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Classifying Pan-STARRS with (un)supervised learning

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Mission Overview

Classifying Pan-STARRS sources with unsupervised and supervised learning

This entry explores how to classify unresolved sources extracted from the Pan-STARRS survey. The PS1-STRM team used a convolutional neural network to classify sources into "galaxy", "qso" , "star" and "unsure" classes based on the observed source fluxes. Here we demonstrate how to use simple dimensionality reduction, as well as unsupervised and supervised classification algorithms (k-means and stochastic gradient descent, respectively), to reproduce these classifications. We then compare the performance of these models with the published results.

Data: The PS1-STRM HLSP

Notebook: Classifying Pan-STARRS sources with (un)supervised learning

Released: 2022年06月12日

Updated: 2022年06月12日

Tags: classification, 1d-data, unsupervised, supervised, PCA, tSNE, k-means, clustering

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Pan-STARRS mosaic image (credit: R. White, STScI / PS1 Science Consortium).

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