Paper
31 July 1998 Japanese Large Millimeter and Submillimeter Array
Masato Ishiguro
Author Affiliations +
Abstract
The Large Millimeter and Submillimeter Array (LMSA) being planned at the National Astronomical Observatory of Japan (NAOJ) is a high priority plan for the future large-scale ground-based astronomical facility coming after the Subaru telescope. The LMSA will consist of 50 10-m antennas. The planning of the instrument places a special emphasis on high- resolution and high-sensitivity observations at submillimeter wavelengths. Efforts at Nobeyama Radio Observatory (NRO) have been focused in the site testing at the two candidate sites in Northern Chile and engineering developments, especially in antenna design, submillimeter mixers, high-speed digital technology for wide-band correlator, and phase calibration methods. A possible joint-array operations with other large array projects is under discussion.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Masato Ishiguro "Japanese Large Millimeter and Submillimeter Array", Proc. SPIE 3357, Advanced Technology MMW, Radio, and Terahertz Telescopes, (31 July 1998); https://doi.org/10.1117/12.317359
Lens.org Logo
CITATIONS
Cited by 11 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Antennas

Opacity

Optical correlators

Astronomy

Observatories

Fourier transforms

Receivers

RELATED CONTENT

Overview of engineering activities at the SMA
Proceedings of SPIE (July 12 2008)
The Allen Telescope Array
Proceedings of SPIE (September 28 2004)
The Atacama Large Millimeter Array (ALMA)
Proceedings of SPIE (February 04 2003)
Mathematic model of the FX correlator of the Chinese VLBI...
Proceedings of SPIE (September 18 2001)

Back to Top