activity
19972008
most citedWSRT Ultra-Deep Neutral Hydrogen Imaging of Galaxy Clusters at z=0.2, a Pilot Survey of Abell 963 and Abell 2192

92 citations · 217 across the 8 of their papers we have counts for

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astro-ph2008

Deconstructing Disk Velocity Distribution Functions in the Disk-Mass Survey

Kyle B. Westfall, Matthew A. Bershady, Marc A. W. Verheijen +2

We analyze integral-field ionized gas and stellar line-of-sight kinematics in the context of determining the stellar velocity ellipsoid for spiral galaxies observed by the Disk-Mas…

astro-ph20075 cited

HI imaging of Galaxy Clusters at z=0.2; a Pilot Survey of Abell 963 and Abell 2192

Marc Verheijen, Jacqueline van Gorkom, Arpad Szomoru +3

A pilot study with the powerful new backend of the Westerbork Synthesis Radio Telescope (WSRT) of two galaxy clusters at z=0.2 has revealed neutral hydrogen emission from 39 galaxi…

astro-ph2004

Galaxy Kinematics with SALT

Matthew A. Bershady, Marc A. W. Verheijen, David R. Andersen +2

The combination of dynamical and photometric properties of galaxies offers a largely un-tapped source of information on how galaxies assembled and where stars formed. Bi-dimensiona…

astro-ph2003

The Kinematics in the Cores of Low Surface Brightness Galaxies

R. A. Swaters, M. A. W. Verheijen, M. A. Bershady +1

Systematic effects on HI and Halpha long-slit observations make a measurement of the inner slope of the dark matter density distribution difficult to determine. Halos with constant…

astro-ph2002

WIYN Integral-Field Kinematics of Disk Galaxies

Matthew Bershady, Marc Verheijen, David Andersen

We have completed a new fiber array, SparsePak, optimized for low-surface-brightness studies of extended sources on the WIYN telescope. We are now using this array as a measuring e…

astro-ph2001

Reconciling Damped Ly-alpha Statistics and 21cm Studies at z=0

Martin Zwaan, Frank Briggs, Marc Verheijen

Blind 21cm surveys in the local universe have shown that the local HI mass density, Omega_HI, is dominated by luminous, high surface brightness, spiral galaxies. On the other hand,…