We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 Type Ia Supernovae (SNe Ia) in the redshift range 0.01<z<2.3 compiled by Scolnic et al. (2018). Applying the flux-averaging method for detecting unknown systematic effects, we find that the "Pantheon" sample has been well calibrated and the bias caused by unknown systematic errors has been minimized. We present the estimate of distances measured from SNe Ia and reconstruct the expansion history of the Universe. The results are in agreement with a simple cosmological constant model and reveals the possible improvements that future SN Ia observations from WFIRST and LSST can target. We have derived distance priors using the Cosmic Microwave Bac...
In the late 1990s, precise distance measurements with Type Ia supernovae (SNe Ia) were used to show ...
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z 〉 1 (9 at 1.5 〈 z 〈 2.3) rece...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
We present the distance priors that we have derived from the 2015 Planck data, and use these in comb...
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
Aims: We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
In the late 1990s, precise distance measurements with Type Ia supernovae (SNe Ia) were used to show ...
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z 〉 1 (9 at 1.5 〈 z 〈 2.3) rece...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
We present the distance priors that we have derived from the 2015 Planck data, and use these in comb...
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
International audienceWe present constraints on cosmological parameters from the Pantheon+ analysis ...
Aims: We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves o...
In the late 1990s, precise distance measurements with Type Ia supernovae (SNe Ia) were used to show ...
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observa...
We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z 〉 1 (9 at 1.5 〈 z 〈 2.3) rece...