The Future Large Millimeter and Submillimeter Array (LMSA/ALMA)Project

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概要

• 論文の詳細を見る

• The Japanese Large Millimeter and Submillimeter Array (LMSA) and the US/EuropeAtacama Large Millimeter Array (ALMA) are planned to be constructed at a very high and drysite in the northern Chile and to be operated at the frequency range of 80 to 900 GHz fromaround the year of 2008. LMSA (or ALMA) will provide 0.01 arcsecond resolution and a veryhigh sensitivity comparable to a 70 m single dish. Their main targets include planetary systemformation and galaxy formation/evolution. Big advances in other researches (e.g., cosmology) arealso expected. The technical challenges to key instruments for such arrays are now being tackled.The international collaboration toward a so-called `enhanced ALMA' (an unfied array of LMSAand ALMA) is under discussion.

• 宇宙航空研究開発機構の論文

著者

• Ryohei Kawabe

  Nobeyama Radio Observatory (nro) National Astronomical Observatory (naoj)

• LMSA working

  LMSA working group

関連論文

• The Future Large Millimeter and Submillimeter Array (LMSA/ALMA)Project

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