm0.4$ $10\pm60$
3.6 VLA-BCD $1.9\times1.7$ -70 50 $0.43\pm0.05$ $\phantom{0}1.62\pm0.16$ $3.9\pm0.4\times3.7\pm0.4$ $180\pm60$
1.3c VLA-D $5.9\times4.5$ -21 70 $0.59\pm0.07$ $\phantom{0}1.7\pm0.2$ $5.9\pm1.8\times5\pm2$ $120\pm50$
0.7 VLA-D $4.0\times3.0$ +64 170 $1.35\pm0.17$ $1.4\pm0.3$ $2.7\pm1.2\times0.0$ $150\pm30$
0.32 PdBI-CD $4.3\times3.4$ +61 180 ... <1 ... ...
0.13 SMA-comp $3.2\times2.0$ +45 600 ... <4 ... ...
0.12d PdBI-CD $1.5\times1.2$ +58 1000 ... <25 ... ...

MM1
$\alpha(J2000.0)=00^{\rm h}14^{\rm m}26\hbox{$.\!\!^{\rm s}$ }05$b            
  $\delta(J2000.0)=+64\hbox{$^\circ$ }28\hbox{$^\prime$ }43\hbox{$.\!\!^{\prime\prime}$ }7$b            

6.0
VLA-C $5.2\times4.0$ -4 30 ... <0.12 ... ...
3.6 VLA-CD $3.8\times3.7$ +45 30 $0.14\pm0.03$ $0.17\pm0.07$ $6.4\pm3.0\times3\pm2$ $120\pm30$
3.6 VLA-BCD $1.9\times1.7$ -70 50 $0.21\pm0.05$ $0.15\pm0.06$ $4.0\pm1.5\times2.2\pm1.5$ $160\pm50$
1.3 VLA-D $5.9\times4.5$ -21 70 ... <0.27 ... ...
0.7 VLA-D $4.0\times3.0$ +64 170 ... <0.69 ... ...
0.32 PdBI-CD $4.3\times3.4$ +61 180 $4.16\pm0.19$ $5.1\pm0.9$ $3.2\pm0.4\times0.0$ $75\pm10$
0.13 SMA-comp $3.2\times2.0$ +45 600 $51\pm1$ $71\pm14$ $2.4\pm0.3\times1.0\pm0.2$ $50\pm10$
0.12d PdBI-CD $1.5\times1.2$ +58 1000 $21\pm1$ $65\pm10$ $2.9\pm0.4\times1.6\pm0.4$ $25\pm10$

MM2
$\alpha(J2000.0)=00^{\rm h}14^{\rm m}26\hbox{$.\!\!^{\rm s}$ }31$b            
  $\delta(J2000.0)=+64\hbox{$^\circ$ }28\hbox{$^\prime$ }27\hbox{$.\!\!^{\prime\prime}$ }8$b            

6.0
VLA-C $5.2\times4.0$ -4 30 ... <0.12 ... ...
3.6 VLA-CD $3.8\times3.7$ +45 30 ... <0.12 ... ...
3.6 VLA-BCD $1.9\times1.7$ -70 50 ... <0.21 ... ...
1.3 VLA-D $5.9\times4.5$ -21 70 ... <0.27 ... ...
0.7 VLA-D $4.0\times3.0$ +64 170 ... <0.69 ... ...
0.32 PdBI-CD $4.3\times3.4$ +61 180 $2.8\pm0.2$ $3.2\pm0.6$ $1.6\pm1.0\times1.0\pm1.5$ $160\pm50$
0.13 SMA-comp $3.2\times2.0$ +45 600 $19\pm1$ $24\pm5$ $2.0\pm0.5\times0.0$ $170\pm20$
0.12d PdBI-CD $1.5\times1.2$ +58 1000 $20\pm5$ $50\pm13$ $3.5\pm1.0\times1.1\pm0.8$ $140\pm30$

Notes. (a) Primary beam corrected (mainly affecting the millimeter data). In case of non-detection at one of the frequencies, an upper limit of 4$\sigma$ was used. Error in intensity is $1\sigma$. Error in flux density has been calculated as $\sqrt{(\sigma\sqrt{\theta_{\rm source}/\theta_{\rm beam}})^{2}+(\sigma_{\rm flux-scale})^{2}}$, where $\sigma$ is the rms noise level of the map, $\theta_{\rm source}$and $\theta_{\rm beam}$ are the size of the source and the beam respectively, and $\sigma_{\rm flux-scale}$is the error in the flux scale, which takes into account the uncertainty on the calibration applied to the flux density of the source ( $S_\nu\times\%_{\rm uncertainty}$).(b) Coordinates for the UCH II region, MM1, and MM2 were measured in the VLA 3.6 cm, PdBI 1.2 mm, and SMA 1.3 mm images (Fig. 1), respectively. Note that the coordinates of MM1 correspond to the coordinates of MM1-main, listed in Table 3. (c) Data from Sánchez-Monge et al. (2008). Deconvolved size and PA correspond to the component VLA 3 from Sánchez-Monge et al. (2008), which is the component associated with the easternmost 2MASS source shown in Fig. 1c. (d) 1.2 mm PdBI continuum map done with natural weighting; for flux densities and coordinates for the different subcondensations detected in the uniform-weighted map, see Table 3.


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