Customized chromatic noise models for 67 pulsars detect non-dispersive delays in 21 cases, alter achromatic noise inferences in 19, and enable solar wind density estimates over 1.5 cycles.
Paradigms in Physics 2.0
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
In 2016, the Department of Physics at Oregon State University began a process to revise our Paradigms in Physics curriculum for physics majors. We began with a colloquium to inform the department of our plans and request their assistance, followed by a survey of students and faculty as well as individual interviews with the faculty teaching each course. As we developed a plan to address student- and faculty-identified challenges in the curriculum, we met with each faculty member individually to explain and refine our proposal, which was unanimously approved by the faculty. Major changes include major changes to several courses (math methods, computational physics, modern physics, electronics, and classical mechanics), including the introduction of two sophomore-year courses designed specifically to help prepare students for their upper-division courses.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Customized chromatic noise models applied to NANOGrav 15 yr data raise the Bayes factor for Hellings-Downs GWB correlations by a factor of ~8, lower the amplitude to 2.1e-15, and increase the spectral index to 3.5.
citing papers explorer
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The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
Customized chromatic noise models for 67 pulsars detect non-dispersive delays in 21 cases, alter achromatic noise inferences in 19, and enable solar wind density estimates over 1.5 cycles.