While the PSDLoss loss function essentially measures PSDR (or ASDR if asd=True), and this might function as a good proxy for DeepClean's ability to improve the sensitivity of astrophysical searches, there might be other loss functions out there which measure this more directly with continuous functions and hence be optimized via gradient descent.
Take for example equation (1) in the SenseMonitor white paper, which gives the average distance to which an interferometer with a given spectral density could detect a BNS inspiral with SNR > 8. The integral in this equation could be replace by a sum over the relevant frequency bins, with a minus sign in to minimize rather than maximize, and in principle we could optimize this equation directly.
This really asks three questions:
While the
PSDLossloss function essentially measures PSDR (or ASDR ifasd=True), and this might function as a good proxy for DeepClean's ability to improve the sensitivity of astrophysical searches, there might be other loss functions out there which measure this more directly with continuous functions and hence be optimized via gradient descent.Take for example equation (1) in the SenseMonitor white paper, which gives the average distance to which an interferometer with a given spectral density could detect a BNS inspiral with SNR > 8. The integral in this equation could be replace by a sum over the relevant frequency bins, with a minus sign in to minimize rather than maximize, and in principle we could optimize this equation directly.
This really asks three questions: