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Positional Encodings for Light Curve Transformers: Playing with Positions and Attention

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arxiv 2308.06404 v1 pith:NYFBYR4X submitted 2023-08-11 astro-ph.IM

classification astro-ph.IM
keywords attentiontransformercurvedatasetsencodingslightpositionalproposed
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We conducted empirical experiments to assess the transferability of a light curve transformer to datasets with different cadences and magnitude distributions using various positional encodings (PEs). We proposed a new approach to incorporate the temporal information directly to the output of the last attention layer. Our results indicated that using trainable PEs lead to significant improvements in the transformer performances and training times. Our proposed PE on attention can be trained faster than the traditional non-trainable PE transformer while achieving competitive results when transfered to other datasets.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. How Low Can We Go? Minimum Spectroscopic Requirements For Supernova Subtype Classification

    astro-ph.IM 2026-07 accept novelty 6.0 of 10

    ABC-SN classifies ten supernova subtypes with no performance loss down to R_λ=50 and SNR=5, and only minimal loss at R_λ=25.

  2. StarCLR: Contrastive Learning Representation for Astronomical Light Curves

    astro-ph.SR 2026-04 conditional novelty 6.0 of 10

    StarCLR pretrains on TESS light curves via contrastive learning on overlapping subsequences and improves variable star classification F1 scores over scratch-trained models when fine-tuned on TESS, ZTF, and Gaia.

  3. ABC-SN: Attention Based Classifier for Supernova Spectra

    astro-ph.IM 2025-07 conditional novelty 6.0 of 10

    ABC-SN, a transformer-based classifier, reaches 82.5% macro F1 on ten supernova subtypes, outperforming a retrained DASH at 58.9% on the same test set.

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