A spectral-energy distribution (SED) model for Type Ia supernovae (SNe Ia) is a critical tool
for measuring precise and accurate distances across a large redshift range and constraining …

Type Ia supernovae (SNe Ia) were instrumental in establishing the acceleration of the
universe's expansion. By virtue of their combination of distance reach, precision, and …

ABSTRACT While conventional Type Ia supernova (SN Ia) cosmology analyses rely
primarily on rest-frame optical light curves to determine distances, SNe Ia are excellent …

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 …

Abstract Type Ia supernovae (SNe Ia) are standardizable candles, but for over a decade
there has been a debate on how to properly account for their correlations with host galaxy …

The unknown cause of the correlation between Type Ia supernova (SN Ia) Hubble residuals
and their host-galaxy masses (the" mass step") may bias cosmological parameter …

Abstract Type Ia supernovae (SNe Ia) are powerful standardizable candles for constraining
cosmological models and provided the first evidence of the accelerated expansion of the …

We introduce the Hawaii Supernova Flows project and present summary statistics of the first
1218 astronomical transients observed, 669 of which are spectroscopically classified Type …

We use type Ia supernova (SN Ia) data obtained by the Sloan Digital Sky Survey-II
Supernova Survey (SDSS-II SNS) in combination with the publicly available SDSS DR16 …

ABSTRACT Type Ia Supernovae (SNe Ia) are powerful standardized candles for
constraining the cosmological model and provided the first evidence of accelerated …