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  • Qu, H.; Sako, M.; Vincenzi, M.; Sánchez, C.; Brout, D.; Kessler, R.; Chen, R.; Davis, T.; Galbany, L.; Kelsey, L.; Lee, J.; Lidman, C.; Popovic, B.; Rose, B.; Scolnic, D.; Smith, M.; Sullivan, M.; Wiseman, P.; Abbott, T.M.C.; Aguena, M.; Alves, O.; Bacon, D.; Bertin, E.; Brooks, D.; Burke, D.L.; Carnero Rosell, A.; Carretero, J.; da Costa, L.N.; Pereira, M.E.S.; Diehl, H.T.; Doel, P.; Everett, S.; Ferrero, Ismael; Frieman, J.; García-Bellido, J.; Giannini, G.; Gruen, D.; Gruendl, R.A.; Gutierrez, G.; Hinton, S.R.; Hollowood, D.L.; Honscheid, K.; James, D.J.; Kuehn, K.; Lahav, O.; Marshall, J.L.; Mena-Fernández, J.; Menanteau, F.; Miquel, R.; Ogando, R.L.C.; Palmese, A.; Pieres, A.; Plazas-Malagón, A.A.; Raveri, M.; Sanchez, E.; Sevilla-Noarbe, I.; Soares-Santos, M.; Suchyta, E.; Tarle, G.; Weaverdyck, N. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2024)
    Abstract Redshift measurements, primarily obtained from host galaxies, are essential for inferring cosmological parameters from type Ia supernovae (SNe Ia). Matching SNe to host galaxies using images is nontrivial, ...