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馬克斯威次毫米波望遠鏡 (JCMT)

JCMT 網站 (英文)
James Clerk Maxwell Telescope
JCMT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 。

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 (182)

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