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Found 6 papers, 4 papers with code
Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays
Here we give a frequentist analysis of a very simple signal+noise model showing that the current lack of evidence for spatial correlations is consistent with the magnitude of the correlation coefficients for pairs of Earth-pulsar baselines in the array, and the fact that pulsar timing arraysbare most-likely operating in the intermediate-signal regime.
General Relativity and Quantum Cosmology
PMLB v1.0: An open source dataset collection for benchmarking machine learning methods
Motivation: Novel machine learning and statistical modeling studies rely on standardized comparisons to existing methods using well-studied benchmark datasets.
Is deep learning necessary for simple classification tasks?
providing a head-to-head comparison of AutoML and DL in the context of binary classification on 6 well-characterized public datasets, and (2.)
Realistic sensitivity curves for pulsar timing arrays
We construct realistic sensitivity curves for pulsar timing array searches for gravitational waves, incorporating both red and white noise contributions to individual pulsar noise spectra, as well as the effect of fitting to a pulsar timing model.
General Relativity and Quantum Cosmology Instrumentation and Methods for Astrophysics
An Acoustical Analogue of a Galactic-scale Gravitational-Wave Detector
By precisely monitoring the "ticks" of Nature's most precise clocks (millisecond pulsars), scientists are trying to detect the "ripples in spacetime" (gravitational waves) produced by the inspirals of supermassive black holes in the centers of distant merging galaxies.
Physics Education Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology
Sensitivity curves for searches for gravitational-wave backgrounds
We propose a graphical representation of detector sensitivity curves for stochastic gravitational-wave backgrounds that takes into account the increase in sensitivity that comes from integrating over frequency in addition to integrating over time.
Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology
