activity
19972009
most citedThe Submillimeter Array

622 citations · 1.1k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2009★ 45 cited

The AMiBA Hexapod Telescope Mount

Patrick M. Koch, Michael Kesteven, Hiroaki Nishioka +35

AMiBA is the largest hexapod astronomical telescope in current operation. We present a description of this novel hexapod mount with its main mechanical components -- the support co…

astro-ph2008★ 38 cited

The Yuan-Tseh Lee Array for Microwave Background Anisotropy

Paul T. P. Ho, Pablo Altamirano, Chia-Hao Chang +52

The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelen…

astro-ph2004★ 622 cited

The Submillimeter Array

Paul T. P. Ho, James M. Moran, Kwok Yung Lo

The Submillimeter Array (SMA), a collaborative project of the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), h…

astro-ph2002

Terahertz Initiatives at the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO)

Antony A Stark, Adair P. Lane, Christopher L. Martin +3

The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) is a 1.7-meter diameter offset Gregorian instrument located at the NSF Amundsen-Scott South Pole Station. This…

astro-ph2001★ 13 cited

Gas Distribution and Starburst Activity in the Widely Separated Interacting Galaxies NGC 6670

Wei-Hao Wang, K. Y. Lo, Yu Gao +1

We present high resolution H I 21 cm line, 20 cm radio continuum, and CO(1-0) line observations of the luminous infrared galaxy NGC 6670. NGC 6670 consists of two edge-on disk gala…

astro-ph2001★ 5 cited

Infrared Line Emission in the Interacting Region of Arp 244 (the Antennae): Colliding Molecular Cloud Complexes ?

M. C. Liang, T. R. Geballe, K. Y. Lo +1

We report velocity-resolved spectroscopy of infrared hydrogen recombination lines in the interacting region of the Antennae galaxies (NGC 4038/4039). It generally has been assumed…