With ugrizY colors alone, an LSST-like catalog yields at best ~35% contamination and ~19% completeness for globular-cluster candidates; principal components help marginally, autoencoders do not.
Empirical comparison between autoencoders and traditional dimensionality reduction methods
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
In order to process efficiently ever-higher dimensional data such as images, sentences, or audio recordings, one needs to find a proper way to reduce the dimensionality of such data. In this regard, SVD-based methods including PCA and Isomap have been extensively used. Recently, a neural network alternative called autoencoder has been proposed and is often preferred for its higher flexibility. This work aims to show that PCA is still a relevant technique for dimensionality reduction in the context of classification. To this purpose, we evaluated the performance of PCA compared to Isomap, a deep autoencoder, and a variational autoencoder. Experiments were conducted on three commonly used image datasets: MNIST, Fashion-MNIST, and CIFAR-10. The four different dimensionality reduction techniques were separately employed on each dataset to project data into a low-dimensional space. Then a k-NN classifier was trained on each projection with a cross-validated random search over the number of neighbours. Interestingly, our experiments revealed that k-NN achieved comparable accuracy on PCA and both autoencoders' projections provided a big enough dimension. However, PCA computation time was two orders of magnitude faster than its neural network counterparts.
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The contribution of the color space in LSST-like photometry for the selection of extragalactic globular cluster candidates
With ugrizY colors alone, an LSST-like catalog yields at best ~35% contamination and ~19% completeness for globular-cluster candidates; principal components help marginally, autoencoders do not.