This independent survey utilizes the ATNF Pulsar Catalogue (v2. 70) to map physical anomalies across 1, 522 pulsars. By establishing a mathematical baseline (R²=1. 0) and applying a Z-score filtering framework, the study identifies high-sigma outliers, including an 11. 41-sigma Alpha candidate (J0952-0607). The Results demonstrate a scalable, automated framework for prioritizing relativistic targets in large-scale astrophysical datbases like the Square Kilometre Array (SKA).
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Anubhuti Kaushal
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Anubhuti Kaushal (Thu,) studied this question.
synapsesocial.com/papers/69abc2075af8044f7a4eb29d — DOI: https://doi.org/10.5281/zenodo.18877589