Carnegie Supernova Project-II: Extending the Near-Infrared Hubble Diagram for Type Ia Supernovae to \(z\sim0.1\)

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 \(\sim100\) Type Ia supernovae located in the smooth Hubble flow (\(0.03 \lesssim z \lesssim 0.10\)). Light curves were also obtained...

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Hauptverfasser: Phillips, M M, Contreras, Carlos, Hsiao, E Y, Morrell, Nidia, Burns, Christopher R, Stritzinger, Maximilian, Ashall, C, Freedman, Wendy L, Hoeflich, P, Persson, S E, Piro, Anthony L, Suntzeff, Nicholas B, Uddin, Syed A, Anais, Jorge, Baron, E, Busta, Luis, Abdo Campillay, Castellón, Sergio, Corco, Carlos, Diamond, T, Gall, Christa, Gonzalez, Consuelo, Holmbo, Simon, Krisciunas, Kevin, Roth, Miguel, Serón, Jacqueline, Taddia, F, Torres, Simón, Anderson, J P, 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, B J, Walker, Emma S
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creator Phillips, M M
Contreras, Carlos
Hsiao, E Y
Morrell, Nidia
Burns, Christopher R
Stritzinger, Maximilian
Ashall, C
Freedman, Wendy L
Hoeflich, P
Persson, S E
Piro, Anthony L
Suntzeff, Nicholas B
Uddin, Syed A
Anais, Jorge
Baron, E
Busta, Luis
Abdo Campillay
Castellón, Sergio
Corco, Carlos
Diamond, T
Gall, Christa
Gonzalez, Consuelo
Holmbo, Simon
Krisciunas, Kevin
Roth, Miguel
Serón, Jacqueline
Taddia, F
Torres, Simón
Anderson, J P
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, B J
Walker, Emma S
description 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 \(\sim100\) Type Ia supernovae located in the smooth Hubble flow (\(0.03 \lesssim z \lesssim 0.10\)). Light curves were also obtained of a "Physics" sample composed of 90 nearby Type Ia supernovae at \(z \leq 0.04\) selected for near-infrared spectroscopic time-series observations. The primary emphasis of the CSP-II is to use the combination of optical and near-infrared photometry to achieve a distance precision of better than 5%. In this paper, details of the supernova sample, the observational strategy, and the characteristics of the photometric data are provided. In a companion paper, the near-infrared spectroscopy component of the project is presented.
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subjects Cosmology
Hubble diagram
Infrared photometry
Infrared spectra
Infrared spectroscopy
Light curve
Near infrared radiation
Photometry
Supernovae
title Carnegie Supernova Project-II: Extending the Near-Infrared Hubble Diagram for Type Ia Supernovae to \(z\sim0.1\)
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