Open Polarolouis opened 2 weeks ago
Currently with our implementation we are limited to scalar alpha values.
Following an approach like GrossSBM/sbm with fit$theta$mean, fit$theta$var etc. This would allow us to handle multinomial or gaussian emission distribution.
fit$theta$mean
fit$theta$var
Currently with our implementation we are limited to scalar alpha values.
Following an approach like GrossSBM/sbm with
fit$theta$mean
,fit$theta$var
etc. This would allow us to handle multinomial or gaussian emission distribution.