A hierarchical pruning framework reduces the computational cost of fully coherent circular-orbit binary pulsar searches by up to 10 orders of magnitude, enabling sensitivity 3-5x better than acceleration searches.
Jankowski , author W
6 Pith papers cite this work, alongside 224 external citations. Polarity classification is still indexing.
representative citing papers
A search of repeating FRBs identifies RM flare candidates in FRB 20121102A, FRB 20201124A, and FRB 20180916B, suggesting such events may be common and tied to dynamic magneto-ionic environments.
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
uGMRT ranks as the best current instrument for cyclic spectroscopy of pulsars, with the 80-300 MHz band optimal for most of the 312 sources examined.
A multi-wavelength SKA1-Mid continuum survey of ~290 pc × 60 pc around Sgr A* plus decade-long NSC monitoring can address remnant, pulsar, massive-star, star-formation and magnetic-field science with one dataset.
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
citing papers explorer
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Coherent Signal Detection with Pruning -- I. Finding Short-Period Binary Pulsars in Circular Orbits
A hierarchical pruning framework reduces the computational cost of fully coherent circular-orbit binary pulsar searches by up to 10 orders of magnitude, enabling sensitivity 3-5x better than acceleration searches.
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A Search for Rotation Measure Flare Candidates in Repeating Fast Radio Bursts
A search of repeating FRBs identifies RM flare candidates in FRB 20121102A, FRB 20201124A, and FRB 20180916B, suggesting such events may be common and tied to dynamic magneto-ionic environments.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
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Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars
uGMRT ranks as the best current instrument for cyclic spectroscopy of pulsars, with the 80-300 MHz band optimal for most of the 312 sources examined.
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The Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid
A multi-wavelength SKA1-Mid continuum survey of ~290 pc × 60 pc around Sgr A* plus decade-long NSC monitoring can address remnant, pulsar, massive-star, star-formation and magnetic-field science with one dataset.
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Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.