Figure 4:
Comparison of projections from multiple data sets using UMAP, UMAP in tensorflow, parametric UMAP, parametric UMAP with an autoencoder loss, parametric t-SNE, t-SNE, SCVIS, IVIS, PHATE, a VAE, an AE, and PCA. (a) Moons. (B) 3D buffalo. (c) MNIST, (d) Cassin's vireo song segments, (e) Mouse retina single-cell transcriptomes. (f) Fashion MNIST, (g) CIFAR10. The Cassin's vireo data set uses a dynamic time warping loss and an LSTM network for the encoder and decoder for the neural networks. The image data sets use a convnet for the encoder and decoder for the neural networks. The bison examples use a t-SNE perplexity of 500 and 150 nearest neighbors in UMAP to capture more global structure.

Comparison of projections from multiple data sets using UMAP, UMAP in tensorflow, parametric UMAP, parametric UMAP with an autoencoder loss, parametric t-SNE, t-SNE, SCVIS, IVIS, PHATE, a VAE, an AE, and PCA. (a) Moons. (B) 3D buffalo. (c) MNIST, (d) Cassin's vireo song segments, (e) Mouse retina single-cell transcriptomes. (f) Fashion MNIST, (g) CIFAR10. The Cassin's vireo data set uses a dynamic time warping loss and an LSTM network for the encoder and decoder for the neural networks. The image data sets use a convnet for the encoder and decoder for the neural networks. The bison examples use a t-SNE perplexity of 500 and 150 nearest neighbors in UMAP to capture more global structure.

Close Modal

or Create an Account

Close Modal
Close Modal