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19952023
most citedFinal Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

3.3k citations · 35.1k across the 237 of their papers we have counts for

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astro-ph2000★ 3.3k cited

Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

W. L. Freedman, B. F. Madore, B. K. Gibson +12

We present here the final results of the Hubble Space Telescope Key Project to measure the Hubble constant. We summarize our method, the results and the uncertainties, tabulate our…

astro-ph2000★ 1 cited

Evolution of Cluster Early-Type Galaxies

P. G. van Dokkum, M. Franx, D. D. Kelson +2

The slow evolution of the M/L ratios, colors, and line strengths of cluster early-type galaxies to z=1 suggests that their stars were formed at very high redshift. At the same time…

astro-ph2000

Type Ia Supernovae and the Value of the Hubble Constant

Brad K. Gibson, Chris B. Brook

The methodology involved in deriving the Hubble Constant via the calibration of the corrected peak luminosities of Type Ia supernovae (SNe) is reviewed. We first present a re-analy…

astro-ph2000★ 1 cited

Galaxies at High Redshift

Garth Illingworth

Within just the last few years, we have advanced from knowing only a few galaxies at z>2 to having redshifts for nearly 1000 z~2-5 objects. The majority of this sample has been det…

astro-ph2000★ 14 cited

Formation and Evolution of E and S0 Galaxies from HST and Keck Studies of z~0.3-1 Clusters

Garth Illingworth, Daniel Kelson, Pieter van Dokkum +1

We have witnessed a dramatic increase over the last five years in results on distant galaxies, in large part because of the high resolution imaging capability of HST, and the multi…

astro-ph2000★ 280 cited

HST Photometry and Keck Spectroscopy of the Rich Cluster MS1054-03: Morphologies, Butcher-Oemler Effect and the Color-Magnitude Relation at z=0.83

Pieter G. van Dokkum, Marijn Franx, Daniel Fabricant +2

We present a study of 81 I selected, spectroscopically-confirmed members of the X-ray cluster MS1054-03 at z=0.83. Redshifts and spectral types were determined from Keck spectrosco…