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馬克斯威次毫米波望遠鏡 JCMT 網站 (英文)
馬克斯威次毫米波望遠鏡
馬克斯威次毫米波望遠鏡是目前全世界專門用於探測次毫米輻射之單碟望遠鏡中最大的

馬克斯威次毫米波望遠鏡 (JCMT) 位居美國夏威夷 (Hawaii) 大島 (Big Island) 上海拔4000多公尺的毛納基(Mauna kea) 山頂上，是目前世界上最大之專注在次毫米波段探索宇宙的望遠鏡。馬克斯威次毫米波望遠鏡擁有直徑15米的主鏡以及地球上絕佳的觀測天候條件。天文學家可以利用掛載其上的一系列先進的儀器套件，包括操作於450微米與850微米的連續譜相機 SCUBA2、850微米16像素譜線接收機 HARP、以及由中研院天文所提供之多波段單像素譜線接收機 Namakanui 等觀測宇宙中天體次毫米波的輻射。JCMT在研究鄰近地球的彗星、太陽系中的行星與衛星、本銀河系分子雲內的恆星形成區域，一直到系外星系和高紅移的早期宇宙等領域持續有卓越的貢獻！馬克斯威次毫米波望遠鏡同時也是事件視界望遠鏡 (EHT) 的成員，成功取得人類史上首張在 M87 星系中心的黑洞影像。

本所為馬克斯威次毫米波望遠鏡的運轉提供了許多重要的貢獻，包括派遣工程師和科學家，以及提供格陵蘭望遠鏡的備用接收機組Namakanui。台灣的天文學家同時積極參與馬克斯威次毫米波望遠鏡的科學研究，包括參與大部分的大型跨國科學觀測計畫 。

s Magnetized Inflow
磁場對銀河系中心黑洞附近氣體吸積的影響
Namakanui
本所提供之格陵蘭望遠鏡備用單像素多波度接收機 Namakanui

期刊論文(187)

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