Lesson 7 further discussion ✅

(Pushkar) #21

Hi All,

I am getting an error while doing learn.fit(40,lr) in lesson7-superres-gan notebook.

NameError Traceback (most recent call last)
----> 1 learn.fit(40,lr)

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/basic_train.py in fit(self, epochs, lr, wd, callbacks)
176 callbacks = [cb(self) for cb in self.callback_fns] + listify(callbacks)
177 fit(epochs, self.model, self.loss_func, opt=self.opt, data=self.data, metrics=self.metrics,
–> 178 callbacks=self.callbacks+callbacks)
180 def create_opt(self, lr:Floats, wd:Floats=0.)->None:

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/utils/mem.py in wrapper(*args, **kwargs)
102 try:
–> 103 return func(*args, **kwargs)
104 except Exception as e:
105 if (“CUDA out of memory” in str(e) or

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/basic_train.py in fit(epochs, model, loss_func, opt, data, callbacks, metrics)
78 cb_handler = CallbackHandler(callbacks, metrics)
79 pbar = master_bar(range(epochs))
—> 80 cb_handler.on_train_begin(epochs, pbar=pbar, metrics=metrics)
82 exception=False

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/callback.py in on_train_begin(self, epochs, pbar, metrics)
213 self.state_dict[‘n_epochs’],self.state_dict[‘pbar’],self.state_dict[‘metrics’] = epochs,pbar,metrics
214 names = [(met.name if hasattr(met, ‘name’) else camel2snake(met.class.name)) for met in self.metrics]
–> 215 self(‘train_begin’, metrics_names=names)
217 def on_epoch_begin(self)->None:

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/callback.py in call(self, cb_name, call_mets, **kwargs)
199 “Call through to all of the CallbakHandler functions.”
200 if call_mets: [getattr(met, f’on_{cb_name}’)(**self.state_dict, **kwargs) for met in self.metrics]
–> 201 return [getattr(cb, f’on_{cb_name}’)(**self.state_dict, **kwargs) for cb in self.callbacks]
203 def set_dl(self, dl:DataLoader):

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/callback.py in (.0)
199 “Call through to all of the CallbakHandler functions.”
200 if call_mets: [getattr(met, f’on_{cb_name}’)(**self.state_dict, **kwargs) for met in self.metrics]
–> 201 return [getattr(cb, f’on_{cb_name}’)(**self.state_dict, **kwargs) for cb in self.callbacks]
203 def set_dl(self, dl:DataLoader):

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/vision/gan.py in on_train_begin(self, **kwargs)
91 “Create the optimizers for the generator and critic if necessary, initialize smootheners.”
92 if not getattr(self,‘opt_gen’,None):
—> 93 self.opt_gen = self.opt.new([nn.Sequential(*flatten_model(self.generator))])
94 else: self.opt_gen.lr,self.opt_gen.wd = self.opt.lr,self.opt.wd
95 if not getattr(self,‘opt_critic’,None):

~/anaconda3/envs/fastai/lib/python3.7/site-packages/fastai/callback.py in new(self, layer_groups)
28 “Create a new OptimWrapper from self with another layer_groups but the same hyper-parameters.”
29 opt_func = getattr(self, ‘opt_func’, self.opt.class)
—> 30 split_groups = split_bn_bias(layer_groups)
31 opt = opt_func([{‘params’: trainable_params(l), ‘lr’:0} for l in split_groups])
32 return self.create(opt_func, self.lr, layer_groups, wd=self.wd, true_wd=self.true_wd, bn_wd=self.bn_wd)

NameError: name ‘split_bn_bias’ is not defined

I looked at the fastai source code, and it does not seem to be defined anywhere.
However, it is defined in the old fastai source code.

Anyone else face the same issue?


Developer chat
(Pierre Guillou) #22

Hi @pushkarneo, I’ve got the same error with fastai 1.0.43. Did you solve it?


(Pushkar) #23

Hi @pierreguillou, I did not.
I couldn’t spend much time on it.
But since the code for that function is present in old source code.
Try copying and pasting it in the new source code and running.

If you do try the above, lemme know how it goes.


(Pierre Guillou) #24

Hi @pushkarneo, @sgugger made the correction (cf post).



Hi, I would like to recheck with you the Model0 from the Human Numbers resource.

