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CYBERSKA
A Cyberinfrastructure platform to meet the needs of data intensive radio astronomy on route to the SKA |
Latest comments
Natasha Maddox on MIGHTEE expression of interest. (12 days ago): Hi Matt et al, Confirming I'm still interested, and still able to co-chair the...- Garret Cotter on MIGHTEE expression of interest. (14 days ago): Hi Matt & All, Just to confirm I am interetsed, with a view to looking at...
- Lourdes Verdes-Montenegro on MIGHTEE expression of interest. (52 days ago): Dear Matt, Russ, Ian. I am answering on behalf of AMIGA team. AMIGA core...
- Aprajita Verma on MIGHTEE expression of interest. (57 days ago): Dear Matt, Russ and Ian, I remain interested in being involved in MIGHTEE. My...
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MIGHTEE expression of interest.
Last updated 55 days ago by Renee Hlozek Comments (56)Hi Matt, Russ, Ian I'm interested in contributing to MIGHTEE, both in understanding/characterising radio transient sources in the data, and multi-wavelength studies of sources detected by e.g. microwave experiments. cheers Renée...Straw man MIGHTEE Observing Plan
Last updated 233 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 1336 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 1336 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 1774 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 1776 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 1742 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 1777 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 2035 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 2220 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...
