With the completion of the Hubble Space Telescope (HST) Key Project on the Extragalactic Distance Scale, it is interesting to form the dimensionless quantity H0t0 by multiplying the Hubble Constant by the age of the Universe. In a matter dominated decelerating Universe with a density exceeding 0.26 of the critical value, H0t0 < 1; in an accelerating Universe with the same Omega_m = 0.26, but dominated by vacuum energy with Omega_V >= 1 - Omega_m, H0t0 >= 1. If the first globular clusters formed 10^9 years after the Big Bang, then with 95% confidence H0t0 = 1.0 +-0.3. The classical Einstein-de Sitter cosmological model has H0t0 = 2/3
We present a measurement of the Hubble constant (H-0) and other cosmological parameters from a joint...
Strong gravitational lens systems with time delays between the multiple images are a powerful probe ...
Abstract The multi-messenger observations of GW170817 indicated a new independent measurement of the...
With the completion of the Hubble Space Telescope (HST) Key Project on the Extragalactic Distance Sc...
A brief history of the determination of the Hubble constant H_0 is given. Early attempts following L...
A brief history of the determination of the Hubble constant H0 is given. Early attempts following Le...
The story of the Hubble constant logically begins just where the Curtis-Shapley debate on the distan...
The "constant" H, whose customary units are (km/sec)/Megaparsecs, is a measure of the distance scale...
The Hubble constant sets the size and age of the Universe, and, together with independent determinat...
The Hubble constant, H-0, sets the scale of the size and age of the Universe and its determination f...
We determine the Hubble constant H0 precisely (2.3% uncertainty) in a manner independent of cosmolo...
International audienceContext. In relativistic inhomogeneous cosmology, structure formation couples ...
Recent observations of Cepheids in the Virgo cluster have bolstered the evidence that supports a Hub...
We present the first determination of the Hubble constant H-0 from strong lensing time delay data an...
An interesting way to calibrate the absolute magnitudes of remote Type Ia supernovae (SNe Ia) that a...
We present a measurement of the Hubble constant (H-0) and other cosmological parameters from a joint...
Strong gravitational lens systems with time delays between the multiple images are a powerful probe ...
Abstract The multi-messenger observations of GW170817 indicated a new independent measurement of the...
With the completion of the Hubble Space Telescope (HST) Key Project on the Extragalactic Distance Sc...
A brief history of the determination of the Hubble constant H_0 is given. Early attempts following L...
A brief history of the determination of the Hubble constant H0 is given. Early attempts following Le...
The story of the Hubble constant logically begins just where the Curtis-Shapley debate on the distan...
The "constant" H, whose customary units are (km/sec)/Megaparsecs, is a measure of the distance scale...
The Hubble constant sets the size and age of the Universe, and, together with independent determinat...
The Hubble constant, H-0, sets the scale of the size and age of the Universe and its determination f...
We determine the Hubble constant H0 precisely (2.3% uncertainty) in a manner independent of cosmolo...
International audienceContext. In relativistic inhomogeneous cosmology, structure formation couples ...
Recent observations of Cepheids in the Virgo cluster have bolstered the evidence that supports a Hub...
We present the first determination of the Hubble constant H-0 from strong lensing time delay data an...
An interesting way to calibrate the absolute magnitudes of remote Type Ia supernovae (SNe Ia) that a...
We present a measurement of the Hubble constant (H-0) and other cosmological parameters from a joint...
Strong gravitational lens systems with time delays between the multiple images are a powerful probe ...
Abstract The multi-messenger observations of GW170817 indicated a new independent measurement of the...