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20032008
most citedThe VLBA Imaging and Polarimetry Survey at 5 GHz

219 citations · 362 across the 10 of their papers we have counts for

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12 papers · 1 filter

astro-ph200814 cited

The dependence of HII region properties on global and local surface brightness within galaxy discs

J. F. Helmboldt, R. A. M. Walterbos, G. D. Bothun +2

Using B, R, and H-alpha images of roughly equal-sized samples of low surface brightness (LSB) and high surface brightness (HSB) galaxies (~40 galaxies apiece), we have explored the…

astro-ph200816 cited

A shrinking Compact Symmetric Object: J11584+2450?

S. E. Tremblay, G. B. Taylor, J. F. Helmboldt +2

We present multi-frequency multi-epoch Very Long Baseline Array (VLBA) observations of J11584+2450. These observations clearly show this source, previously classified as a core-jet…

astro-ph20089 cited

Current star formation in early-type galaxies and the K+A phenomenon

J. F. Helmboldt, R. A. M. Walterbos, T. Goto

We present the results of an effort to identify and study a sample of the likely progenitors of elliptical (E) and lenticular (S0) K+A galaxies. To achieve this, we have searched a…

astro-ph20084 cited

A Statistical Description of AGN Jet Evolution from the VLBA Imaging and Polarimetry Survey (VIPS)

J. F. Helmboldt, G. B. Taylor, R. C. Walker +1

A detailed analysis of the evolution of the properties of core-jet systems within the VLBA Imaging and Polarimetry Survey (VIPS) is presented. We find a power-law relationship betw…

astro-ph200743 cited

Characteristics of EGRET Blazars in the VLBA Imaging and Polarimetry Survey (VIPS)

G. B. Taylor, S. E. Healey, J. F. Helmboldt +12

We examine the radio properties of EGRET-detected blazars observed as part of the VLBA Imaging and Polarimetry Survey (VIPS). VIPS has a flux limit roughly an order of magnitude be…

astro-ph200724 cited

Radio Frequency Spectra of 388 Bright 74 MHz Sources

J. F. Helmboldt, N. E. Kassim, A. S. Cohen +2

As a service to the community, we have compiled radio frequency spectra from the literature for all sources within the VLA Low Frequency Sky Survey (VLSS) that are brighter than 15…