Automated Author ProfileStaveley-Smith, Lister
University of Western Australia, Australia
Staveley-Smith, Lister
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: 31.8 (sum of 116 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
We have re-processed all the observations in the Parkes pulsar data archive obtained during the first four years of the Parkes multibeam receiver and have developed a new artificial intelligence (AI) algorithm to investigate huge volume of candidates. Except for our previous detections, the latest results include 87 new fast radio burst (FRB) candidates with S/N above 7. These signals were only detected in a single beam of the receiver suggesting that they are unlikely to be terrestrial. Their dispersion measure (DM) excesses over the estimated Galactic DM place them at extragalactic distances. Using the Ultra Wideband Low (UWL) receiver we have opportunity to detect repeating signals from some of these FRB candidates. As all these signals were detected in the 20 cm band, the UWL provides the opportunity to observe stronger emission in other observing bands.
Authors
- Zhang, Songbo ;
- Manchester, D ;
- Staveley-Smith, Lister ;
- Hobbs, George ;
- Dai, Shi ;
- Russell, Christopher ;
- Wu, Xuefeng ;
- Luo, Rui ;
- Li, Ye ;
- Wei, Junjie ;
- Yang, Xuan ;
- Tang, Zhenfan ;
- Chang, Chenming ;
- Geng, Jinjun
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning the National Facility observing modes for the wide-band receiver and the cryoPAF.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew ;
- Hafner, Anita
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning the National Facility observing modes for the wide-band receiver and the cryoPAF.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew ;
- Hafner, Anita
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning the National Facility observing modes for the wide-band receiver and the cryoPAF.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew ;
- Hafner, Anita
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning the National Facility observing modes for the wide-band receiver and the cryoPAF.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew ;
- Hafner, Anita
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. In particular for commissioning the National Facility observing modes for the wide-band receiver and the cryoPAF.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew ;
- Hafner, Anita
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Shannon, Ryan ;
- Kaczmarek, Jane ;
- Dai, Shi ;
- Zic, Andrew
The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. The scheduled time is used to measure beam shapes, determine polarisation calibration solutions and commission the National Facility observing modes for the new wide-band receiver.
Authors
- Hobbs, George ;
- Manchester, Dick ;
- Staveley-Smith, Lister ;
- Green, James ;
- Johnston, Simon ;
- Sarkissian, John ;
- Reynolds, John ;
- Mader, Stacy ;
- van Straten, Willem ;
- Jameson, Andrew ;
- Cameron, Andrew ;
- Shannon, Ryan ;
- Zic, Andrew