5 pages, 1 figure. Submitted to MNRASThe Hubble parameter H0 is still not very well measured. Although the Hubble Key Project, Chandra and WMAP gave good estimates, the uncertainties remain quite large. In this brief report, we suggest an original and independent method to derive a lower limit on H0 using the absorption of very high energy gamma-rays by the cosmic infrared background. With conservative hypothesis, we obtain H0>74 km/s/Mpc at the 68% confidence level, which favors the upper end of the intervals allowed by dedicated experiments
By coupling observations of type Ia supernovae with results obtained from the best available numeric...
In the model of low-energy quantum gravity by the author, the ratio H(z)/(1 + z) should be equal to...
An extraordinary number of Hubble constant measurements challenges physicists with selection of the ...
5 pages, 1 figure. Submitted to MNRASThe Hubble parameter H0 is still not very well measured. Althou...
The Hubble parameter H0 is still not very well measured. Although the Hubble Key Project, Chandra an...
International audienceA new method, based on the absorption of very high-energy gamma-rays by the co...
International audienceKilonovae observations can be used to out constraints on the Hubble constant (...
Kilonovae observations can be used to out constraints on the Hubble constant (H0). Here, the authors...
A brief history of the determination of the Hubble constant H0 is given. Early attempts following Le...
We combine Dark Energy Survey Year 1 clustering and weak lensing data with baryon acoustic oscillati...
By coupling observations of type Ia supernovae with results obtained from the best available numeric...
A brief history of the determination of the Hubble constant H_0 is given. Early attempts following L...
The Hubble constant (H0) is a measurement to describe the expansion rate of the Universe in the curr...
By coupling observations of type Ia supernovae with results obtained from the best available numeric...
In the model of low-energy quantum gravity by the author, the ratio H(z)/(1 + z) should be equal to...
An extraordinary number of Hubble constant measurements challenges physicists with selection of the ...
5 pages, 1 figure. Submitted to MNRASThe Hubble parameter H0 is still not very well measured. Althou...
The Hubble parameter H0 is still not very well measured. Although the Hubble Key Project, Chandra an...
International audienceA new method, based on the absorption of very high-energy gamma-rays by the co...
International audienceKilonovae observations can be used to out constraints on the Hubble constant (...
Kilonovae observations can be used to out constraints on the Hubble constant (H0). Here, the authors...
A brief history of the determination of the Hubble constant H0 is given. Early attempts following Le...
We combine Dark Energy Survey Year 1 clustering and weak lensing data with baryon acoustic oscillati...
By coupling observations of type Ia supernovae with results obtained from the best available numeric...
A brief history of the determination of the Hubble constant H_0 is given. Early attempts following L...
The Hubble constant (H0) is a measurement to describe the expansion rate of the Universe in the curr...
By coupling observations of type Ia supernovae with results obtained from the best available numeric...
In the model of low-energy quantum gravity by the author, the ratio H(z)/(1 + z) should be equal to...
An extraordinary number of Hubble constant measurements challenges physicists with selection of the ...