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Book Categories |
Preface | ||
Symposium Organizers and Sponsors | ||
List of Participants | ||
Seeing | 1 | |
Comparing optical and radio - quantum issues | 11 | |
Heterodyne interferometry in the infrared | 19 | |
The SAO submillimeter wavelength array | 27 | |
Imaging techniques: Limitations to the quality of images | 37 | |
Surprise and sociology in multi-disciplinary sciences | 47 | |
HST image restoration: current capabilities and future prospects | 61 | |
Lunar occultations: from past to future achievements | 71 | |
Beam combination for wide field imaging | 83 | |
Direct maximum-entropy image reconstruction from the bispectrum | 91 | |
Source-noise in radio synthesis images of polarized sources | 95 | |
Phase calibration of the proposed millimeter array | 101 | |
VLBA phase-referencing | 105 | |
Radio arrays - mm to meters | 109 | |
The Very Long Baseline Array | 117 | |
Recent results from the VLBA | 125 | |
MERLIN A phase-stable 'VLBI' array | 128 | |
The Southern Hemisphere VLBI Experiment program, SHEVE | 131 | |
The Sydney University Stellar Interferometer (SUSI) | 135 | |
The VLT Interferometer | 143 | |
The Big Optical Array | 151 | |
Progress on G12T | 155 | |
The COAST interferometer | 163 | |
An adaptive steerable imaging array | 167 | |
CIROI project | 171 | |
The baseline metrology system of the USNO astrometric interferometer | 174 | |
Design and construction of a beam combiner and related hardware | 177 | |
An overview of the SUSI control system | 181 | |
The fringe tracking servo in SUSI | 184 | |
Motion of the delay lines of an optical interferometer when reconstructing an image by redundant spacing calibration | 187 | |
The micro-precision interferometer testbed instrument design | 193 | |
Phase and image reconstruction from pupil-plane observations in the near infrared: integration of the phasors | 197 | |
Radio source variability as a tool for very high resolution | 201 | |
Iterative blind deconvolution method with use of Lucy's algorithm: application to IR speckle data | 205 | |
Speckle imaging with the bispectrum and without reference star | 209 | |
CLEAN/MEM deconvolution errors: semicompact sources | 212 | |
Generalized versus classical maximum entropy for imaging | 215 | |
Super-resolution by phase-gradient unravelling | 218 | |
Restoration over fields of view wider than the isoplanatic patch | 221 | |
Differential diffraction in Michelson stellar interferometry | 224 | |
Optical fibres in radioastronomy | 227 | |
Recent developments in mm and sub-mm interferometry | 235 | |
High resolution radio source maps at 73.8 MHz | 243 | |
AIPS++: A new astronomical imaging package | 247 | |
Latest technical developments at the infrared spatial interferometer | 257 | |
Integrated optics in astronomical interferometry | 261 | |
Adaptive optics: performance and limitations | 273 | |
Laser guide star adaptive optics: present and future | 283 | |
Laser guide star adaptive optics on the 1.5 m telescope at the Starfire Optical Range | 293 | |
Minimum redundant aperture masking interferometry with tip-tilt wavefront correction | 296 | |
Observations of seeing at 0.5 and 12.4 [mu]m | 299 | |
Preliminary seeing measurements for SUSI | 302 | |
Aspects of the theoretical performance of modal adaptive optics | 305 | |
Simulation study of a low-light-level wavefront sensor driving a low-order, near-IR adaptive optics system | 308 | |
Fringe visibility and phase measurements | 311 | |
Speckle vs non-redundant masking | 317 | |
MAPPIT: optical interferometry with non-redundant masks | 327 | |
Optimal linear arrays for wide bandwidths | 331 | |
High resolution and high sensitivity spectral-line imaging with multiple arrays | 334 | |
High resolution imaging forty years ago | 337 | |
Results with the extended MERLIN | 343 | |
High resolution image reconstruction at Yunnan Observatory | 346 | |
High resolution imaging at mm-wavelengths with the Hat Creek Array | 349 | |
Miyun 232 MHz survey and some new imaging techniques | 352 | |
Compact array mapping of the nuclear starburst in NGC 7552 | 355 | |
ATCA radio polarization observations of NGC 1566 and NGC 1672 | 358 | |
Fluctuations of polarized radiation in a random magnetoplasma | 361 | |
High angular resolution observations of Her 36 | 364 | |
The Caltech-Jodrell Bank (CJ) VLBI snapshot surveys | 367 | |
First experimental results from pupil masking on a solar telescope | 370 | |
Optical interferometry in the multi-speckle mode | 373 | |
Near infrared high angular resolution observations of stars and circumstellar regions by the |
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Add Very high angular resolution imaging, In the rapidly developing field of high resolution astronomical imaging, there are strong parallels between the interferometric methods used at radio frequencies and in the optical/infrared, despite the differences in hardware. IAU Symposium 158 brought t, Very high angular resolution imaging to the inventory that you are selling on WonderClubX
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Add Very high angular resolution imaging, In the rapidly developing field of high resolution astronomical imaging, there are strong parallels between the interferometric methods used at radio frequencies and in the optical/infrared, despite the differences in hardware. IAU Symposium 158 brought t, Very high angular resolution imaging to your collection on WonderClub |