Abstract

We describe how the Grid enables new research possibilities in astronomy through multi‐wavelength images. To see sky images in the same pixel space, they must be projected to that space, a computer‐intensive process. There is thus a virtual data space induced that is defined by an image and the applied projection. This virtual data can be created and replicated with Planners and Replica catalog technology developed under the GriPhyN project. We plan to deploy our system (MONTAGE) on the U.S. Teragrid. Grid computing is also needed for ingesting data—computing background correction on each image—which forms a separate virtual data space. Multi‐wavelength images can be used for pushing source detection and statistics by an order of magnitude from current techniques; for optimization of multi‐wavelength image registration for detection and characterization of extended sources; and for detection …

Metadata

publication

Concurrency and Computation: Practice and Experience 15 (6), 539-549, 2003

year

2003

publication date

2003/5

authors

Roy Williams, Bruce Berriman, Ewa Deelman, John Good, Joseph Jacob, Carl Kesselman, Carol Lonsdale, Seb Oliver, Thomas A Prince

link

https://onlinelibrary.wiley.com/doi/abs/10.1002/cpe.715

resource_link

https://pegasus.isi.edu/wordpress/wp-content/papercite-data/pdf/williams2003image.pdf

journal

Concurrency and Computation: Practice and Experience

volume

15

issue

6

pages

539-549

publisher

John Wiley & Sons, Ltd.