A PCA-based generalization of template matching corrects jitter noise in pulsar TOA measurements by modeling pulse shape variations.
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N-body simulations demonstrate that post-capture chaotic planet-planet interactions around pulsars can produce stable low-eccentricity orbits after ejections.
Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.
Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.
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A Generalized Template Matching Algorithm for Correcting Jitter Noise in Pulsar Timing
A PCA-based generalization of template matching corrects jitter noise in pulsar TOA measurements by modeling pulse shape variations.
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Scintillation of the first-known pulsar planetary system
Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.