First light for the first station of the long wavelength array
The first station of the Long Wavelength Array (LWA1) was completed in April 2011 and is
currently performing observations resulting from its first call for proposals in addition to a …
currently performing observations resulting from its first call for proposals in addition to a …
Modification of Large Reflector Antennas for Low Frequency Operation
M Harun - 2011 - vtechworks.lib.vt.edu
Modifications of large reflector antennas, such that their observing capabilities are enhanced
in the range of about 10-500~ MHz without affecting operation of the pre-existing higher …
in the range of about 10-500~ MHz without affecting operation of the pre-existing higher …
Imaging at both ends of the spectrum: the Long Wavelength Array and Fermi
GB Taylor, TLWA Collaboration - arXiv preprint arXiv:1206.1799, 2012 - arxiv.org
The Long Wavelength Array (LWA) will be a new multi-purpose radio telescope operating in
the frequency range 10-88 MHz. Scientific programs include pulsars, supernova remnants …
the frequency range 10-88 MHz. Scientific programs include pulsars, supernova remnants …
A Search for Astrophysical Radio Transients at Meter Wavelengths
S Cutchin - 2011 - vtechworks.lib.vt.edu
Astrophysical phenomena such as exploding primordial black holes (PBHs), gamma-ray
bursts (GRBs), compact object mergers, and supernovae, are expected to produce a single …
bursts (GRBs), compact object mergers, and supernovae, are expected to produce a single …
Absolute Flux Density Measurement and Associated Instrumentation for Radio Astronomy below 100 MHz
RH Tillman - 2016 - vtechworks.lib.vt.edu
This dissertation reports new measurements of the absolute flux densities of the brightest
astrophysical sources visible from the northern hemisphere with O [10%] accuracy between …
astrophysical sources visible from the northern hemisphere with O [10%] accuracy between …