Open Access

Table 1

Telescopes, receivers, and backends used in this project along with observed frequency ranges.

Telescope Receiver Backend v (a) Map coverage Average rms(b)
(GHz) G1.3 (″) G1.6 (″) G1.3 TmB (mK) G1.6 TmB (mK)
IRAM 30 m EMIR FFTS 85–93 860 × 550 550 × 330 73 43
(E090) 93–101 850 × 440 550 × 330 88 51
101–109 860 × 550 550 × 330 95 55
109–117 850 × 440 550 × 330 110 71
APEX PI230 FFTS4G 217–221 780 × 500 600 × 300 254 266
229–233 780 × 500 600 × 300
SHeFI (APEX2) XFFTS 265–269 - 650 × 340 - 182
FLASH+(345) XFFTS 289.5–293.5 150 × 150 220 × 160 70 73
301.5–305.5 150 × 150 220 × 160 63 65
328–332 - 600 × 300 - 115
340–344 - 600 × 300 - 116
341.5–345.5 250 × 250 400 × 400 168 116
344–348 - 500 × 300 - 189
353.5–357.5 - 400 × 400 - 141
356–360 - 500 × 300 - 152
FLASH+(460) XFFTS 433–437 150 × 150 220 × 160 209 511
459–463 - 600 × 300 - 260

Notes. (a)Covered frequency range. (b) Average rms value in the reduced cubes after smoothing to a spectral resolution of 1 km s−1 and after spatial regridding to a common pixel size of 14.5″ (see Sect. 2.3). The centres of the mapped regions are given in the text.

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