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ET-EMR workshop on geometry and noise feasibility

21 May 2026
Nikhef
Europe/Amsterdam timezone

Contribution List

23 / 23
1. Welcome - introduction - bidbook - ET symposium Aachen (and proxy to store background materials)
21/05/2026, 09:30
12. Opening: Why the triangle now?
21/05/2026, 10:00
13. Integral feasibility
21/05/2026, 10:20
17. Null stream theory and signal-space decomposition
21/05/2026, 10:40
2. Status of sensors; transient noise sources
21/05/2026, 10:40
18. Glitch mitigation with the null stream
21/05/2026, 11:00
3. Policy toward Datta sharing with ETC
21/05/2026, 11:00
19. Calibration with the null stream
21/05/2026, 11:20
4. Site Selection Criteria - SG1
21/05/2026, 11:20
5. Discussing the narrative at ET symposium
21/05/2026, 11:40
20. Uniform sky coverage and constraining polarisation
21/05/2026, 11:40
6. Correlated seismic and Newtonian noise at the EMR site —
21/05/2026, 13:00
7. Impact of correlated NN on SGWB searches
21/05/2026, 13:20
8. Newtonian noise cancellation: fusion sensor arrays and ML
21/05/2026, 13:40
9. Single-site advantage: coordinated NN mitigation in the triangle
21/05/2026, 14:00
10. Discussion: consolidating the seismology & NN arguments
21/05/2026, 14:20
21. Discussion: drafting the astrophysics section of the bidbook
21/05/2026, 15:00
14. Noise mitigation: Wiener filter and Neural Networks
21/05/2026, 15:00
22. Duty cycle and redundancy: quantitative science metrics
21/05/2026, 15:20
15. Our feedback on the paper of Jan Harms
21/05/2026, 15:20
16. Discussion
21/05/2026, 15:40
23. Infrastructure risk and single-site containment
21/05/2026, 15:40
11. Publication and dissemination plan
21/05/2026, 16:00

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