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. Author manuscript; available in PMC: 2017 Nov 13.
Published in final edited form as: Astron Astrophys. 2017 Jul;603:A124. doi: 10.1051/0004-6361/201730459

Table 1.

Observed frequency ranges and telescope parameters.

Rec.a Backend Freq.b
[GHz]
δυc
[km s-1]
ηMB d HPBWe
[arcsec]
E0 FFTS   80–117 0.75–0.51 0.87–0.82 31–21

E1 WILMA 128–176 4.7–3.4 0.80–0.74 19–14

E2 FFTS 202–275 0.30–0.22 0.70–0.56 12–9

E3 FFTS 275–305 0.22–0.20 0.56–0.50 9–8
FFTS 328–359 0.18–0.17 0.46–0.40 8–7

Notes.

(a)

Emir receiver.

(b)

Observed frequency range.

(c)

Spectral resolution in velocity units (δυ) in the observed frequency ranges.

(d)

Antenna efficiencies.

(e)

The half power beam width can be well fitted by HPBW[arcsec]≈2460/Frequency[GHz].