Exploring molecular complexity with ALMA (EMoCA): Deuterated complex organic molecules in Sagittarius B2(N2)

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Volume 587 (March 2016)

A&A, 587 (2016) A91

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201935428e]

Table 2

Beam sizes and noise levels.

Setup	SPW^a	Frequency	Synthesized beam		rms^c

		range	HPBW	PA^b	mJy
		MHz		°	beam^-1	K

S1	0	84 091–85 966	2.1 × 1.5	−85	3.0	0.16
	1	85 904–87 779	2.0 × 1.5	−83	2.7	0.14
	2	96 154–98 029	1.8 × 1.4	−85	3.0	0.16
	3	97 904–99 779	1.8 × 1.3	−85	3.1	0.16
S2	0	87 729–89 604	1.9 × 1.7	86	3.1	0.15
	1	89 554–91 429	1.8 × 1.6	52	2.8	0.15
	2	99 728–101 602	1.6 × 1.4	48	2.7	0.14
	3	101 552–103 427	1.6 × 1.4	49	2.7	0.14
S3	0	91 368–93 242	2.9 × 1.5	84	3.4	0.12
	1	93 193–95 067	2.8 × 1.5	83	3.1	0.10
	2	103 365–105 239	2.5 × 1.3	82	3.4	0.11
	3	105 189–107 064	2.5 × 1.3	82	3.6	0.12
S4	0	95 021–S96 896	1.9 × 1.4	−82	1.9	0.10
	1	96 846–98 720	1.8 × 1.3	−82	1.9	0.10
	2	107 019–108 893	1.7 × 1.2	−83	2.2	0.11
	3	108 843–110 718	1.6 × 1.2	−82	2.3	0.12
S5	0	98 672–100 546	1.8 × 1.4	−76	2.8	0.14
	1	100 496–102 370	1.7 × 1.4	−76	2.7	0.13
	2	110 669–112 543	1.6 × 1.3	−72	3.5	0.17
	3	112 494–114 368	1.6 × 1.2	−77	4.9	0.24

Notes.

^(a)

Spectral window.

^(b)

Position angle east from north.

^(c)

Median rms noise level measured in the channel maps of the continuum-removed data cubes.

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