TL;DR
This paper demonstrates that pre-trained vision Transformers, when applied to images of multi-band light curves, can effectively classify astronomical phenomena, outperforming specialized light curve models in several datasets.
Contribution
It introduces a novel image-based approach using pre-trained vision Transformers for light curve classification, eliminating the need for feature extraction or multi-band preprocessing.
Findings
SwinV2 achieved an 80.2 F1-score on MACHO dataset.
Adding a second band increased the F1-score to 84.1.
SwinV2 slightly outperformed existing models like Astromer and ATAT.
Abstract
This study investigates the potential of a pre-trained vision Transformer (VT) model, specifically the Swin Transformer V2 (SwinV2), to classify photometric light curves without the need for feature extraction or multi-band preprocessing. The goal is to assess whether this image-based approach can accurately differentiate astronomical phenomena and serve as a viable option for working with multi-band photometric light curves. We transformed each multi-band light curve into an image. These images serve as input to the SwinV2 model, which is pre-trained on ImageNet-21K. The datasets employed include the public Catalog of Variable Stars from the Massive Compact Halo Object (MACHO) survey, using both one and two bands, and the first round of the recent Extended LSST Astronomical Time-Series Classification Challenge (ELAsTiCC), which includes six bands. The performance of the model was…
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