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Table B.3:

Complete results of CARMA observations at 1 and 3 mm.

Obs. date
Effective Target sourcea Continuum fluxb rmsc Gaussian size RAb Decb
  wavelength   (P) (G)   (arcsec) (J2000) (J2000)
  (mm)   (mJy) (mJy/bm)      
20080518 1.33 GSC 00446-00153 43.6 50.5 6.0 $0.46 \pm 0.32$ 18 30 06.2 +00 42 33.6
20080618 3.15 EC 82 <2.9d 1.0 - 18 29 56.8 +01 14 46.0
    EC 90 11.3 11.6 1.0 $1.69 \pm 0.97$ 18 29 57.8 +01 14 06.9
    182900.88+002931.5 3.4 3.9 0.6 (unresolved) 18 29 00.9 +00 29 31.7
    IRAS 18268-0025 <1.9d 0.6 - 18 29 28.2 -00 22 57.1
    CoKu Ser G3 <1.6d 0.5 - 18 29 01.8 +00 29 54.6
    VV Ser <1.8d 0.6 - 18 28 47.9 +00 08 40.0
20080619 3.15 182858.08+001724.4 <1.9d 0.6 - 18 28 58.1 +00 17 24.4
    182850.20+000949.7 <1.9d 0.6 - 18 28 50.2 +00 09 49.7
    182944.10+003356.1 <1.7d 0.6 - 18 29 44.1 +00 33 56.1
    182936.19+004216.7 <2.7d 0.9 - 18 29 36.2 +00 42 16.7
20080620 1.33 EC 82 <15.7d 5.2 - 18 29 56.8 +01 14 46.0
    EC 90 91.8 91.7 10.4 (unresolved) 18 29 57.7 +01 14 07.0
    182900.88+002931.5 <16.4d 5.5 - 18 29 00.9 +00 29 31.6
    IRAS 18268-0025 <15.6d 5.2 - 18 29 28.2 -00 22 57.1
    CoKu Ser G3 <17.1d 5.7 - 18 29 01.8 +00 29 54.6
    VV Ser <14.8d 4.9 - 18 29 47.9 +00 08 40.0
    182858.08+001724.4 <24.6d 8.2 - 18 28 58.1 +00 17 24.4
    182850.20+000949.7 <98.2d 32.7 - 18 28 50.2 +00 09 49.7
20080622 3.15 182936.19+004216.7 <5.3d 1.8 - 18 29 36.2 +00 42 16.7
    GSC 00446-00153 6.8 8.1 1.0 $2.71 \pm 1.58$ 18 30 06.3 +00 42 34.2
20080704 1.33 EC 97 <23.3d 7.8 - 18 29 58.2 +01 15 22.0
    182850.20+000949.7 <22.8d 7.6 - 18 28 50.2 +00 09 49.7
    182944.10+003356.1 <15.0d 5.0 - 18 29 44.1 +00 35 56.1
    182936.19+004216.7 <8.7d 2.9 - 18 29 36.2 +00 42 16.7
    GSC 00446-00153 90.8 97.6 2.8 $0.67 \pm 0.23$ 18 30 06.2 +00 42 33.6

Notes. (a) In the case of SSTc2d names, only the coordinates (in J2000) are shown.
(b) Continuum flux and position are from fits in the (uv) plane. For sources that were detected at 3$\sigma$, both the point-source flux (P) and the integrated flux for a Gaussian (G) are shown. For sources that were not detected, the coordinates of the phase centre are quoted.
(c) Calculated from the cleaned image.
(d) Quoted value is 3$\sigma$ upper limit.


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