A thesis.
- Probably shouldn’t use characteristic strain for the plots
- Is equation 2.3 really in the right place?
- No formalism for how we expect a CBC signal to evolve in phase as well as amplitude
- Should I really call them spline surroagte models → just surrogate models?
This section should probably come after the section on detection.
- [ ] Add discussion of LIGO india
- [ ] Should add discussion of the LIGO India project here.
- [ ] Improve list of IMR and SEO versions
- [ ] Add discussion of SXS catalogue
- [ ] Waveform cartoon with inspiral merger ringdown marked on
- [ ] Discussion of tidal effects in NS
- [ ] Discussion of PN accurate waveforms
- [ ] Add a P-Pdot diagram, possibly with some of the O1/O2 data.
- [ ] Add a plot of the energy of the stochastic background.
- [X] Fix CCSN plot- this is just wrong.
- [ ] Complete discussion of search methods
- [X] Add a figure for the ad-hoc waveforms This plot should probably still be checked over however.
- [X] Add a figure for the supernova waveforms
- [ ] Add a very brief discussion of SN models
- [X] Complete the discussion of burst parameters
- [X] Complete the discussion of null streams
- Call characteristic squared “hrss”
- Encounter waveforms reference from Siong
- Supernova section needs work
- Consider changing the searches section to a transient one
- Fundamental search methods section
- Cartoon to illustrate the signal construction diagrams
- Make sure that coherent and incoherent diagrams visually distinct
- [X] Discuss calibration uncertainties
- [X] Various data formats required
- [X] Signal production process (signal → ant pattern → noise)
- [ ] APPENDIX: Example script for MDC production
- [ ] Add discussion of the sensitivity results from O1 and O2 MDCs.