149,086 research outputs found

    Montage : eine Bibliographie

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    Kompiliert von Hans J. Wulff Inhalt: 1. Montage 2. Montageexperiment

    The Montage Image Mosaic Service: Custom Image Mosaics On-Demand

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    The Montage software suite has proven extremely useful as a general engine for reprojecting, background matching, and mosaicking astronomical image data from a wide variety of sources. The processing algorithms support all common World Coordinate System (WCS) projections and have been shown to be both astrometrically accurate and flux conserving. The background ‘matching’ algorithm does not remove background flux but rather finds the best compromise background based on all the input and matches the individual images to that. The Infrared Science Archive (IRSA), part of the Infrared Processing and Analysis Center (IPAC) at Caltech, has now wrapped the Montage software as a CGI service and provided a compute and request management infrastructure capable of producing approximately 2 TBytes / day of image mosaic output (e.g. from 2MASS and SDSS data). Besides the basic Montage engine, this service makes use of a 16-node LINUX cluster (dual processor, dual core) and the ROME request management software developed by the National Virtual Observatory (NVO). ROME uses EJB/database technology to manage user requests, queue processing and load balance between users, and managing job monitoring and user notification. The Montage service will be extended to process userdefined data collections, including private data uploads

    Montage: a grid portal and software toolkit for science-grade astronomical image mosaicking

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    Montage is a portable software toolkit for constructing custom, science-grade mosaics by composing multiple astronomical images. The mosaics constructed by Montage preserve the astrometry (position) and photometry (intensity) of the sources in the input images. The mosaic to be constructed is specified by the user in terms of a set of parameters, including dataset and wavelength to be used, location and size on the sky, coordinate system and projection, and spatial sampling rate. Many astronomical datasets are massive, and are stored in distributed archives that are, in most cases, remote with respect to the available computational resources. Montage can be run on both single- and multi-processor computers, including clusters and grids. Standard grid tools are used to run Montage in the case where the data or computers used to construct a mosaic are located remotely on the Internet. This paper describes the architecture, algorithms, and usage of Montage as both a software toolkit and as a grid portal. Timing results are provided to show how Montage performance scales with number of processors on a cluster computer. In addition, we compare the performance of two methods of running Montage in parallel on a grid.Comment: 16 pages, 11 figure

    Vincente Minnelli : eine Bibliographie

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    Die meisten dieser Aufnahmen enstammen Katalogen und den Bibliographien aus Büchern über Minnelli. Eine erste Fassung der Bibliographie wurde als bibliographische Beilage der 'Montage / AV' (Beil. 1, 1993) vorgelegt

    The Application of the Montage Image Mosaic Engine To The Visualization Of Astronomical Images

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    The Montage Image Mosaic Engine was designed as a scalable toolkit, written in C for performance and portability across *nix platforms, that assembles FITS images into mosaics. The code is freely available and has been widely used in the astronomy and IT communities for research, product generation and for developing next-generation cyber-infrastructure. Recently, it has begun to finding applicability in the field of visualization. This has come about because the toolkit design allows easy integration into scalable systems that process data for subsequent visualization in a browser or client. And it includes a visualization tool suitable for automation and for integration into Python: mViewer creates, with a single command, complex multi-color images overlaid with coordinate displays, labels, and observation footprints, and includes an adaptive image histogram equalization method that preserves the structure of a stretched image over its dynamic range. The Montage toolkit contains functionality originally developed to support the creation and management of mosaics but which also offers value to visualization: a background rectification algorithm that reveals the faint structure in an image; and tools for creating cutout and down-sampled versions of large images. Version 5 of Montage offers support for visualizing data written in HEALPix sky-tessellation scheme, and functionality for processing and organizing images to comply with the TOAST sky-tessellation scheme required for consumption by the World Wide Telescope (WWT). Four online tutorials enable readers to reproduce and extend all the visualizations presented in this paper.Comment: 16 pages, 9 figures; accepted for publication in the PASP Special Focus Issue: Techniques and Methods for Astrophysical Data Visualizatio

    The ear against the eye : Vertov’s symphony

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    Vertov defined the basic qualities of his Cine-Eye by means of a simple negation: it sees what remains inaccessible to the human eye. This means that in his films we see media-based and media-produced images that have nothing to do with the imitation of human perception. According to Vertov, such filmic, telescopic, or microscopic perception develops, educates, and expands the viewer’s analytical abilities. Thus, we have on the one hand a media-induced perception and on the other a new assemblage or montage of the fragments of this mediated perception. This new montage is based on a specific interaction and follows poetic rather than prosaic rules. It is freed from such constraints as time, space, causality, or speed. In other words it is based on properly media-specific qualities and, following the terminology of the Russian Futurists who influenced Vertov in his youth, it constitutes zaum or transrationality

    MOSAIX: a tool to built large mosaics from GALEX images

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    Large sky surveys are providing a huge amount of information for studies of the interstellar medium, the galactic structure or the cosmic web. Setting into a common frame information coming from different wavelengths, over large fields of view, is needed for this kind of research. GALEX is the only nearly all-sky survey at ultraviolet wavelengths and contains fundamental information for all types of studies. GALEX field of view is circular embedded in a squared matrix of 3840 x 3840 pixels. This fact makes it hard to get GALEX images properly overlapped with the existing astronomical tools such as Aladin or Montage. We developed our own software for this purpose. In this article, we describe this software and makes it available to the community.Comment: 7 pages, including 8 figures, accepted by Astrophysics and Space Scienc

    Le montage : de la vision à l’action

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    Cet article a pour ambition de montrer en quoi le montage, que l'on décrit souvent comme l'essence du langage cinématographique, est un dispositif de médiation de la vision et de l'action. Walter Benjamin, en élargissant les analyses de Eisenstein sur le « montage des attractions », fut un des premiers théoriciens à souligner que le choc visuel du montage obligeait le spectateur à réagir sur le plan politique et à adopter un comportement progressiste.The aim of this article is to show how montage, often described as the essence of cinematographic language, constitutes an apparatus for the mediation of vision and action. Walter Benjamin, building on Eisenstein's analysis of the "montage of attractions," was one of the first theorists to stress that the visual shock of montage obliges the spectator to react politically and to adopt a progressive mode of behaviour
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