학술논문
Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z ∼ 0.1∗ ∗ This paper includes data gathered with the 6.5 meter Magellan telescopes at Las Campanas Observatory, Chile.
Document Type
article
Author
Phillips, MM; Contreras, Carlos; Hsiao, EY; Morrell, Nidia; Burns, Christopher R; Stritzinger, Maximilian; Ashall, C; Freedman, Wendy L; Hoeflich, P; Persson, SE; Piro, Anthony L; Suntzeff, Nicholas B; Uddin, Syed A; Anais, Jorge; Baron, E; Busta, Luis; Campillay, Abdo; Castellón, Sergio; Corco, Carlos; Diamond, T; Gall, Christa; Gonzalez, Consuelo; Holmbo, Simon; Krisciunas, Kevin; Roth, Miguel; Serón, Jacqueline; Taddia, F; Torres, Simón; Anderson, JP; Baltay, C; Folatelli, Gastón; Galbany, L; Goobar, A; Hadjiyska, Ellie; Hamuy, Mario; Kasliwal, Mansi; Lidman, C; Nugent, Peter E; Perlmutter, S; Rabinowitz, David; Ryder, Stuart D; Schmidt, Brian P; Shappee, BJ; Walker, Emma S
Source
Publications of the Astronomical Society of the Pacific. 131(995)
Subject
Language
Abstract
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical and near-infrared observations of a “Cosmology” sample of ∼100 TypeIa supernovae located in the smooth Hubble flow (0.03