Union through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
University of Hawaiʻi at Mānoa · Lawrence Berkeley National Laboratory · +11 more institutions
Abstract
Abstract 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 prevalence, they continue to provide key cosmological constraints, complementing other cosmological probes. Individual SN surveys cover only over about a factor of 2 in redshift, so compilations of multiple SN data sets are strongly beneficial. We assemble an up-to-date “Union” compilation of 2087 cosmologically useful SNe Ia from 24 data sets (“Union3”). We take care to put all SNe on the same distance scale and update the light-curve fitting with SALT3 to use the full rest-frame optical. Over the next few years, the number of…
Citation impact
- FWCI
- 105.67
- Percentile
- 100%
- References
- 300
Authors
11- DRD. RubinCorresponding
University of Hawaiʻi at Mānoa, Lawrence Berkeley National Laboratory
- GAG. AlderingCorresponding
Lawrence Berkeley National Laboratory
- MBM. BetouleCorresponding
Centre National de la Recherche Scientifique, Sorbonne Université, Laboratoire de Physique Nucléaire et de Hautes Énergies
- AFAndy FruchterCorresponding
Space Telescope Science Institute, Université Bourgogne Franche-Comté
- XHXiaosheng HuangCorresponding
Lawrence Berkeley National Laboratory, University of San Francisco
Topics & keywords
- Cosmology
- Bayesian probability
- Theoretical physics
- Physics
- Computer science
- Astronomy
- Artificial intelligence
- Climate action
Funding
- NSNational Science FoundationAwards: 1920304, DE-AC02-05CH11231
- UDU.S. Department of EnergyAwards: -AC02-05CH11231, 05CH11231, DE- AC02-05CH11231, AC02-05CH11231, DE-AC02, DE-AC02-05CH11231, DE-AC02-
- NANational Aeronautics and Space AdministrationAward: DE-AC02-05CH11231
- CICalifornia Institute of Technology
- ESEuropean Space Agency
- MDMinisterio de Ciencia e InnovaciónAward: PID2021-123528NB-I00
- OOOffice of ScienceAwards: AC02-05CH11231, -AC02-05CH11231, DE-AC02
- HEHigh Energy PhysicsAward: DE-AC02-05CH11231