The Dark Energy Survey: Cosmology Results with∼ 1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set
DES Collaboration, TMC Abbott… - The Astrophysical …, 2024 - iopscience.iop.org
We present cosmological constraints from the sample of Type Ia supernovae (SNe Ia)
discovered and measured during the full 5 yr of the Dark Energy Survey (DES) SN program …
discovered and measured during the full 5 yr of the Dark Energy Survey (DES) SN program …
Union through UNITY: Cosmology with 2,000 SNe using a unified Bayesian framework
D Rubin, G Aldering, M Betoule, A Fruchter… - arxiv preprint arxiv …, 2023 - arxiv.org
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 …
universe's expansion. By virtue of their combination of distance reach, precision, and …
[HTML][HTML] The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties
M Vincenzi, D Brout, P Armstrong… - The Astrophysical …, 2024 - iopscience.iop.org
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 …
Ia) from the Dark Energy Survey supernova program (DES-SN). DES-SN discovered more …
The dark energy survey supernova program: investigating beyond-ΛCDM
R Camilleri, TM Davis, M Vincenzi… - Monthly Notices of …, 2024 - academic.oup.com
We report constraints on a variety of non-standard cosmological models using the full 5-yr
photometrically classified type Ia supernova sample from the Dark Energy Survey (DES …
photometrically classified type Ia supernova sample from the Dark Energy Survey (DES …
The dark energy survey supernova program: light curves and 5 yr data release
We present griz photometric light curves for the full 5 yr of the Dark Energy Survey
Supernova (DES-SN) program, obtained with both forced point-spread function photometry …
Supernova (DES-SN) program, obtained with both forced point-spread function photometry …
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 …
ZTF SN Ia DR2: Study of Type Ia supernova light-curve fits
M Rigault, M Smith, N Regnault, WD Kenworthy… - Astronomy & …, 2025 - aanda.org
Type Ia supernova (SN Ia) cosmology relies on the estimation of light-curve parameters to
derive precision distances, which are used to infer cosmological parameters such as H 0, Ω …
derive precision distances, which are used to infer cosmological parameters such as H 0, Ω …
ZTF SN Ia DR2: Exploring SN Ia properties in the vicinity of under-dense environments
M Aubert, P Rosnet, B Popovic, F Ruppin… - Astronomy & …, 2025 - aanda.org
Context. The unprecedented statistics of detected Type Ia supernovae (SNe Ia) brought by
the Zwicky Transient Facility (ZTF) enable us to probe the impact of the large-scale structure …
the Zwicky Transient Facility (ZTF) enable us to probe the impact of the large-scale structure …
Environmental Dependence of Type Ia Supernovae in Low-redshift Galaxy Clusters
We present an analysis of 102 Type Ia supernovae (SNe Ia) in nearby (z< 0.1), x-ray-
selected galaxy clusters. This is the largest such sample to date and is based on archival …
selected galaxy clusters. This is the largest such sample to date and is based on archival …
The Dark Energy Survey Supernova Program: Corrections on photometry due to wavelength-dependent atmospheric effects
Wavelength-dependent atmospheric effects impact photometric supernova flux
measurements for ground-based observations. We present corrections on supernova flux …
measurements for ground-based observations. We present corrections on supernova flux …