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Table 2:

Millimeter sources found in our MAMBO-2 maps.
Source name Star Field $\alpha$(J2000) a $\delta$(J2000) a Integrated flux density b S/N Source
        at 1.2 mm (mJy)   FWHM
MM145428+160439 GJ569 14  54  28.2 16  04  39 $ 5.3 \pm 1.1$ 4.9 11''
MM184222+593828 GJ725 18  42  22.7 59  38  28 30-63 c 6.7-7.3 13''-15''
MM184253+593756 GJ725 18  42  53.3 59  37  56 $ 9.7 \pm 1.9 $ 5.1 11''
MM134539+145139 GJ526 13  45  39.0 14  51  39 $3.2 \pm 0.7 $ 4.4 11''
MM134540+145446 GJ526 13  45  40.7 14  54  46 $4.3 \pm 0.8 $ 5.2 11''
MM134541+145417 GJ526 13  45  41.3 14  54  17 $6.3 \pm 1.0 $ 6.1 11''
MM134543+145317 GJ526 13  45  43.1 14  53  17 $3.0 \pm 0.7 $ 4.9 11''
MM134546+145240 GJ526 13  45  46.7 14  52  40 $5.6 \pm 0.7 $ 8.6 11''
MM163007-123942 GJ628 d 16  30  07.6 -12  39  42 $7.3 \pm 1.2 $ 6.2 $14\pm 4''$
MM163022-123925 GJ628 e 16  30  22.3 -12  39  25 $3.8 \pm 0.9 $ 4.4 $17\pm 5''$
MM163019-123830 GJ628 f 16  30  19.7 -12  38  30 $4.1 \pm 0.8 $ 4.9 11''
MM163015-123911 GJ628 g 16  30  15.6 -12  39  11 $4.8 \pm 0.8 $ 6.2 11''
MM163013-124057 GJ628 h 16  30  13.7 -12  40  57 $4.3 \pm 1.0 $ 4.8 11''

a The MAMBO coordinate uncertainties are $\sim $3.5''. b Flux density (mJy) is integrated under the fitted 2D-Gaussian. c Flux density is provided as lower and upper limits because the source is located close to one of the borders of the map where some systematics remain in the data (see text). d, e, f, g, h These sources were found in survey I; d is GJ628-W, e is GJ628-E, f is GJ628-NE, g is GJ628-NW, and h is GJ628-SW in Fig. 2 and Table 3 of Lestrade et al. (2006). Note that there are typographic errors in the minute column of declinations in Table 3 of Lestrade et al. (2006). The positions of the GJ628 sources given now are correct and supersede this first publication. Also, the flux densities in this first publication were peak flux densities while they are integrated flux densities now.


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