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「今後10年の(日本の)電波天文学」 銀河の研究 ... - 国立天文台 野辺山

「今後10年の(日本の)電波天文学」 銀河の研究 ... - 国立天文台 野辺山

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ALMA vs single dish telescopes<br />

telescope D [m] Main beam eff. Tsys [K] Integration time<br />

ASTE 10 0.6 125 65 hrs<br />

CCAT 25 0.7 125 100 min<br />

IRAM 30 0.54 350 ~12 hrs<br />

New 30m 30 0.7 125 48 min<br />

(30/25) 4<br />

~2.1<br />

New 50m 50 0.7 (!) 125 6.24 min (374 sec)<br />

• ALMA instantaneous bandwidth: 8 GHz (4 GHz per<br />

sideband) for line survey, 24 sec (or 45 sec) per set<br />

• The new 50 m telescope should have the same<br />

line survey speed if it is equipped with a single<br />

beam, 8 × (374sec/45sec) = 66 GHz bandwidth RX<br />

for practical observing conditions for ALMA

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