Python Speaker Diarization

Spectral Clustering Python

Speaker Diarization Spectral Clustering

• This repository deals with python speaker diarization, especially speaker clustering.
• Kaldi is required to fully perform the speaker diarization task.

Auto Tuning Spectral Clustering for SpeakerDiarization Using Normalized Maximum Eigengap

• Code for the IEEE Signal Processing Letters (SPL) paper "Auto-Tuning Spectral Clustering for SpeakerDiarization Using Normalized Maximum Eigengap"
• Spectral Clustering with auto tuning approach for speaker diarization tasks.
• Based on Kaldi binaries, python and bash script

Features of Auto-tuning NME-SC method

Auto-tuning NME-SC poposed method - g

• does not need to be tuned on dev-set. (Unlike PLDA-AHC)
• Only requires speaker embedding. (No PLDA or supervised method for distance measuring)
• also estimates the number of speakers in the given session.
• shows better performance than AHC+PLDA method in general. (See the below table)

Performance Table

• All the results are based on X-vector speaker embedding from [1]
• Cosine distance (COS) is used for distance measure. [2]

Track 1: Oracle VAD

System	CALLHOME	CHAES-eval	CH109	RT03(SW)
Callhome Diarization Xvector Model[1]	8.39%	24.27%	9.72%	1.73%
Spectral Clustering COS+B-SC	8.78%	4.4%	2.25%	0.88%
Auto-Tuning COS+NME-SC	7.29%	2.48%	2.63%	2.21%
Auto-Tuning COS+NME-SC Sparse-Search-20	7.24%	2.48%	2.00%	0.92%

Track 2: System VAD

• Based on the ASpIRE SAD Model to get SAD output.
• The performance is: Speaker Error(%) ( Total DER(%) )

System	CALLHOME	CHAES-eval	CH109	RT03(SW)
Callhome Diarization Xvector Model[1]	6.64% (12.96%)	1.45% (5.52%)	2.6% (6.89%)	0.99% (3.53%)
Spectral Clustering COS+B-SC[2]	6.91% (13.23%)	1.00% (5.07%)	1.46% (5.75%)	0.56% (3.1%)
Auto-Tuning COS+NME-SC[2]	5.41% (11.73%)	0.97% (5.04%)	1.32% (5.61%)	0.59% (3.13%)
Auto-Tuning COS+NMME-SC Sparse-Search-20	5.41% (11.73%)	0.97% (5.04%)	1.32% (5.61%)	0.59% (3.13%)

Datasets

CALLHOME NIST SRE 2000 (LDC2001S97):
CALLHOME American English Subset (CHAES) (LDC97S42): CH-109 (LDC97S42): RT03 (LDC2007S10) :

Reference

[1] Callhome Diarization Xvector Model
[2] Tae Jin Park et. al., Auto Tuning Spectral Clustering for SpeakerDiarization Using Normalized Maximum Eigengap, IEEE Singal Processing Letters, 2019

Getting Started

TLDR; One-click demo script

• virtualenv should be installed on your machine.
• run_demo_clustering.sh installs a virtualenv and runs spectral a clustering example.
• This script runs two utterances from CALLHOME dataset with precomputed segment files and affinity matrices in ./sample_CH_xvector folder.

source run_demo_clustering.sh

Prerequisites

• This repo is based on python 3.7.
• The mainly required python3 libraries:

joblib==0.14.0
numpy==1.17.4
scikit-learn==0.22
scipy==1.3.3
kaldi_io==0.9.1

• Kaldi is required to reproduce the numbers in the paper. Go to Kaldi install to install Kaldi software.
• Kaldi should be installed in your home folder ~/kaldi to be successfully loaded.
• You can still run the clustering algorithm without Kaldi by saving your affinity matrix into .npy.

Installing

You have to first have virtualenv installed on your machine. Install virtualenv with the following command:

sudo pip3 install virtualenv 

If you installed virtualenv, run the "install_venv.sh" script to make a virtual-env.

source install_venv.sh

This command will create a folder named "env_nmesc".

