BBH waveform generated from Bilby can't tell the distance. We adjust its amplitude the same to Korean waveform's, then we can infer BBH waveform's distance(since we know all information of Korean waveform).
## (2)make injection
## (3)whiten signal
> The way forward is to whiten the signal generations and then add white noise to it. However, we are not sure what noise curve VItamin is expecting for the whitening.
> For Vitamin we would require the data to match the properties fo the training data. So regarding noise and whitening, I think Hunter is assuming Advanced design noise for LIGO and Virgo.
The way forward is to whiten the signal generations and then add white noise to it. So we need to know what noise curve VItamin is expecting for the whitening.
> For Vitamin we would require the data to match the properties fo the training data.
It’s important that your signals are whitened in the same way. We would expect the input data to then have whitened signal + Gaussian white noise of unit variance and zero mean.
> Hunter is using the aLIGO zero detuning, high power design sensitivity PSD found at the link below under the file titled "aLIGO_ZERO_DET_high_P_psd.txt". For Virgo the file is "AdV_psd.txt". These are the default noise curves used by bilby.
