The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries*

Hayden, Brian; Rubin, D.; Boone, K.; Aldering, G.; Nordin, J.; Brodwin, M.; E. Deustua, Susana; Dixon, S.; Fagrelius, Parker; Fruchter, Andy; Eisenhardt, Peter; H. Gonzalez, Anthony; Gupta, R.; Hook, I.; Lidman, C.; Luther, Kyle; Muzzin, Adam; Raha, Zachary; Ruiz-Lapuente, Pilar; Saunders, C.; Sofiatti, C.; Stanford, Adam; Suzuki, N.; Webb, Tracy; C. Williams, S.; Wilson, Gillian; Yen, Mike; Amanullah, R.; Barbary, K.; Böhringer, H.; Chappell, Greta; E. Cunha, Carlos; Currie, Miles; Fassbender, R.; D. Gladders, Michael; Goobar, A.; Hildebrandt, H.; Hoekstra, Henk; Huang, Xiaosheng; Huterer, Dragan; James Jee, M.; Kim, Alex; Kowalski, M.; V. Linder, Eric; Meyers, J.; Pain, R.; Perlmutter, S.; Richard, Johan; Rosati, P.; Rozo, Eduardo; S. Rykoff, E.; Santos, Joana; L. Spadafora, A.; Stern, Daniel; H. Wechsler, Risa; Supernova Cosmology Project, The

doi:10.3847/1538-4357/abed4d

Public

The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries*

Published in The Astrophysical Journal • May 1, 2021

Authors:

Brian Hayden

D. Rubin

K. Boone

Abstract

Abstract The See Change survey was designed to make z > 1 cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measurements through weak lensing. This survey observed twelve galaxy clusters with the Hubble Space Telescope (HST) spa...

Subject

Redshift

Physics

Supernova

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