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CYBERSKA
A Cyberinfrastructure platform to meet the needs of data intensive radio astronomy on route to the SKA |
Latest comments
Russ Taylor on Observations and Observing (1198 days ago): March observations Start (AST) | LST | Length...- Russ Taylor on Observations and Observing (1243 days ago): Scheduled...
- Marijke Haverkorn on SKA1 Key science in cosmic magnetism (1708 days ago): Hi Russ, Even though the Milky Way may not be a separate science driver, I...
- Russ Taylor on SKA1 Key science in cosmic magnetism (1720 days ago): Frederica: I was not my intention to recommend a wide-area survey with...
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All site pages
Straw man MIGHTEE Observing Plan
Last updated 107 days ago by Russ TaylorThe MIGHTEE observing plan consists of two-tiers. A mid-tier and a deep-tier. Deep-tier The deep tier will be done commensally with the LADUMA project (deep HI emission). LADUMA will observe one primary beam of MeerKAT for 5000 hours,...License information
Last updated 1210 days ago by David AikemaElgg, DMS, and the CyberSKA image viewer are licensed under the GPL v2.0 (http://www.cyberska.org/LICENSE.txt). The CyberSKA image viewer is built upon the PureWeb SDK, available under license from Calgary Scientific.Release notes
Last updated 1210 days ago by David AikemaThe Elgg core was upgraded from 1.7.15 to 1.8.19, which represented a major upgrade for Elgg and included major changes to the internal Elgg API, requiring plugins created or modified for the CyberSKA platform to be updated or in some cases...CyberSKA Image Viewer User Documentation
Last updated 1648 days ago by Pavol FederlUser documentation for CyberSKA Image Viewer There is also a screencast video of Pavol using the viewer.Links to demo files
Last updated 1649 days ago by Demo 2013Spectral image cube of atomic hydrogen emission in the plane of our Milky Way Galaxy. The dimensions of the cube are 3424x1824 pixels x 222 channels, or approximately 5.5GB. http://www.cyberska.org/pg/file/read/30241/supermosaic8fits GALFACTS...Output of SAD source finding challenge
Last updated 1615 days ago by Russ TaylorAIPS SAD was run on the three challenge data images. The run was carred out by Larry. Due to the limit on the number of sources that can be fit, Larry split the the challenge 1 and 2 images into east and west portions and ran SAD...SKA1 Key science in cosmic magnetism
Last updated 1651 days ago by Russ Taylor Comments (7)Hi all,Here is a first cut at characterizing core cosmic magnetism science goals in the SKA1 era. It is based on the submission from a few individuals over the past few days, folded in with my own thoughts. So to some degree this...Canadian SKA Industry Association Meeting - Feb 2013
Last updated 1909 days ago by Russ TaylorPresentations Morning: SKA Update and the Canadian SKA Program Welcome (Frank Maurer) Big Data and Analytics at the University of Calgary (Frank Maurer) SKA Overview and update (Russ Taylor) Preconstruction RFP...RFI flagging comparison between RFLAG , TFCROP in CASA and the LOFAR flagger for 610 MHz ELAIS N1...
Last updated 2094 days ago by Preshanth Jagannathan Comments (1)In CASA 3.4 the old flagdata and flagdata2 tools have been replaced by the tool tflagdata. Tflagdata offers two different flagging algorithms namely tfcrop and rflag. Tfcrop is a thresholding alogrithm while Rflag is an implementation of the...Server-side Data Visualization
Last updated 2326 days ago by Arne GrimstrupA Web-based Tool for Remote Visualization of Large Multi-dimensional Radio Astronomy Data Sets The visualization tool provides users the ability to interactively explore large multi-dimensional radio astronomy data sets directly in the browser,...
