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19982026
most citedThe Arecibo Legacy Fast ALFA Survey: I. Science Goals, Survey Design and Strategy

830 citations · 4.7k across the 131 of their papers we have counts for

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astro-ph2008★ 4 cited

An EVLA search for water megamaser emission in the submm galaxy SMM J16359+6612 at z=2.5

R. Edmonds, J. Wagg, E. Momjian +5

Using the Expanded Very Large Array, we have conducted a search for 22.2 GHz H2O megamaser emission in the strongly lensed submm galaxy, SMM J16359+6612 at z=2.517. This object is…

astro-ph2008★ 37 cited

The Arecibo Legacy Fast ALFA Survey VII: A Neutral Hydrogen Cloud Complex in the Virgo Cluster

Brian R. Kent, Kristine Spekkens, Riccardo Giovanelli +5

We present observations of an HI cloud complex most likely located in the Virgo galaxy cluster, first reported by Kent et al. (2007). The complex consists of five clouds, detected…

astro-ph2008★ 38 cited

LCDM Satellites and HI Companions - The Arecibo ALFA Survey of NGC 2903

J. A. Irwin, G. L. Hoffman, K. Spekkens +11

We have conducted a deep, complete HI survey, using Arecibo/ALFA, of a field centered on the nearby, isolated galaxy, NGC 2903, which is similar to the Milky Way in its properties.…

astro-ph2008★ 69 cited

Formation of a Quasar Host Galaxy through a Wet Merger 1.4 Billion Years after the Big Bang

Dominik A. Riechers, Fabian Walter, Christopher L. Carilli +2

We present high-resolution Very Large Array imaging of the molecular gas in the host galaxy of the high redshift quasar BRI 1335-0417 (z=4.41). Our CO(2-1) observations have a line…

astro-ph2008★ 35 cited

VLA and VLBA Observations of the Highest Redshift Radio-Loud QSO J1427+3312 at z = 6.12

E. Momjian, C. L. Carilli, I. D. McGreer

We present 8.4 GHz VLA A-array and 1.4 GHz VLBA results on the radio continuum emission from the highest redshift radio-loud quasar known to date, the QSO J1427+3312. The…

astro-ph2008★ 49 cited

Resolving distance ambiguities towards 6.7 GHz methanol masers

J. D. Pandian, E. Momjian, P. F. Goldsmith

Distances to most star forming regions are determined using kinematics, through the assumption that the observed radial velocity arises from the motion of the source with respect t…