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


Table 1

Observational setups of the EMoCA survey.

Setup Frequency range Date of t start a N a b Baseline t int d Calibratorse Peakf



LSB USB observation (UTC) rangec B A P Δα Δδ
GHz GHz yyyy-mm-dd hh:mm m min ′′ ′′

S1 84.1–87.8 96.2–99.8 2012-08-27 01:05 26 17–400 54.7 1 3 2 0.2 −2.4
S2 87.7–91.4 99.7–103.4 2012-06-05 09:03 20 14–392 24.2 1 3 2 1.2 −2.4
2012-07-01 07:04 13 25–393 40.0 1 3 2 1.2 −2.6
2012-07-03 06:36 21 14–395 48.4 1 3 2 0.6 −2.3
2012-09-28 21:57 25 20–387 44.1 1 4 2 0.2 −2.5
S3 91.4–95.1 103.4–107.1 2012-06-06 08:20 18 15–395 40.2 1 3 2 0.7 −2.4
2012-06-18 07:29 22 15–395 40.4 1 3 2 0.6 −2.2
S4 95.0–98.7 107.0–110.7 2012-07-04 05:38 21 17–398 8.1 1 3 2 0.1 −2.3
2012-08-01 02:32 24 19–442 34.9 1 3 2 0.1 −2.4
2012-08-10 00:45 26 21–400 35.0 1 3 2 0.2 −2.4
S5 98.7–102.4 110.7–114.4 2014-04-05 06:22 38 15–413 24.4 2 4 5 0.2 −2.4

Notes.

(a)

Start time of observation.

(b)

Number of ALMA 12 m antennas.

(c)

Minimum and maximum projected baseline separations.

(d)

On-source integration time.

(e)

Bandpass (B), amplitude (A), and phase (P) calibrators. The calibrators are: 1: B1730-130, 2: J1700-2610, 3: Neptune, 4: Titan, 5: J1744-3116.

(f)

Offset of the continuum peak position of Sgr B2(N1) with respect to the phase center, in equatorial coordinate system (J2000). Measurement sets with Δα differing from 0.1′′ by more than 0.2′′ (marked with a ) are believed to be affected by an astrometric problem.

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