Diffraction-Limited Imaging with Very Large Telescopes

Diffraction-Limited Imaging with Very Large Telescopes
Author: D.M. Alloin
Publisher: Springer Science & Business Media
Total Pages: 444
Release: 2012-12-06
Genre: Science
ISBN: 9400923406

A few years ago, a real break-through happened in observational astronomy: the un derstanding of the effect of atmospheric turbulence on the structure of stellar images, and of ways to overcome this dramatic degradation. This opened a route to diffraction-limited observations with large telescopes in the optical domain. Soon, the first applications of this new technique led to some outstanding astrophysical results, both at visible and infrared wavelengths. Yet, the potential of interferometric observations is not fully foreseeable as the first long-baseline arrays of large optical telescopes are being built or cOIIllnissioned right now. In this respect a comparison with the evolution of radio-astronomy is tempting. From a situation where, in spite of the construction of giant antennas, low angular resolution was prevailing, the introduction of long baseline and very long baseline interferometry and the rapid mastering of sophisticated image reconstruction techniques, have brought on a nearly routine basis high dynamic range images with milliarcseconds resolution. This, of course, has completely changed our views of the radio sky.

Literature 1984, Part 2

Literature 1984, Part 2
Author: S. Böhme
Publisher: Springer Science & Business Media
Total Pages: 928
Release: 2013-04-17
Genre: Science
ISBN: 3662123460

Instrumentation and Research Programmes for Small Telescopes

Instrumentation and Research Programmes for Small Telescopes
Author: J.B. Hearnshaw
Publisher: Springer Science & Business Media
Total Pages: 464
Release: 2012-12-06
Genre: Science
ISBN: 9401094330

This volume is the proceedings of IAU Symposium No. 118 on "Instrumentation. and Research Programmes for Small Telescopes", where small telescopes were defined as those ground-based instruments with apertures less than 1.5m. The scientific goal of the symposium was to emphasise research programmes which were more suited to smaller tele scopes, on which frequent regular observations can be made. A wide variety of topics on instrumentation, photometry, spectroscopy and polarimetry of objects in the solar system to extragalactic systems were discussed. Each of the four scientific days of the symposium comprised a number of invited review papers, contributed oral papers and discussion sessions devoted purely to the large number (~4) of poster papers. An introductory paper on the research potential of small telescopes sets the scene for the symposium. The proceedings have then been divided into three sections. Section I: Telescopes and instrumentation; Section II: Photometric research programmes; Section III: Spectroscopic research programmes. The diversity of topics within each of these sections indicated the extent to which small telescopes have (and can) contribute greatly to astronomical research. Dr J.A. Graham's summary of the symposium, which illustrates the opportunities available with small telescopes, concludes these proceedings. As in all symposia, the importance of the discussion following each paper was realised. The discussion was recorded on tape (and wherever possible on questions and answer sheets), transcribed and then edited.

Science with the VLT Interferometer

Science with the VLT Interferometer
Author: Francesco Paresce
Publisher: Springer Science & Business Media
Total Pages: 414
Release: 2013-06-29
Genre: Science
ISBN: 354069398X

It has always been ESO's aim to operate the VLT in an interferometric mode (VLTI) which allows the coherent combination of stellar light beams col lected by the four 8-m telescopes and by several smaller auxiliary telescopes. In December 1993, in response to financial difficulties, the ESO Council de cided to postpone implement at ion of the VLTI, Coude trains and associated adaptive optics for all the UTs but included provisions for continuing tech nological and development programmes devoted to the aim of reintroducing these capabilities at the earliest possible date. The desirability of carrying out the full VLTI programme as originally envisaged at the earliest possible moment has not, however, diminished, es pecially in view of VLTI's exceptional capabilities and resulting potential for new and exciting discoveries. In recent years, interferometric projects have begun to playa central role in ground-based high-resolution astronomy, and numerous instruments have been completed or are in the process of construc tion. Several large-aperture interferometers will probably co me on-line near the turn of the century. The impending presence of these new instruments represents an important incentive both for clarifying the scientific cases for various VLTI implementation plans and for ensuring VLTI's competitiveness in the international context over the next 1O~20 years.

Reflecting Telescope Optics II

Reflecting Telescope Optics II
Author: Raymond N. Wilson
Publisher: Springer Science & Business Media
Total Pages: 566
Release: 2013-04-17
Genre: Science
ISBN: 3662084880

This book, written by the designer of the worlds largest telescope, the VLT in Chile, covers the essential modern developments in telescope optics. In the last twenty years, modern technology has revolutionized not only manufacturing and test procedures but also the entire area of quality specification. In addition to these topics, the book also covers the alignment of telescope optics, atmospheric optics, adaptive optics, reflective coatings, and ancillary equipment. Richly illustrated, this work covers important modern techniques, which makes it one of the most complete references on telescope optics.