Usage Example

You need to prepare the followings:

1. Segmentation files in Kaldi style format:
   <segment_id> <utt_id> <start_time> <end_time>

ex) segments

iaaa-00000-00327-00000000-00000150 iaaa 0 1.5
iaaa-00000-00327-00000075-00000225 iaaa 0.75 2.25
iaaa-00000-00327-00000150-00000300 iaaa 1.5 3
...
iafq-00000-00272-00000000-00000150 iafq 0 1.5
iafq-00000-00272-00000075-00000225 iafq 0.75 2.25
iafq-00000-00272-00000150-00000272 iafq 1.5 2.72

3. Affinity matrix files in Kaldi scp/ark format: Each affinity matrix file should be N by N square matrix.
4. Speaker embedding files (optional): If you don't have affinity matrix, you can calculate cosine similarity ark files using ./sc_utils/score_embedding.sh

Running the python code with arguments:

python spectral_opt.py --distance_score_file $DISTANCE_SCORE_FILE \
                       --threshold $threshold \
                       --score-metric $score_metric \
                       --max_speaker $max_speaker \
                       --spt_est_thres $spt_est_thres \
                       --segment_file_input_path $SEGMENT_FILE_INPUT_PATH \
                       --spk_labels_out_path $SPK_LABELS_OUT_PATH \
                       --reco2num_spk $reco2num_spk 

Arguments:

• distance_score_file: A list of affinity matrix files.

# If you want to use kaldi .ark score file as an affinity matrix
DISTANCE_SCORE_FILE=$PWD/sample_CH_xvector/cos_scores/scores.scp

# If you want to use .npy numpy file as an affinity matrix
DISTANCE_SCORE_FILE=$PWD/sample_CH_xvector/cos_scores/scores.txt

Two options are available:

(1) scores.scp: Kaldi style scp file that contains the absolute path to .ark files and its binary address. Space separted <utt_id> and <path>.

ex) scores.scp

iaaa /path/sample_CH_xvector/cos_scores/scores.1.ark:5
iafq /path/sample_CH_xvector/cos_scores/scores.1.ark:23129
...

(2) scores.txt: List of <utt_id> and the absolute path to .npy files.
ex) scores.txt

iaaa /path/sample_CH_xvector/cos_scores/iaaa.npy
iafq /path/sample_CH_xvector/cos_scores/iafq.npy
...

• score-metric: Use 'cos' to apply for affinity matrix based on cosine similarity.
  ex)

score_metric='cos'

• max_speaker: If you do not provide oracle number of speakers (reco2num_spk), the estimated number of speakers is capped by max_speaker. Default is 8.

max_speaker=8

• threshold: Manually setup a threshold. We apply this threshold for all utterances. This should be setup in conjuction with spt_est_thres. ex)

threshold=0.05

• spt_est_thres: spt_est_thres $spt_est_thres \

# You can specify a threshold.
spt_est_thres='None'
threshold=0.05 

# Or you can use NMESC in the paper to estimate the threshold.
spt_est_thres='NMESC'
threshold='None'

# Or you can specify different threshold for each utterance.
spt_est_thres="thres_utts.txt"
threshold='None'

thres_utts.txt has a format as follows: <utt_id>

ex) thres_utts.txt

iaaa 0.105
iafq 0.215
...

• segment_file_input_path: "segments" file in Kaldi format. This file is also necessary for making rttm file and calculating DER.

segment_file_input_path=$PWD/sample_CH_xvector/xvector_embeddings/segments

ex) segments

iaaa-00000-00327-00000000-00000150 iaaa 0 1.5
iaaa-00000-00327-00000075-00000225 iaaa 0.75 2.25
iaaa-00000-00327-00000150-00000300 iaaa 1.5 3
...
iafq-00000-00272-00000000-00000150 iafq 0 1.5
iafq-00000-00272-00000075-00000225 iafq 0.75 2.25
iafq-00000-00272-00000150-00000272 iafq 1.5 2.72

• reco2num_spk: A list of oracle number of speakers. Default is 'None'. reco2num_spk $reco2num_spk

reco2num_spk='None'
reco2num_spk='oracle_num_of_spk.txt'

In the text file, you must include <utt_id> and <oracle_number_of_speakers>
ex) oracle_num_of_spk.txt

iaaa 2
iafq 2
iabe 4
iadf 6
...

