189 citations · 605 across the 19 of their papers we have counts for
18 papers
A Multifrequency Census of 100 Pulsars below 100 MHz with LWA: A Systematic Study of Flux Density, Spectra, Timing, Dispersion, Polarization, and Its Variation from a Decade of Observations
Pratik Kumar, Greg B. Taylor, Kevin Stovall +2
We present a census of 100 pulsars, the largest below 100 MHz, including 94 normal pulsars and six millisecond pulsars, with the Long Wavelength Array (LWA). Pulse profiles are det…
Pulsar Observations at Low Frequencies: Applications to Pulsar Timing and Solar Wind Models
P. Kumar, S. M. White, K. Stovall +2
Efforts are underway to use high-precision timing of pulsars in order to detect low-frequency gravitational waves. A limit to this technique is the timing noise generated by disper…
Detecting Pulsar Polarization below 100 MHz with the Long Wavelength Array
V. Dike, G. B. Taylor, J. Dowell +1
Using the first station of the Long Wavelength Array (LWA1), we examine polarized pulsar emission between 25 and 88 MHz. Polarized light from pulsars undergoes Faraday rotation as…
Discovery of a Pulsar Wind Nebula around B0950+08 with the ELWA
D. Ruan, G. B. Taylor, J. Dowell +3
With the Expanded Long Wavelength Array (ELWA) and pulsar binning techniques, we searched for off-pulse emission from PSR B0950+08 at 76 MHz. Previous studies suggest that off-puls…
Scattering study of Pulsars below 100 MHz using LWA1
Karishma Bansal, G. B. Taylor, Kevin Stovall +1
Interstellar scattering causes pulsar profiles to grow asymmetrically, thus affecting the pulsar timing residuals, and is strongest at lower frequencies. Different Interstellar med…
Modeling the Ionosphere with GPS and Rotation Measure Observations
J. B. Malins, S. M. White, G. B. Taylor +2
The ionosphere contributes time-varying Faraday Rotation (FR) to radio signals passing through it. Correction for the effect of the ionosphere is important for deriving magnetic fi…