| [Nathan K. Johnson-McDaniel](https://git.ligo.org/nathan-johnson-mcdaniel) | Choice on ending frequency of the $`22-`$mode track | To be updated | [Link](https://git.ligo.org/soumen.roy/o3inspiralhom/wikis/overelap33) | Soumen | Haris: for S190412m the overlaps between $`S(\alpha)`$ for 22 and 33 modes are less than 3% for ending frequencies<0.6f_ISCO. We need to check for S190814bv also. | Nathan: :x: , Haris: :x: |
| [Haris K](https://git.ligo.org/haris-k), [Nathan K. Johnson-McDaniel](https://git.ligo.org/nathan-johnson-mcdaniel) | Comparison of PSDs between Welch and BayesLine | DONE | [Link](https://git.ligo.org/soumen.roy/o3inspiralhom/wikis/PSDs-comparison) | Soumen | Haris: PSDs look consistent for detection purposes. Nathan: PSDs are not exactly the same, but have the same general amplitude. However, the GW190814 BayesLine PSD appears to be from 60 Hz-subtracted data, while the Welch PSD for that event and both PSDs for GW190412 have the 60 Hz line present. This should be sorted out. | Nathan: :x:, Haris: :heavy_check_mark: |
| [Haris K](https://git.ligo.org/haris-k), [Nathan K. Johnson-McDaniel](https://git.ligo.org/nathan-johnson-mcdaniel) | Study on choice of deltaT and deltaF | Done | [Link](https://git.ligo.org/soumen.roy/o3inspiralhom/-/wikis/Study-on-choice-of-deltaT-and-deltaF) | Soumen | Haris: $`Y(\alpha)`$ is defined as the sum of energy content of the pixels along the $`\alpha`$ track. Thus it will depend on the pixel size. However, the final $`\beta`$ will be independent of the choice of pixel size. Further, for sample rates<=4KHz, the spectrograms seem to be consistent for various choices of the sampling rate. The analysis is restricted to sample rates<=4KHz | Nathan: :x:, Haris: :x: |
| [Haris K](https://git.ligo.org/haris-k), [Nathan K. Johnson-McDaniel](https://git.ligo.org/nathan-johnson-mcdaniel) | Study on choice of deltaT and deltaF | Done | [Link](https://git.ligo.org/soumen.roy/o3inspiralhom/-/wikis/Study-on-choice-of-deltaT-and-deltaF) | Soumen | Haris: $`Y(\alpha)`$ is defined as the sum of energy content of the pixels along the $`\alpha`$ track. Thus it will depend on the pixel size. However, the final $`\beta`$ will be independent of the choice of pixel size. Further, for sample rates<=4KHz, the spectrograms seem to be consistent for various choices of the sampling rate. The analysis is restricted to sample rates<=4KHz | Nathan: :x:, Haris: :heavy_check_mark: |
| [Haris K](https://git.ligo.org/haris-k), [Nathan K. Johnson-McDaniel](https://git.ligo.org/nathan-johnson-mcdaniel) | Study on $`p-`$value | Done | [Link](https://git.ligo.org/soumen.roy/o3inspiralhom/-/wikis/Study-on-p-value) | Soumen | Extrapolation of $`P(\beta\|H_0)`$ doesn't seem to be a good idea. Will use background samples to quote an upper bound on *p*-value | :heavy_check_mark: |
...
...
@@ -74,7 +74,7 @@ We performed a set of investigations on the analysis to check it's efficiency.
| Script | Short description | Status | git hash | Comment | final sign-off |
| [test_insphom_GW190412_C01.sh](https://git.ligo.org/soumen.roy/o3inspiralhom/blob/master/GW190412/analysis/C01/test_insphom_GW190412_C01.sh) | Bash script to produce results (h5 file) for the event GW190412m | Done | 8e5b4c8ee8fafc512ede902c4e8101d004775ec8 | Haris: In future, the choice of `track-max-length` can be optimized to get maximum SNR | Nathan: :x: , Haris: :heavy_check_mark: |
| [ReadResults.ipynb](https://git.ligo.org/soumen.roy/o3inspiralhom/blob/master/GW190412/analysis/C01/ReadResults.ipynb) | Notebook used for producing final plots for GW190412 from `h5` file | Done | 16d4c1376dbd0805383ec027d1988fe8a6be511d | Haris: It would be better if you can place the colorbar in the spectrogram on the top pf the pannel horozontaly. Location of data file: /home/soumen.roy/HHM/o3inspiralhom/inspiral_hom_contribution/GW190412/C01/S190412m_L1_C01_0p6fISCO_0p45.h5 in CIT cluster | Nathan: :x: , Haris: :heavy_check_mark: |
| [ReadResults.ipynb](https://git.ligo.org/soumen.roy/o3inspiralhom/blob/master/GW190412/analysis/C01/ReadResults.ipynb) | Notebook used for producing final plots for GW190412 from `h5` file | Done | | Haris: It would be better if you can place the colorbar in the spectrogram on the top pf the pannel horozontaly. Location of data file: /home/soumen.roy/HHM/o3inspiralhom/inspiral_hom_contribution/GW190412/C01/S190412m_L1_C01_0p6fISCO_0p45.h5 in CIT cluster | Nathan: :x: , Haris: :x: |
Below is the summary of investigations to test the S190412m results.