Cosine similarity calculator script

Running the python code for cosine similarity calculation:

data_dir=$PWD/sample_CH_xvector
pushd $PWD/sc_utils
text_yellow_info "Starting Script: affinity_score.py"
./score_embedding.sh --cmd "run.pl --mem 5G" \
                     --score-metric $score_metric \
                      $data_dir/xvector_embeddings \
                      $data_dir/cos_scores 
popd

• cmd: This is for following the kaldi style argument.
• score-metric: Should be 'cos' for cosine similarity.

score_metric='cos'

• <src-embedding-dir>: Source embedding directory where xvector.scp and xvector.ark files are
• <out-dir>: Output directory. This script will create scores.1.ark file and scores.scp

Expected output result of one-click script

$ source run_demo_clustering.sh 
=== [INFO] The python_envfolder exists: /.../Auto-Tuning-Spectral-Clustering/env_nmesc 
=== [INFO] Cosine similariy scores exist: /.../Auto-Tuning-Spectral-Clustering/sample_CH_xvector/cos_scores 
=== [INFO] Running Spectral Clustering with .npy input... 
=== [INFO] .scp file and .ark files were provided
Scanning eig_ratio of length [19] mat size [76] ...
1  score_metric: cos  affinity matrix pruning - threshold: 0.105  key: iaaa Est # spk: 2  Max # spk: 8  MAT size :  (76, 76)
Scanning eig_ratio of length [15] mat size [62] ...
2  score_metric: cos  affinity matrix pruning - threshold: 0.194  key: iafq Est # spk: 2  Max # spk: 8  MAT size :  (62, 62)
Method: Spectral Clustering has been finished 
=== [INFO] Computing RTTM 
=== [INFO] RTTM calculation was successful. 
=== [INFO] NMESC auto-tuning | Total Err. (DER) -[ 0.32 % ] Speaker Err. [ 0.32 % ] 
=== [INFO] .scp file and .ark files were provided
1  score_metric: cos  affinity matrix pruning - threshold: 0.050  key: iaaa Est # spk: 2  Max # spk: 8  MAT size :  (76, 76)
2  score_metric: cos  affinity matrix pruning - threshold: 0.050  key: iafq Est # spk: 5  Max # spk: 8  MAT size :  (62, 62)
Method: Spectral Clustering has been finished 
=== [INFO] Computing RTTM 
=== [INFO] RTTM calculation was successful. 
=== [INFO] Threshold 0.05 | Total Err. (DER) -[ 20.57 % ] Speaker Err. [ 20.57 % ] 
Loading reco2num_spk file:  reco2num_spk
=== [INFO] .scp file and .ark files were provided
1  score_metric: cos  Rank based pruning - RP threshold: 0.0500  key: iaaa  Given Number of Speakers (reco2num_spk): 2  MAT size :  (76, 76)
2  score_metric: cos  Rank based pruning - RP threshold: 0.0500  key: iafq  Given Number of Speakers (reco2num_spk): 2  MAT size :  (62, 62)
Method: Spectral Clustering has been finished 
=== [INFO] Computing RTTM 
=== [INFO] RTTM calculation was successful. 
=== [INFO] Known Num. Spk. | Total Err. (DER) -[ 0.15 % ] Speaker Err. [ 0.15 % ] 

Authors

Tae Jin Park: inctrljinee@gmail.com, tango4j@gmail.com
Kyu J.
Manoj Kumar
Shrikanth Narayanan