Measuring the Effect of Progenitor Metallicity on Type Ia Supernova Distance Estimates
R. J. Foley(Center for Astrophysics Harvard & Smithsonian), J. C. Wheeler(The University of Texas at Austin), G. Dimitriadis(Trinity College Dublin), Y. C. Pan(University of Oxford), M. R. Siebert(University of California, Santa Cruz), C. Rojas-Bravo(University of California, Santa Cruz), R. Kirshner(TMT Observatory), David Jones, Ori Dosovitz Fox, Alex Filippenko, S. Taubenberger(Max Planck Institute for Astrophysics), F. K. Roepke, Stuart Sim(Queen's University Belfast)
HST Proposal
May 1, 2020
Cited by 1
Related Papers
The Pantheon+ Analysis: Cosmological Constraints
|The Astrophysical Journal|2022|1.3k
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
|The Astrophysical Journal Letters|2017|1k
The Pantheon+ Analysis: The Full Data Set and Light-curve Release
|The Astrophysical Journal|2022|900
A γ-ray burst at a redshift of z ≈ 8.2
|Nature|2009|639