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Table 3.

Participating telescopes.

Name Code D G Tsys ηA SEFD Δ512, 20 σrms
(m) (K Jy−1) (K) (Jy) (mJy) (mJy)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
Brewster Br 25 0.033 110 0.22 3333.3 23.44 164.09
Effelsberg Eb 80a 0.140 140 0.08 1000 12.84 89.87
Fort Davis Fd 25 0.039 140 0.22 3589.7 24.32 170.28
Kitt Peak Kp 25 0.028 100 0.22 3571.4 24.26 169.85
Los Alamos La 25 0.042 120 0.22 2857.1 21.70 151.91
Metsähovi Mh 14 0.017 300 0.3 17647.1 53.94 377.55
Mauna Kea Mk 25 0.019 100 0.22 5263.2 29.45 206.18
North Liberty Nl 25 0.022 130 0.22 5909.1 31.21 218.47
Onsala On 20 0.049 250 0.43 5102 29.00 203.00
Owens Valley Ov 25 0.035 120 0.22 3428.6 23.77 166.41
Plateau de Bure Pb 36b 0.22 180 0.7 818.2 11.61 81.29
Pie Town Pt 25 0.044 100 0.22 2272.7 19.36 135.52
Pico Veleta Pv 30 0.153 100 0.6 653.6
Yebes Ys 40 0.09 150 0.2 1666.7 16.58 116.03

Notes. Columns: 1 – telescope name; 2 – abbreviation for the telescope name; 3 – diameter; 4 – antenna gain; 5 – zenith system temperature; 6 – aperture efficiency; 7 – zenith SEFD; 8 – sensitivity on the baseline to Pico Veleta, for a 20 s fringe fit interval and 512 Mbps recording rate; 9 – 7σ detection threshold.

(a)Effective diameter at 86 GHz.

(b)Effective diameter in the phased array mode.

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