Tuesday | Wednesday | Thursday | ||
9:00 – 10:30 | Arrival | using LAL waveforms (Schmidt/Khan) | Unit tests (Ohme) | |
NR Review (Husa) | ||||
NS-NR data format (Kastaun) | ||||
10:30 – 11:00 | Coffee | |||
11:00 – 13:00 | time series projections (Lovelace) | |||
Goals for the Workshop | NR Follow-up (NR + NS) (Pfeiffer / Dietrich) | Improving precessing phenomenological frequency domain models (Khan) | ||
Status & Future of the Waveform Group | ROM/ROQ (Pürrer) | Statistical Gravitational Waveform Models: What to Simulate Next? (Pürrer) | ||
Post-merger BNS waveform intro for BBH people (Kastaun) | ||||
Preliminary results of the BNS injection study (Lackey) | ||||
13:00 – 14:00 | Lunch | |||
14:00 – 16:00 | Waveform standards (BH + NS) (Hannam/Bernuzzi) | Group Structure & Communication (Buonanno) | Toward full parameter-space coverage (Haney) | |
Interface between PE & waveforms (Raymond) | Written guidelines for O3 (London) | Modular waveforms (Pratten) | ||
Code standards (Ohme) | Making coding & review easier | |||
16:00 – 16:30 | PE call | Coffee | ||
16:30 – 18:00 | Review of a first higher mode phenom model for spin-aligned BBH signals (London) | Closing | ||
Extending TaylorF2 with extra physical parameters including injection table io (Lee) | Progress report: Calibrating PhenomHM to numerical data (Husa) | |||
Effect of higher modes on parameter recovery : Improvements and comparisons (Kalaghatgi) | Towards including mode mixing in the ringdown phase of phenomenological binary black hole waveform models. (Johnson-McDaniel) | |||
Determining the binary orbital separation direction from NR waveforms (Hamilton) |
Format:
- Talks: Standard (conference-style) presentations with limited time for questions
- Parallel interactive small-group discussions: Time to split up into small groups to discuss specific topics and report results back to the full group
- Tutorials: Hands-on sessions with guided examples