We present constraints on cosmological parameters from the Pantheon+ analysis of 1701
light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from z= 0.001 to …

The difference from 4 to 6 σ in the Hubble constant (H 0) between the values observed with
the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (Cosmic Microwave …

The tip of the red giant branch (TRGB) provides a luminous standard candle for constructing
distance ladders to measure the Hubble constant. In practice, its measurements via edge …

We use the state-of-the-art data on cosmic chronometers (CCH) and the Pantheon+
compilation of supernovae of Type Ia (SNIa) to test the constancy of the SNIa absolute …

Separating the components of redshift due to expansion and peculiar motion in the nearby
universe (z< 0.1) is critical for using Type Ia Supernovae (SNe Ia) to measure the Hubble …

Current observations do not rule out the possibility that the Universe might end up in an
abrupt event, but that fatality might be avoided, as it happens in the pseudorip dark energy …

We present the full Hubble diagram of photometrically classified Type Ia supernovae (SNe
Ia) from the Dark Energy Survey supernova program (DES-SN). DES-SN discovered more …

The currently used standardization of Type Ia supernovae results in Hubble residuals whose
physical origin is unaccounted for. Here, we present a complete physical interpretation of the …

We decompose Pantheon+ Type Ia supernovae (SN) in hemispheres on the sky finding
angular variations up to 4 km/s/Mpc, corresponding to a statistical significance up to 1.9 σ, in …

For the past decade, SALT2 has been the most common model used to fit Type Ia supernova
(SN Ia) light curves for dark energy analyses. Recently, the SALT3 model was released …