LABOCA 870 μm dust continuum mapping of selected infrared-dark cloud regions in the Galactic plane

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Table 1

Target fields mapped with LABOCA.

Field^a	Map size	No. of maps	On-source time	1σ rms noise^b
	[′ × ′]		[min]	[mJy beam^-1]

G1.87-0.14	30.2 × 27.9	3	50.7	80–90 (90)
G2.11+0.00	31.3 × 26.7	5	79.2	60
G11.36+0.80	30.1 × 27.7	3^c	48.9	40–50 (40)
G13.22-0.06	33.1 × 32.6	3	76.0	60–90 (80)

Notes.

^(a)

The fields are named here after their approximate central Galactic coordinates (l, b).

^(b)

These rms noise values refer to the maps used in the analysis (see text). The value given in parenthesis is the 1σ noise adopted in the clumpfind analysis.

^(c)

The observations were interrupted during the fourth mapping of this field, and therefore only the first three maps could be used.

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