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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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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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.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Cosmology ; Hubble diagram ; Infrared photometry ; Infrared spectra ; Infrared spectroscopy ; Light curve ; Near infrared radiation ; Photometry ; Supernovae</subject><ispartof>arXiv.org, 2018-10</ispartof><rights>2018. 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Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>781,785</link.rule.ids></links><search><creatorcontrib>Phillips, M M</creatorcontrib><creatorcontrib>Contreras, Carlos</creatorcontrib><creatorcontrib>Hsiao, E Y</creatorcontrib><creatorcontrib>Morrell, Nidia</creatorcontrib><creatorcontrib>Burns, Christopher R</creatorcontrib><creatorcontrib>Stritzinger, Maximilian</creatorcontrib><creatorcontrib>Ashall, C</creatorcontrib><creatorcontrib>Freedman, Wendy L</creatorcontrib><creatorcontrib>Hoeflich, P</creatorcontrib><creatorcontrib>Persson, S E</creatorcontrib><creatorcontrib>Piro, Anthony L</creatorcontrib><creatorcontrib>Suntzeff, Nicholas B</creatorcontrib><creatorcontrib>Uddin, Syed A</creatorcontrib><creatorcontrib>Anais, Jorge</creatorcontrib><creatorcontrib>Baron, E</creatorcontrib><creatorcontrib>Busta, Luis</creatorcontrib><creatorcontrib>Abdo Campillay</creatorcontrib><creatorcontrib>Castellón, Sergio</creatorcontrib><creatorcontrib>Corco, Carlos</creatorcontrib><creatorcontrib>Diamond, T</creatorcontrib><creatorcontrib>Gall, Christa</creatorcontrib><creatorcontrib>Gonzalez, Consuelo</creatorcontrib><creatorcontrib>Holmbo, Simon</creatorcontrib><creatorcontrib>Krisciunas, Kevin</creatorcontrib><creatorcontrib>Roth, Miguel</creatorcontrib><creatorcontrib>Serón, Jacqueline</creatorcontrib><creatorcontrib>Taddia, F</creatorcontrib><creatorcontrib>Torres, Simón</creatorcontrib><creatorcontrib>Anderson, J P</creatorcontrib><creatorcontrib>Baltay, C</creatorcontrib><creatorcontrib>Folatelli, Gastón</creatorcontrib><creatorcontrib>Galbany, L</creatorcontrib><creatorcontrib>Goobar, A</creatorcontrib><creatorcontrib>Hadjiyska, Ellie</creatorcontrib><creatorcontrib>Hamuy, Mario</creatorcontrib><creatorcontrib>Kasliwal, Mansi</creatorcontrib><creatorcontrib>Lidman, C</creatorcontrib><creatorcontrib>Nugent, Peter E</creatorcontrib><creatorcontrib>Perlmutter, S</creatorcontrib><creatorcontrib>Rabinowitz, David</creatorcontrib><creatorcontrib>Ryder, Stuart D</creatorcontrib><creatorcontrib>Schmidt, Brian P</creatorcontrib><creatorcontrib>Shappee, B J</creatorcontrib><creatorcontrib>Walker, Emma S</creatorcontrib><title>Carnegie Supernova Project-II: Extending the Near-Infrared Hubble Diagram for Type Ia Supernovae to \(z\sim0.1\)</title><title>arXiv.org</title><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. 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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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
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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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