Download ossi/utils.py from adollahamini1998/ScriptsForVoxBlink2: direct link, hf CLI and curl.
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https://huggingface.co/datasets/adollahamini1998/ScriptsForVoxBlink2/resolve/main/ossi/utils.py
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hf download hf://datasets/adollahamini1998/ScriptsForVoxBlink2/ossi/utils.py
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curl -L -o utils.py https://huggingface.co/datasets/adollahamini1998/ScriptsForVoxBlink2/resolve/main/ossi/utils.py
3.51 kB
| import numpy as np | |
| import pandas as pd | |
| import matplotlib.pyplot as plt | |
| import torch | |
| import torch.nn.functional as F | |
| def cosine(x,w): | |
| # x, w shape: [B, d], where B = batch size, d = feature dim. | |
| x_norm = F.normalize(x,dim=1) | |
| w_norm = F.normalize(w,dim=1) | |
| cos_sim = torch.mm(x_norm, w_norm.T).clamp(-1, 1) | |
| return cos_sim | |
| def compute_dir_far(Gfeat, Glabel, Pfeat, Plabel,): | |
| num_cls = Plabel[-1].item() | |
| # num_cls = Plabel[-1] | |
| temp = torch.zeros(num_cls, Gfeat.size(1)) | |
| for i in range(num_cls): | |
| mask = Glabel.eq(i) | |
| temp[i] = Gfeat[mask].mean(dim=0) # make embd vector | |
| Gfeat = temp.clone() | |
| num_cls = Plabel[-1].item() | |
| # num_cls = Plabel[-1] | |
| Umask = Plabel.eq(num_cls) | |
| Klabel = Plabel[~Umask] | |
| Kfeat = Pfeat[~Umask] | |
| Ufeat = Pfeat[Umask] | |
| # compute cosine similarity | |
| Kcos = cosine(Kfeat, Gfeat) | |
| Ucos = cosine(Ufeat, Gfeat) | |
| # get prediction & confidence | |
| Kconf, Kidx = Kcos.max(1) | |
| Uconf, _ = Ucos.max(1) | |
| corr_mask = Kidx.eq(Klabel) | |
| dir_far_tensor = torch.zeros(1000, 3) # intervals: 1000 | |
| for i, th in enumerate(torch.linspace(Uconf.min(), Uconf.max(), 1000)): | |
| mask = (corr_mask) & (Kconf > th) | |
| dir = torch.sum(mask).item() / Kcos.size(0) | |
| far = torch.sum(Uconf > th).item() / Ucos.size(0) | |
| dir_far_tensor[i] = torch.FloatTensor([th, dir, far]) # [threshold, DIR, FAR] for each row | |
| return dir_far_tensor | |
| def dir_at_far(dir_far_tensor,far): | |
| # deal with exceptions: there can be multiple thresholds that meets the given FAR (e.g., FAR=1.000) | |
| # if so, we must choose maximum DIR value among those cases | |
| abs_diff = torch.abs(dir_far_tensor[:,2]-far) | |
| minval = abs_diff.min() | |
| mask = abs_diff.eq(minval) | |
| dir_far = dir_far_tensor[mask] | |
| dir = dir_far[:,1].max().item() | |
| return dir | |
| # area under DIR@FAR curve | |
| def AUC(dir_far_tensor): | |
| auc = 0 | |
| eps = 1e-5 | |
| for i in range(dir_far_tensor.size(0)-1): | |
| if dir_far_tensor[i,1].ge(eps) and dir_far_tensor[i,2].ge(eps)\ | |
| and dir_far_tensor[i+1,1].ge(eps) and dir_far_tensor[i+1,2].ge(eps): | |
| height = (dir_far_tensor[i,1] + dir_far_tensor[i+1,1])/2 | |
| width = torch.abs(dir_far_tensor[i,2] - dir_far_tensor[i+1,2]) | |
| auc += (height*width).item() | |
| return auc | |
| def save_dir_far_curve(Gfeat, Glabel, Pfeat, Plabel, save_dir,save_name): | |
| cos_tensor = compute_dir_far(Gfeat, Glabel, Pfeat, Plabel, matcher='cos') | |
| cos_auc = AUC(cos_tensor) | |
| fig,ax = plt.subplots(1,1) | |
| ax.plot(cos_tensor[:,2], cos_tensor[:,1]) | |
| ax.set_xscale('log') | |
| ax.set_xlabel('FAR') | |
| ax.set_ylabel('DIR') | |
| ax.legend(['cos-AUC: {:.3f}'.format(cos_auc)]) | |
| ax.grid() | |
| fig.savefig(save_dir+'/'+save_name, bbox_inches='tight') | |
| def save_dir_res(Gfeat, Glabel, Pfeat, Plabel, save_pic, save_res, fars): | |
| cos_tensor = compute_dir_far(Gfeat, Glabel, Pfeat, Plabel) | |
| cos_auc = AUC(cos_tensor) | |
| fig,ax = plt.subplots(1,1) | |
| ax.plot(cos_tensor[:,2], cos_tensor[:,1]) | |
| ax.set_xscale('log') | |
| ax.set_xlabel('FAR') | |
| ax.set_ylabel('DIR') | |
| ax.legend(['cos-AUC: {:.3f}'.format(cos_auc)]) | |
| ax.grid() | |
| fig.savefig(save_pic, bbox_inches='tight') | |
| with open(save_res,'a') as f: | |
| for far in fars: | |
| dir= dir_at_far(cos_tensor,far=far) | |
| f.write("\tFAR=%.4f:\tDIR=%.4f\n"%(far,dir)) | |
| f.flush() | |