Automated Author ProfileWest, Jennifer
National Research Council of Canada
West, Jennifer
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets for this author
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the author's datasets
Total Mentions
Total mentions of the author's datasets
S-Index Interpretation
The S-Index (Sharing Index) is a comprehensive metric that represents the cumulative impact of all your datasets. It is calculated as the sum of Dataset Index scores across all your claimed datasets.
What it means:
- A higher S-index indicates greater overall impact of your datasets relative to typical datasets in their fields of research
- The S-Index grows as you add more datasets or as existing datasets gain more citations and mentions
- It provides a single number to track your research data impact over time
Current S-Index: 0.1 (sum of 1 dataset Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
This collection contains post-processed image cubes from the POlarization Sky Survey of the Universe’s Magnetism (POSSUM) Pilot 1 survey. These data products include Stokes IQU cubes and corresponding weight cubes for the 10 Pilot 1 survey ASKAP observations. These data are a combination of 10 separate but contiguous 36-beam observations centered on RA (J2000) 321.815° and Dec (J2000) −54.670°. Each field had an integration time of ten hours and the beams were formed in the closepack36 footprint. The survey was observed at full resolution at the ASKAP mid-band frequency range (1152 – 1439 MHz) and averaged to a 288 MHz bandwidth with 1-MHz channel width. The lower half of the band was discarded due to RFI, leaving only the upper 144 frequency channels (1295 – 1439 MHz). These cubes have been leakage corrected using a source based method that involves stacking the 10 observations beam by beam, and fitting residuals with Zernike polynomials to map intensity as a function of distance from the centre of the beam. The cubes have also been convolved to a common 13”x13” resolution across all channels.
Authors
- Ma, Yik Ki ;
- Vernstrom, Tessa ;
- Akahori, Takuya ;
- Thomson, Alec ;
- Anderson, Craig ;
- Sun, Xiaohui ;
- Taylor, Russ ;
- Van Eck, Cameron ;
- Harvey-Smith, Lisa ;
- Willis, Anthony ;
- West, Jennifer ;
- Stil, Jeroen ;
- Rudnick, Lawrence ;
- Raja, Wasim ;
- Purcell, Cormac ;
- O'Sullivan, Shane ;
- Mcclure-Griffiths, Naomi ;
- Leahy, J Patrick ;
- Landecker, Tom ;
- Heald, George ;
- Farnes, Jamie ;
- Carretti, Ettore ;
- Brown, Shea ;
- Gaensler, Bryan ;
- Vanderwoude, Shannon