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19942021
most citedThe Arecibo Legacy Fast ALFA Survey: I. Science Goals, Survey Design and Strategy

830 citations · 14.7k across the 186 of their papers we have counts for

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Showing 1999Show all

8 papers · 1 filter

astro-ph1999

A Search for OH Megamasers at z > 0.1: Preliminary Results

J. Darling, R. Giovanelli

We report the discovery of 11 OH megamasers and one OH absorber, along with upper limits on the OH luminosity of 53 other luminous infrared galaxies at z > 0.1. The new megamasers…

astro-ph1999

The Convergence Depth of the Local Peculiar Velocity Field

Daniel A. Dale, Riccardo Giovanelli

We have obtained Tully-Fisher (TF) measurements for some 3000 late-type galaxies in the field and in 76 clusters distributed throughout the sky between 10 and 200\h Mpc. The cluste…

astro-ph1999★ 19 cited

Correlation Analysis of SFI Peculiar Velocities

S. Borgani, L. N. da Costa, I. Zehavi +5

We present results of a statistical analysis of the SFI catalog of peculiar velocities, a recently completed survey of spiral field galaxies with I-band Tully-Fisher distances (Hay…

astro-ph1999★ 92 cited

Seeking the Local Convergence Depth. V. Tully-Fisher Peculiar Velocities for 52 Abell Clusters

Daniel A. Dale, Riccardo Giovanelli, Martha P. Haynes +2

We have obtained I band Tully-Fisher (TF) measurements for 522 late-type galaxies in the fields of 52 rich Abell clusters distributed throughout the sky between 50 and 200\h Mpc. H…

astro-ph1999★ 41 cited

Seeking the Local Convergence Depth. IV. Tully-Fisher Observations of 35 Abell Clusters

Daniel A. Dale, Riccardo Giovanelli, Martha P. Haynes +2

We present Tully-Fisher observations for 35 rich Abell clusters of galaxies. Results from I band photometry and optical rotation curve work comprise the bulk of this paper. This is…

astro-ph1999★ 44 cited

No Hubble Bubble in the Local Universe

R. Giovanelli, Daniel Dale, Martha Haynes +2

Zehavi et al. (1998) have suggested that the Hubble flow within 70/h Mpc may be accelerated by the existence of a void centered on the Local Group. Its underdensity would be ~20 %,…