189 citations · 1.5k across the 53 of their papers we have counts for
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Spectral index of the Galactic foreground emission in the 50-87 MHz range
Marta Spinelli, Gianni Bernardi, Hugh Garsden +4
Total-power radiometry with individual meter-wave antennas is a potentially effective way to study the Cosmic Dawn () through measurement of sky brightness arising from th…
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…
Observing Flare Stars Below 100 MHz with the LWA
Ivey Davis, Greg Taylor, Jayce Dowell
We observed the flare stars AD Leonis, Wolf 424, EQ Pegasi, EV Lacertae, and UV Ceti for nearly 135 hours. These stars were observed between 63 and 83 MHz using the interferometry…
Using the Long Wavelength Array to Search for Cosmic Dawn
Christopher DiLullo, Gregory B. Taylor, Jayce Dowell
The search for the spectral signature of hydrogen from the formation of the first stars, known as Cosmic Dawn or First Light, is an ongoing effort around the world. The signature s…
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…
Detection of Echoes in PSR B1508+55 at frequencies below 100 MHz using the LWA1
Karishma Bansal, Greg Taylor, Kevin Stovall +1
PSR B1508+55 is known to have a single component profile above 300 MHz. However, when we study it at frequencies below 100 MHz using the first station of the Long Wavelength Array,…