The code for Model0 on video differs from the code in Jupiter notebook with a tiny bit:

  • if x.shape[0]>1: (in video)
  • if x.shape[1]>1: (in Jupiter notebook)

As it turns out, I may set if True:, or I may completely remove the if branches and the result will be the same.

I created the counter to check how many times we enter the branch like this:

class Model0(nn.Module):
    def __init__(self):
        self.i_h = nn.Embedding(nv,nh)  # green arrow
        self.h_h = nn.Linear(nh,nh)     # brown arrow
        self.h_o = nn.Linear(nh,nv)     # blue arrow
        self.bn = nn.BatchNorm1d(nh)
        self.counter0 =0
        self.counter1 =0
        self.counter2 =0
    def forward(self, x):
        self.counter0 +=1
        h = self.bn(F.relu(self.i_h(x[:,0])))
        if x.shape[0]>1:            
            h = h + self.i_h(x[:,1])            
            h = self.bn(F.relu(self.h_h(h)))
        if x.shape[0]>2:
            h = h + self.i_h(x[:,2])
            h = self.bn(F.relu(self.h_h(h)))
        return self.h_o(h)

As it turns out these lines:


Will return:

torch.Size([64, 3])

Any feedback?


(Pierre Guillou) #26

Hi @jeremy. In the lesson 7, you show in the lesson7-wgan.ipynb notebook how to generate fake images of bathroom by training a WGAN.

The training set you use has 303125 images and you train your GAN within 30 epochs with a lr of 2e-4.

I did try to use the exact same code with mango images from ImageNet dataset that has only 1305 images (and about 500 after cleaning).

However, even after 100 epochs, the result is bad. I guess my issue is the size of my training dataset?
With you experience, what would be the minimum size for the training dataset of a WGAN? And how to choose the right lr? Thank you.

After 100 epochs (lr = 2e-4)

After 100 epochs (lr = 2e-3)




Any feedback on this tiny little issue?


(Thomas) #28

I would like to know how to use the models exposed in the human-numbers notebook to generate predictions.
As I can see, the batch_size is hard coded in the model, so If I want to predict a batch of size 1 (one prediction) it is not possible.
I am building an equivalent model to forecast time series, so given the N past values I would like to predict value N+1



I’m curious to know if anyone tried to pass that black hole picture through a superres network…


(Andreas) #30

I tried it, and the result is not too impressive:

However, it makes sense. The loss function was based on a pretrained ResNET34, where the training data didn’t have a lot of black hole images (or anything remotely similar). Training a model on pictures of planets, stars, etc. instead of cats might help too :stuck_out_tongue:

(It did however work extremely well on cats.)



Thanks for trying!


(Divyanshu Sharma) #32

Has any one used models from this GAN zoo https://github.com/eriklindernoren/PyTorch-GAN ? Is the implementation reliable and error free ?




In the notebook lesson7_superres, I am looking at the gram_matrix function output and have a hard time understanding why a certain result occurs on the diagonal. If I have a single unit vectors v_1 and and I do it’s inner product with itself <v_1, v_1>=cos\theta, knowing that the angle is 0, the value should be 1, mainly, the diagonal should be full of ones. Why is that not the case ?

def gram_matrix(x):
    n,c,h,w = x.size()
    x = x.view(n, c, -1)
    return (x @ x.transpose(1,2))/(c*h*w)

> tensor([[[0.0759, 0.0711, 0.0643],
           [0.0711, 0.0672, 0.0614],
           [0.0643, 0.0614, 0.0573]],

          [[0.0759, 0.0711, 0.0643],
           [0.0711, 0.0672, 0.0614],
           [0.0643, 0.0614, 0.0573]]])

Thank you in advance for your help :slight_smile:



sorry didnt look at the competition, but reading Jeremy’s comment…can spark be helpful in this situation? downsample?



Does anyone know where the lesson 7 Kaggle notebooks for superres, superres-imagenet, superres-gan and wgan are?


(Levi Ritchie) #36

I suspect, beyond just regular pictures of planets and stars, you’d need a large set of high-resolution images of celestial objects taken with the same kind of black hole spectroscopy. Especially gaseous objects, since I think that’s what we’re seeing in the black hole picture. Then, rather than blurring them with image compression, you’d need a function that approximates the blur of objects in space across a vast distance.

Unfortunately, I’m a few million bucks shy of a good radio telescope.