| ... | ... | @@ -20,6 +20,10 @@ |
|
|
|
|GW170818|[config.ini](https://ldas-jobs.ligo-la.caltech.edu/~muhammed.saleem/SIQM-events/GW170818/lalinferencenest/IMRPhenomPv2threePointFivePN/config.ini) <br>[results page](https://ldas-jobs.ligo-la.caltech.edu/~nv.krishnendu/realevent_runs_31March2019/GW170818/)||
|
|
|
|
|GW170823|[config.ini](https://ldas-jobs.ligo-la.caltech.edu/~muhammed.saleem/SIQM-events/GW170823/lalinferencenest/IMRPhenomPv2threePointFivePN/config.ini) <br>[results page](https://ldas-jobs.ligo-la.caltech.edu/~nv.krishnendu/realevent_runs_31March2019/GW170823/)||
|
|
|
|
|
|
|
|
**Comments:**
|
|
|
|
- High mass signals: The Ks posterior (with symmetric Ks prior) peaks around zero in f_imr runs while they are mostly biased towards negative Ks in f_isco runs. This can attributed to the fact that for high mass signals the additional SNR coming from MR part helps breaking the degeneracies between parameters and results in more symmetric Ks posteriors.
|
|
|
|
- Low mass signals: The effect of f_imr vs f_isco is minor in low mass signals like GW151226 because the contribution from MR part is minor.
|
|
|
|
|
|
|
|
|
|
|
|
## O3
|
|
|
|
* S190412m [Link to the O3-TGR wiki](https://wiki.ligo.org/CBC/TestingGR/BHmimickerTestGW190412m)
|
| ... | ... | |
| ... | ... | |
