Herschel-ATLAS and ALMA - HATLAS J142935.3-002836, a lensed major merger at redshift 1.027

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Volume 568 (August 2014)

A&A, 568 (2014) A92

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Table 2

Continuum emission from H1429−0028.

SPW	λ_cent	rms	Total	A+B	C	D
	[mm]	[mJy]	[mJy]	[mJy]	[mJy]	[mJy]

B3^a	2.80	0.025	0.54 ± 0.11^b	0.374 ± 0.044	0.107 ± 0.044	<0.075
B3-0	2.64	0.063	0.72 ± 0.22	0.49 ± 0.13	0.20 ± 0.16	<0.19
B3-1	2.67	0.038	0.47 ± 0.13	0.309 ± 0.067	0.058 ± 0.067	<0.11
B3-2	2.94	0.070	0.22 ± 0.10	0.22 ± 0.10	<0.21	<0.21
B3-3	2.97	0.054	0.56 ± 0.16	0.38 ± 0.11	0.111 ± 0.094	<0.16
B6	1.28	0.078	5.86 ± 0.99^b	3.69 ± 0.28	1.31 ± 0.27	0.71 ± 0.16
B6-0	1.23	0.217	7.1 ± 1.3	4.12 ± 0.86	1.40 ± 0.69	0.79 ± 0.47
B6-1	1.24	0.137	6.15 ± 0.83	3.67 ± 0.48	1.39 ± 0.50	0.76 ± 0.31
B6-2	1.32	0.132	6.12 ± 0.74	3.92 ± 0.48	1.17 ± 0.42	0.95 ± 0.30
B6-3	1.33	0.115	5.29 ± 0.57	3.26 ± 0.40	1.22 ± 0.28	0.50 ± 0.16

Notes. Information of the different continuum bands targeted by our ALMA observations. Numbers in parenthesis indicate the 1σ uncertainty. Upper limits are set at the 3σ level. Flux densities measured in the clean component map using natural weighting.

^(a)

Considering only the line-free spectral windows 1, 2 and 3.

^(b)

The errors consider a conservative 15% error, added in quadrature, to account for flux density calibration uncertainty, as suggested by ALMA staff.

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