Leveraging SN Ia spectroscopic similarity to improve the measurement of H 0
Recent studies suggest spectroscopic differences explain a fraction of the variation in Type
Ia supernova (SN Ia) luminosities after light-curve/color standardization. In this work,(i) we …
Ia supernova (SN Ia) luminosities after light-curve/color standardization. In this work,(i) we …
Cosmological results from the RAISIN survey: using Type Ia Supernovae in the near infrared as a novel path to measure the dark energy equation of state
DO Jones, KS Mandel, RP Kirshner… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract Type Ia supernovae (SNe Ia) are more precise standardizable candles when
measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012 to …
measured in the near-infrared (NIR) than in the optical. With this motivation, from 2012 to …
SALT3-NIR: Taking the Open-source Type Ia Supernova Model to Longer Wavelengths for Next-generation Cosmological Measurements
JDR Pierel, DO Jones, WD Kenworthy… - The Astrophysical …, 2022 - iopscience.iop.org
A large fraction of Type Ia supernova (SN Ia) observations over the next decade will be in
the near-infrared (NIR), at wavelengths beyond the reach of the current standard light-curve …
the near-infrared (NIR), at wavelengths beyond the reach of the current standard light-curve …
The Dark Energy Survey Supernova Program results: type Ia supernova brightness correlates with host galaxy dust
Cosmological analyses with type Ia supernovae (SNe Ia) often assume a single empirical
relation between colour and luminosity (β) and do not account for varying host-galaxy dust …
relation between colour and luminosity (β) and do not account for varying host-galaxy dust …
Constraining the SN Ia host galaxy dust law distribution and mass step: hierarchical BayeSN analysis of optical and near-infrared light curves
S Thorp, KS Mandel - Monthly Notices of the Royal Astronomical …, 2022 - academic.oup.com
We use the BayeSN hierarchical probabilistic SED model to analyse the optical–NIR
(BVriYJH) light curves of 86 Type Ia supernovae (SNe Ia) from the Carnegie Supernova …
(BVriYJH) light curves of 86 Type Ia supernovae (SNe Ia) from the Carnegie Supernova …
Hawai 'i Supernova Flows: a peculiar velocity survey using over a Thousand Supernovae in the near-infrared
A Do, BJ Shappee, JL Tonry, RB Tully… - Monthly Notices of …, 2025 - academic.oup.com
We introduce the Hawai 'i Supernova Flows project and present summary statistics of the
first 1217 astronomical transients observed, 668 of which are spectroscopically classified …
first 1217 astronomical transients observed, 668 of which are spectroscopically classified …
Two-population Bayesian hierarchical model of Type Ia supernovae
R Wojtak, J Hjorth, JO Hjortlund - Monthly Notices of the Royal …, 2023 - academic.oup.com
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 …
physical origin is unaccounted for. Here, we present a complete physical interpretation of the …
SN H0pe: The First Measurement of H0 from a Multiply Imaged Type Ia Supernova, Discovered by JWST
Abstract The first James Webb Space Telescope (JWST) Near InfraRed Camera imaging in
the field of the galaxy cluster PLCK G165. 7+ 67.0 (z= 0.35) uncovered a Type Ia supernova …
the field of the galaxy cluster PLCK G165. 7+ 67.0 (z= 0.35) uncovered a Type Ia supernova …
SICRET: Supernova Ia cosmology with truncated marginal neural Ratio EsTimation
ABSTRACT Type Ia supernovae (SNe Ia), standardizable candles that allow tracing the
expansion history of the Universe, are instrumental in constraining cosmological …
expansion history of the Universe, are instrumental in constraining cosmological …
Bird-Snack: Bayesian inference of dust law RV distributions using SN Ia apparent colours at peak
SM Ward, S Dhawan, KS Mandel… - Monthly Notices of …, 2023 - academic.oup.com
To reduce systematic uncertainties in Type Ia supernova (SN Ia) cosmology, the host galaxy
dust law shape parameter, RV, must be accurately constrained. We thus develop a …
dust law shape parameter, RV, must be accurately constrained. We thus develop a …