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The Cepheid distance to NGC 5236 (M83) with the ESO Very Large Telescope
Cepheids have been observed in NGC 5236 (M83) using the Antu (Unit Telescope 1) 8.2 m telescope of the ESO Very Large Telescope with the Focal Reducer/Low Dispersion Spectrograph 1. Repeated imaging
Studies of the Virgo cluster. VI. Morphological and kinematical structure of the Virgo cluster
The structure of the Virgo cluster is analyzed on the basis of the positions, Hubble types, and radial velocities of 1277 Virgo cluster galaxies. The surface distribution of galaxies is considered
The Hubble Constant: A Summary of the Hubble Space Telescope Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
This is the final summary paper of our 15 yr program using the Hubble Space Telescope (HST) to determine the Hubble constant from the Cepheid-calibrated luminosity of Type Ia supernovae. Several
Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae Leading to a Fully Corrected Hubble Diagram to v < 30,000 km s–1
Photometric (BVI) and redshift data corrected for streaming motions are compiled for 111 "Branch-normal," four 1991T-like, seven 1991bg-like, and two unusual supernovae of Type Ia (SNe Ia). Color