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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

「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 detectability of [CII]@z=6.4<br />

• N=50, Tsys = 125K (PWV = 0.91mm or tau220 =<br />

0.052; typical winter condition in Atacama), dv = 50<br />

km/s, dual pol.<br />

24 sec (!) for 1σ = 2.54 mJy/beam (but ignoring<br />

continuum)<br />

• cf. ALMA calculator recommends Tsys = 168 K (PWV =<br />

2.75mm or tau220 = 0.14; typical Mauna-Kea like <br />

condition) for this frequency (better atmospheric<br />

conditions will be used for short wavelengths<br />

observing programs)<br />

45 sec<br />

http://www.eso.org/sci/facilities/alma/observing/tools/etc/<br />

Version: Dec. 17, 2010

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