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Chapter
Effective Sensitivity of a Non-Uniform Phased Array of Short Dipoles
Short dipoles are a key element in new low frequency array antennas as proposed for LOFAR and other astronomical applications. Unfortunately standard texts on short dipole antennas are based on the effective a...
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Article
Effective Sensitivity of A Non-uniform Phased Array of Short Dipoles
Short dipoles are a key element in new low frequency array antennas as proposed for LOFAR and other astronomical applications. Unfortunately standard texts on short dipole antennas are based on the effective a...
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Chapter and Conference Paper
Pupil Plane Interferometry: Some Conclusions from SCASIS
In this contribution we summarize some conclusions from the SCASIS project. The project, which concerns a multiple shearing pupil plane interferometer, was started in 1986 and was concluded in 1992 with the Ph...
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Chapter
SCASIS, Diffraction Limited Imaging using a Redundant Pupil Plane Interferometer
We introduce the concepts of the SCASIS-project. The project aims to realize spectrometry of diffraction limited two-dimensional images from large ground based telescopes. In this paper we describe in detail t...
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Article
Nickel, argon and cobalt in the infrared spectrum of SN1987A: the core becomes visible
Infrared spectra of supernova 1987A taken in April and November 1987 from the Kuiper Airborne Observatory (KAO) show two distinctly different stages in the evolution of the expanding gas shell. In April both t...
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Chapter and Conference Paper
Airborne and groundbased spectrophotometry of comet P/Halley from 5–13 micrometers
Spectrophotometry from 5–10μm (Δλ/λ ≈ 0.02) of comet Halley was obtained from the Kuiper Airborne Observatory on 1985 December 12.1 and 1986 April 8.6 and 10.5, UT. 8–13 μm data were obtained on 17.2 December 198...
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Chapter and Conference Paper
Reflection Nebulae, Non-Equilibrium Thermal Emission, and IRAS
The 1–13 micron spectra of visual reflection nebulae are presented, and their implications for the IRAS 12 micron band discussed.
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Article
A simulation of the thermal behaviour of the UK-NL millimeter wave telescope
To keep the thermally induced average telescope deformations within 15 μm, a thermal design goal has been set which limits the temperature difference between all locations in the panels, backing structure and ...
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Chapter and Conference Paper
Recombination-Line Observations of the Galactic Centre
Aperture-synthesis observations of the H76α and H11Oα recombination lines are presented for the inner (3pc) region of the Galactic Nucleus. The large line width measured with single dishes (Pauls et al., 1974)...