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Table 1

Telescope characteristics and main observational parameters.

Herschel Obs. date Durat. HIFISTARS setting Sky frequency coverage HIFI HPBW Tmb/ Cal.§
OBSID yr:mo:day (s) Name LO (GHz) LSB (GHz) USB (GHz) (K) band (′′) uncer.

1342192528 2010:03:21 1575 14 564.56 556.55–560.69 568.54–572.68 93 1B 37.5 1.3 15%
1342192529 2010:03:21 1575 13 614.86 606.85–610.99 618.84–622.98 91 1B 34.5 1.3 15%
1342192533 2010:03:21 1623 12 653.55 645.55–649.69 657.54–661.68 131 2A 32.0 1.3 15%
1342192534 2010:03:21 617 17 686.42 678.42–682.56 690.41–694.55 142 2A 30.8 1.3 15%
1342194680 2010:04:13 1618 11 758.89 750.90–755.04 762.89–767.03 196 2B 27.8 1.3 15%
1342195039 2010:04:18 1505 10 975.23 967.27–971.41 979.26–983.40 352 4A 21.7 1.3 20%
1342195040 2010:04:18 1505 09 995.63 987.67–991.81 999.66–1003.80 364 4A 21.3 1.3 20%
1342194786 2010:04:17 1487 08 1102.92 1094.98–1099.11 1106.97–1111.10 403 4B 19.2 1.3 20%
1342194787 2010:04:17 1487 07 1106.90 1098.95–1103.09 1110.94–1115.08 416 4B 19.1 1.3 20%
1342192610 2010:03:22 1618 06 1157.67 1149.72–1153.85 1161.71–1165.84 900 5A 18.3 1.5 20%
1342192611 2010:03:22 1538 05 1200.90 1192.95–1197.08 1204.94–1209.07 1015 5A 17.6 1.5 20%
1342195105 2010:04:19 3547 04 1713.85 1709.11–1711.68 1716.37–1718.97 1238 7A 12.4 1.4 30%
1342195106 2010:04:19 3851 03 1757.68 1752.95–1755.52 1760.20–1762.77 1580 7A 12.0 1.4 30%
1342230403 2011:10:09 3103 19 1766.89 1762.23–1764.78 1769.48–1772.04 1248 7A 12.0 1.4 30%
1342194782 2010:04:17 2992 16 1838.31 1833.59–1836.16 1840.84–1843.41 1300 7B 11.6 1.4 30%
1342196570 2010:05:15 3207 16 1838.47 1833.73–1836.30 1840.99–1843.55 1415 7B 11.6 1.4 30%
1342194781 2010:04:17 1535 01 1864.82 1860.10–1862.67 1867.36–1869.92 1330 7B 11.4 1.4 30%

Notes.

(§)

Following Teyssier et al. (2012), we based our absolute-calibration accuracy estimates on the error budget reported by Roelfsema et al. (2012), plus an additional contribution arising from the ripples in the baseline for bands 7A and 7B.

(†)

Instabilities in the baseline that simultaneously affect both receivers were removed by discarding several sub-scans.

(‡)

Ripples in the baseline, which mainly affected the V-receiver, were removed by discarding several sub-scans.

(♭)

Setting 19 was added later in the program.

(♯)

Setting 16 was observed twice using a slightly different value for the systemic velocity.

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