... | ... | @@ -57,3 +57,29 @@ This outputs (p_NS, p_EMB, p_massgap) |
|
|
| ----------- | ------- | --------------------- | ------------- |
|
|
|
| M. Coughlin | ongoing | ligo.em-bright v1.1.0 | :x: |
|
|
|
| S. Antier | ongoing | ligo.em-bright v1.1.0 | :x: |
|
|
|
|
|
|
##Comments
|
|
|
|
|
|
- The code is running both from Coughlin and Antier condor https://git.ligo.org/emfollow/em-properties/em-bright/-/wikis/Mass-gap-review
|
|
|
- clf_kwargs = {'n_estimators':50, 'criterion':'gini', 'max_depth': 20, 'max_features': None, 'min_samples_leaf': 5, 'min_samples_split': 20} is consistent with "https://git.ligo.org/emfollow/em-properties/mass_gap/-/blob/main/mass_gap_grid_search.ipynb" parameters grid search
|
|
|
- Installation is very easy, thanks
|
|
|
- Lack of understanding of conf.ini :
|
|
|
--> executables : two times the same time, can you clarify ?
|
|
|
--> lack of understanding and comments in config_ini parameters
|
|
|
--> What is the definition of the snr here ?
|
|
|
--> Threshold of cfar : does it correspond to the FAR threshold for public alerts in O4 ? does it follow LL group definition ?
|
|
|
--> "weignts": distance : how the distance is calculated here by the NN ?
|
|
|
|
|
|
- Be careful on personal repositories present in the code
|
|
|
--> to run the classifier output_dir -i /home/sushant.sharma-chaudhary/O2-HL-rates-injections
|
|
|
or https://git.ligo.org/emfollow/em-properties/em-bright/-/merge_requests/41/diffs#0064bf8c2663d62fc40433c07c51bf36875714d1_162_192
|
|
|
lin 49 PACKAGE_DATA_LINKS["MASS_GAP.pickle"] = 'https://git.ligo.org/sushant.sharma-chaudhary/em-bright-gp/-/raw/massgap/ligo/em_bright/data/MASS_GAP.pickle'
|
|
|
|
|
|
- in the command em_bright_dag_writer
|
|
|
--> -- mass-gap option, what does it refers to ?
|
|
|
--> Layer em_bright_extract 39 1 --> where 39 comes to ? Arbitrary ?
|
|
|
|
|
|
- 120 m1 threshold discussed in https://git.ligo.org/emfollow/em-properties/mass_gap/-/blob/main/mass_gap_grid_search.ipynb
|
|
|
--> What is the value to set-up this threshold so high while astronomers are interesting for prompt observation in EM_bright objets and with mass-gap ? so 1< m2 < 3 ?
|
|
|
--> One suggestion would be to set a status as unknown when the rapid estimates clearly are deficient to avoid values that does not make sense.
|
|
|
--> For mid terme, one useful study would be to train the NN only with this interesting sub-set of injections ( 1< m2 < 3) |