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Very high angular resolution imaging Book

Very high angular resolution imaging
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 has a rating of 3 stars
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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
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  • Very high angular resolution imaging
  • Written by author J. G. Robertson and W. J. Tango
  • Published by Dordrecht [The Netherlands] ; Kluwer Academic, c1994., 2007
  • 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
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Authors

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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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

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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

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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

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