Technical specification of the millimeter array

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 3357, Issue , 1998, Pages 231-237

  Brown, Robert L ^a  

^a NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

Author keywords

Interferometry; Millimeter array; Millimeter astronomy; Submillimeter astronomy; Telescopes

Indexed keywords

ASTRONOMICAL SATELLITES; ASTROPHYSICS; BOLOMETERS; INTERFEROMETERS; INTERFEROMETRY; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; RADIO ASTRONOMY; TELESCOPES; WIRELESS TELECOMMUNICATION SYSTEMS;

BACKGROUND EMISSIONS; MILLIMETER ARRAY; MILLIMETER ASTRONOMY; PHOTON NOISE; RECEIVER NOISE TEMPERATURES; SUB-MILLIMETER WAVELENGTHS; SUBMILLIMETER ASTRONOMY; SYNTHESIS IMAGING; TECHNICAL DESIGNS; TECHNICAL SPECIFICATIONS;

ASTRONOMY;

EID: 0008648206     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.317357     Document Type: Conference Paper

References (4)

1. R. Hjellming, "Sensitivity Criteria for Aperture Synthesis Arrays," NRAO MMA Memo 29, 1985.
2. A. R. Thompson, J. Moran, and G. Swenson Jr., Interferometry and Synthesis in Radio Astronomy, John Wiley, New York, 1986.
3. A. Kerr, S-K. Pan, "Design of Planar Image Separating and Balanced SIS Mixers," NRAO MMA Memo 151, 1996.
4. A. Franchesini, L. Toffolatti, P. Mazzei, L. Danese, and G. De Zotti, "Galaxy Counts and Contributions to the Background Radiation From 1 μm to 1000 μm," Astron. Ap. Suppl. 89, pp. 285, 1991.