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19932024
most citedThe Updated Zwicky Catalog (UZC)

474 citations · 11.4k across the 166 of their papers we have counts for

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Showing 2001Show all

7 papers · 1 filter

astro-ph2001★ 52 cited

Infrared Mass-to-Light Profile Throughout the Infall Region of the Coma Cluster

K. Rines, M. J. Geller, M. J. Kurtz +3

Using a redshift survey of 1779 galaxies and photometry from the 2-Micron All-Sky Survey (2MASS) covering 200 square degrees, we calculate independent mass and light profiles for t…

astro-ph2001★ 20 cited

Redshifts for 2410 Galaxies in the Century Survey Region

G. Wegner, J. R. Thorstensen, M. J. Kurtz +6

The `Century Survey' strip covers 102 square degrees within the limits 8.5h \leq α_{1950} \leq 16.5h, 29.0 degrees \leq δ_{1950} \leq 30.0 degrees. The strip passes through the Cor…

astro-ph2001★ 83 cited

Star Formation in a Complete Spectroscopic Survey of Galaxies

B. J. Carter, D. G. Fabricant, M. J. Geller +1

The 15R-North galaxy redshift survey is a uniform spectroscopic survey (S/N 10) covering the range 3650---7400Åfor 3149 galaxies with median redshift 0.05. The sample is 90%…

astro-ph2001★ 86 cited

The LX-sigma Relation for Galaxies and Clusters of Galaxies

Andisheh Mahdavi, Margaret J. Geller

We demonstrate that individual elliptical galaxies and clusters of galaxies form a continuous X-ray luminosity---velocity dispersion (LX-sigma) relation. Our samples of 280 cluster…

astro-ph2001★ 54 cited

V and R-band Galaxy Luminosity Functions and Low Surface Brightness Galaxies in the Century Survey

Warren R. Brown, Margaret J. Geller, Daniel G. Fabricant +1

We use 64 square degrees of deep V and R CCD images to measure the local V and R band luminosity function of galaxies. The V_0<16.7 and R_0<16.2 redshift samples contain 1250 galax…

astro-ph2001★ 19 cited

H-Band and Spectroscopic Properties of Abell 1644

Aaron W. Tustin, Margaret J. Geller, Scott J. Kenyon +1

We discuss H-band (1.65 micrometer) near-infrared photometry of the central 3x3h^{-2} Mpc^2 of Abell 1644 to a limiting M_H~M^*_H+3 (throughout this paper H_0=100 h km s^{-1} Mpc^{…