2,209 research outputs found
The Public Archives at the NASA Michelson Science Center
This presentation describes the scientific data sets and user services accessible through the public archive at the Michelson Science Center (MSC). The MSC is charged by NASA with providing long-term data archiving capabilities for the Navigator Program, whose goal is to detect and characterize Earth like planets around stars other than the Sun. The archive makes extensive re-use of the component-based software architecture of the NASA IPAC Infrared Science Archive (IRSA). It also re-uses IRSAs Configuration Management system, user support tools, and development and data ingestion processes
The Role of Provenance Management in Accelerating the Rate of Astronomical Research
The availability of vast quantities of data through electronic archives has
transformed astronomical research. It has also enabled the creation of new
products, models and simulations, often from distributed input data and models,
that are themselves made electronically available. These products will only
provide maximal long-term value to astronomers when accompanied by records of
their provenance; that is, records of the data and processes used in the
creation of such products. We use the creation of image mosaics with the
Montage grid-enabled mosaic engine to emphasize the necessity of provenance
management and to understand the science requirements that higher-level
products impose on provenance management technologies. We describe experiments
with one technology, the "Provenance Aware Service Oriented Architecture"
(PASOA), that stores provenance information at each step in the computation of
a mosaic. The results inform the technical specifications of provenance
management systems, including the need for extensible systems built on common
standards. Finally, we describe examples of provenance management technology
emerging from the fields of geophysics and oceanography that have applicability
to astronomy applications.Comment: 8 pages, 1 figure; Proceedings of Science, 201
The Application of the Montage Image Mosaic Engine To The Visualization Of Astronomical Images
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
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Development of 2MASS Catalog Server Kit
We develop a software kit called "2MASS Catalog Server Kit" to easily
construct a high-performance database server for the 2MASS Point Source Catalog
(includes 470,992,970 objects) and several all-sky catalogs. Users can perform
fast radial search and rectangular search using provided stored functions in
SQL similar to SDSS SkyServer. Our software kit utilizes open-source RDBMS, and
therefore any astronomers and developers can install our kit on their personal
computers for research, observation, etc. Out kit is tuned for optimal
coordinate search performance. We implement an effective radial search using an
orthogonal coordinate system, which does not need any techniques that depend on
HTM or HEALpix. Applying the xyz coordinate system to the database index, we
can easily implement a system of fast radial search for relatively small (less
than several million rows) catalogs. To enable high-speed search of huge
catalogs on RDBMS, we apply three additional techniques: table partitioning,
composite expression index, and optimization in stored functions. As a result,
we obtain satisfactory performance of radial search for the 2MASS catalog. Our
system can also perform fast rectangular search. It is implemented using
techniques similar to those applied for radial search. Our way of
implementation enables a compact system and will give important hints for a
low-cost development of other huge catalog databases.Comment: 2011 PASP accepte
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Thesis (M.B.A.)--Boston University
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The NASA/IPAC Infrared Science Archive (IRSA) as a resource in supporting observatory operations
IRSA's scaleable and extensible architecture is inherited by new missions and data providers, and thus offers substantial cost savings to missions. It has built archives for the W.M. Keck Observatory & the Spitzer Space Telescope Legacy teams, among others. It provided archiving and databases support for 2MASS, when active, and will provide corresponding support for the forthcoming WISE mission. IRSA acts as a resource to projects and missions by advising on product design and providing tools for validating data products
The Montage Image Mosaic Service: Custom Image Mosaics On-Demand
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
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