Advanced technology MMW, radio, and terahertz telescopes : 26-28 March 1998, Kona, Hawaii /

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Bibliographic Details
Imprint:Bellingham, Wash. : Society of Photo-optical Instrumentation Engineers, ©1998.
Description:xv, 786 pages : illustrations (some color) ; 28 cm.
Language:English
Series:SPIE proceedings series, 0277-786X ; v. 3357
Proceedings of SPIE--the International Society for Optical Engineering ; v. 3357.
Subject:
Format: Print Book
URL for this record:http://pi.lib.uchicago.edu/1001/cat/bib/3634385
Hidden Bibliographic Details
Varying Form of Title:Advanced technology millimeter wave, radio, and terahertz telescopes
Other authors / contributors:Phillips, Thomas G.
Society of Photo-optical Instrumentation Engineers.
European Southern Observatory.
American Astronomical Society.
Astronomical Society of the Pacific.
Canadian Astronomical Society.
ISBN:0819428043
9780819428042
Notes:Includes bibliographical references and index.
Table of Contents:
  • Green Bank Telescope and the Millimeter Array
  • Superconductive hot-electron mixers for terahertz heterodyne receiver applications
  • Heterodyne instrumentation at the CSO
  • Research on submillimeter-wave hot-electron bolometer mixers in Europe
  • Laser micromachining of silicon: a new technique for fabricating terahertz imaging arrays
  • Development of SIS mixers for 1 THz
  • Design and fabrication of 800- to 900-GHz Pb-alloy SIS mixing device incorporating an on-substrate tuning element
  • Diode frequency multipliers for terahertz local oscillator applications
  • 2- to 6-THz heterodyne receiver array for the Stratospheric Observatory for Infrared Astronomy (SOFIA)
  • Gaussian-beam-mode analysis of multibeam quasi-optical systems
  • Receiver-beam characterization for the SMA
  • W-band HEMT-based power-amplifier module for millimeter-wave LO multipliers
  • Receivers for the Millimeter Array
  • Terahertz photomixing in low-temperature-grown GaAs
  • Photonic local oscillator system for the Millimeter Array
  • Multipliers for terahertz local oscillators
  • Array receiver development at KOSMA for the submillimeter and terahertz spectral range
  • CHAMP: the Carbon Heterodyne Array of the MPIfR
  • Trends in millimeter-wave antenna design
  • Large Millimeter Telescope project: overview and optical design
  • Heinrich Hertz Telescope
  • Submillimeter array
  • Active segmented primary reflector and pointing accuracy of the Large Millimeter Telescope (LMT)
  • Technical specification of the Millimeter Array
  • LSA project
  • Japanese Large Millimeter and Submillimeter Array
  • CSO-JCMT Interferometer and 183-GHz radiometric phase correction
  • Measurement program for the Green Bank Telescope
  • Development of a broadband submillimeter grating spectrometer
  • Hertz: an imaging polarimeter
  • Silicon nitride micromesh bolometer arrays for SPIRE
  • SCUBA: a submillimeter camera operating on the James Clerk Maxwell Telescope
  • Bolometer array development at the Max-Planck-Institut fuer Radioastronomie
  • Bolocam: a millimeter-wave bolometric camera
  • Heterodyne instrument for FIRST (HIFI): preliminary design
  • Submillimeter-wave astronomy satellite: science objectives and instrument description
  • Design of large-bandwidth acousto-optical spectrometers
  • Wideband digital autocorrelator for FIRST
  • Submillimeter Fourier transform spectroscopy
  • WASP: wideband spectrometer for heterodyne spectroscopy
  • Digital cross-correlation at 250 MHz using high-performance FPGAs
  • SPIRE: a bolometer instrument for FIRST
  • DASI: Degree Angular Scale Interferometer for imaging anisotropy in the cosmic microwave background
  • Wideband correlators for radio astronomy
  • Phase correction for the BIMA array: atmospherical model calculations for the design of a prototype correlation radiometer
  • Phase correction at millimeter wavelengths using observations of water vapor at 22 GHz
  • System design for the Millimeter Array
  • Antenna design for the Millimeter Array
  • Measurement, modeling, and adjustment of the 10.4-m-diameter Leighton telescopes
  • Atmospheric conditions at a site for submillimeter-wavelength astronomy
  • Plans for a 10-m submillimeter-wave telescope at the South Pole
  • Wideband 3-mm SIS mixers operated with partial saturation
  • Space-qualified wideband and ultrawideband acousto-optical spectrometers for millimeter and submillimeter radio astronomy
  • Digital techniques for ground-based low-frequency radio astronomy
  • SPARO: the submillimeter polarimeter for Antarctic remote observing
  • Removing sky contributions from SCUBA data
  • New frequency multipliers for millimeter- and submillimeter-wavelength coherent array receiver applications
  • Design and performance of a dual-polarizing detector system for broadband astronomical spectroscopy at submillimeter wavelengths
  • Sensitivity improvements of SIS photon detectors
  • Characterization of a 200-GHz SIS mixer
  • Receivers for ground-based millimeter-wave radio telescopes
  • Multibeam SIS mixer module for a focal plane array receiver
  • Broadband microwave imaging spectroscopy with a solar-dedicated array
  • 345-GHz facility SIS receiver for the JCMT
  • FTS measurements of submillimeter-wave opacity at Pampa la Bola
  • DREAM: Dutch real-time acquisition mode for SCUBA
  • Method and apparatus for manufacturing high-accuracy radio telescope reflector panels
  • Green Bank Telescope: an overview
  • The Large Millimeter Telescope (LMT) project
  • 12-m antenna design for a joint US-European array
  • Possible explanation of the planetary rings' behavior in the radio and millimeter-wave range via superdiamagnetic model
  • Transmission of timing references to sub-picosecond precision over optical fiber
  • Amplitude stabilization of the Green Bank Telescope fiber optics
  • New KOSMA 3-m telescope
  • New technique for submillimeter-wave reflector construction
  • Array feed signal combining compensation system for antenna reflector deformations
  • Meter- and decameter-wavelength array for astrophysics and solar radar
  • Next-generation radio telescope of the 12- to 15-m class for the future large-interferometer arrays in the southern hemisphere
  • Alternative methods of adaptation of millimeter radio telescopes
  • Proposed 12-m submillimeter antenna design for the Large Southern Array