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OverviewThe importance of wide-field imaging in astronomy has never been so evident. The deep photographic surveys of the sky are nearing completion. The advent of large-format solid state detectors will provide further deep digital sky survey data. Optical surveys of the sky are being complemented by surveys in other wavebands of the electromagnetic spectrum, principally in the X-ray and near-infrared. The mass of digital data being gathered is driving the need for mass-storage archival capability, and for rapid capabilities in data acquisitioning and processing. New techniques are being developed to optimize the extraction of the information content. The quality and quantity of data now available to astronomers are enabling new breakthroughs in many fields, such as studies of the structure of our own galaxy and properties of nearby galaxies, the large-scale distribution of galaxies and the nature of the mass-content of the Universe. These facets of wide-field astronomy are brought together in this book. Full Product DetailsAuthor: H.T. MacGillivray , E.B. Thomson , Barry M. Lasker , I. Neill ReidPublisher: Springer Imprint: Springer Edition: 1994 ed. Volume: 161 Dimensions: Width: 15.50cm , Height: 4.60cm , Length: 23.50cm Weight: 1.533kg ISBN: 9780792328780ISBN 10: 0792328787 Pages: 760 Publication Date: 30 June 1994 Audience: College/higher education , Professional and scholarly , Postgraduate, Research & Scholarly , Professional & Vocational Format: Hardback Publisher's Status: Active Availability: Out of stock ![]() The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available. Table of ContentsOne: Wide-Field Sky Surveys and Patrols.- Two: Digital Detectors in Wide-Field Imaging.- Three: Photography In Wide-Field Imaging.- Four: Digitised Wide-Field Surveys.- Five: Image Detection, Cataloguing and Classification.- Six: Calibration: Astrometric and Photometric.- Seven: Archiving and Databases.- Eight: Solar System Surveys.- Nine: Galactic Structure.- Ten: The Magellanic Clouds.- Eleven: Local Group Dwarf Galaxies And Lsb Galaxies.- Twelve: Properties of Nearby Galaxies.- Thirteen: Properties and Clustering of Galaxies and Clusters.- Fourteen: Mapping The Large-Scale Structure.- Fifteen: Properties and Clustering of Objects at Large Redshifts.- Sixteen: Conference Summary and Resolutions.- IAU Symposium 161 Resolution: Photographic Plate Supply.- IAU Symposium 161 Resolution: The Future Of Sonneberg Observatory.- IAU Working Group On Wide-Field Imaging: Statement Of Goals.- Author Index.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |