Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1                         ∗

M. M. Phillips; Carlos Contreras; E. Y. Hsiao; Nidia Morrell; Christopher R. Burns; Maximilian Stritzinger; C. Ashall; Wendy L. Freedman; P. Hoeflich; S. E. Persson; Anthony L. Piro; Nicholas B. Suntzeff; Syed A. Uddin; Jorge Anais; E. Baron; Luis Busta; Abdo Campillay; Sergio Castellón; Carlos Corco; T. Diamond; Christa Gall; Consuelo Gonzalez; Simon Holmbo; Kevin Krisciunas; Miguel Roth; Jacqueline Serón; F. Taddia; Simón Torres; J. P. Anderson; C. Baltay; Gastón Folatelli; L. Galbany; A. Goobar; Ellie Hadjiyska; Mario Hamuy; Mansi Kasliwal; C. Lidman; Peter E. Nugent; S. Perlmutter; David Rabinowitz; Stuart D. Ryder; Brian P. Schmidt; B. J. Shappee; Emma S. Walker

doi:10.1088/1538-3873/aae8bd

Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ^∗

M. M. Phillips^*
, Carlos Contreras
, E. Y. Hsiao
, Nidia Morrell
, Christopher R. Burns
, Maximilian Stritzinger
, C. Ashall
, Wendy L. Freedman
, P. Hoeflich
, S. E. Persson
, Anthony L. Piro
, Nicholas B. Suntzeff
, Syed A. Uddin
, Jorge Anais
, E. Baron
, Luis Busta
, Abdo Campillay
, Sergio Castellón
, Carlos Corco
, T. Diamond

Christa Gall, Consuelo Gonzalez, Simon Holmbo, Kevin Krisciunas, Miguel Roth, Jacqueline Serón, F. Taddia, Simón Torres, J. P. Anderson, C. Baltay, Gastón Folatelli, L. Galbany, A. Goobar, Ellie Hadjiyska, Mario Hamuy, Mansi Kasliwal, C. Lidman, Peter E. Nugent, S. Perlmutter, David Rabinowitz, Stuart D. Ryder, Brian P. Schmidt, B. J. Shappee, Emma S. Walker

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

81 Citations (Scopus)

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 TypeIa supernovae located in the smooth Hubble flow (0.03<z<0.10). Light curves were also obtained of a “Physics” sample composed of 90 nearby TypeIa supernovae at z≤0.04 selected for near-infrared spectroscopic timeseries 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.

Original language	English
Journal	Publications of the Astronomical Society of the Pacific
Volume	131
Issue number	995
DOIs	https://doi.org/10.1088/1538-3873/aae8bd
Publication status	Published - 1 Jan 2019

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Phillips, M. M., Contreras, C., Hsiao, E. Y., Morrell, N., Burns, C. R., Stritzinger, M., Ashall, C., Freedman, W. L., Hoeflich, P., Persson, S. E., Piro, A. L., Suntzeff, N. B., Uddin, S. A., Anais, J., Baron, E., Busta, L., Campillay, A., Castellón, S., Corco, C., ... Walker, E. S. (2019). Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ^∗. Publications of the Astronomical Society of the Pacific, 131(995). https://doi.org/10.1088/1538-3873/aae8bd

@article{3154a9e4dd3b4797942a1570ea0461ee,

title = "Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ∗",

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 TypeIa supernovae located in the smooth Hubble flow (0.03<z<0.10). Light curves were also obtained of a “Physics” sample composed of 90 nearby TypeIa supernovae at z≤0.04 selected for near-infrared spectroscopic timeseries 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.",

keywords = "(stars:) supernovae: general, Cosmology: observations, Galaxies: distances and redshifts",

author = "Phillips, \{M. M.\} and Carlos Contreras and Hsiao, \{E. Y.\} and Nidia Morrell and Burns, \{Christopher R.\} and Maximilian Stritzinger and C. Ashall and Freedman, \{Wendy L.\} and P. Hoeflich and Persson, \{S. E.\} and Piro, \{Anthony L.\} and Suntzeff, \{Nicholas B.\} and Uddin, \{Syed A.\} and Jorge Anais and E. Baron and Luis Busta and Abdo Campillay and Sergio Castell{\'o}n and Carlos Corco and T. Diamond and Christa Gall and Consuelo Gonzalez and Simon Holmbo and Kevin Krisciunas and Miguel Roth and Jacqueline Ser{\'o}n and F. Taddia and Sim{\'o}n Torres and Anderson, \{J. P.\} and C. Baltay and Gast{\'o}n Folatelli and L. Galbany and A. Goobar and Ellie Hadjiyska and Mario Hamuy and Mansi Kasliwal and C. Lidman and Nugent, \{Peter E.\} and S. Perlmutter and David Rabinowitz and Ryder, \{Stuart D.\} and Schmidt, \{Brian P.\} and Shappee, \{B. J.\} and Walker, \{Emma S.\}",

year = "2019",

month = jan,

day = "1",

doi = "10.1088/1538-3873/aae8bd",

language = "English",

volume = "131",

journal = "Publications of the Astronomical Society of the Pacific",

issn = "0004-6280",

publisher = "Institute of Physics",

number = "995",

}

Phillips, MM, Contreras, C, Hsiao, EY, Morrell, N, Burns, CR, Stritzinger, M, Ashall, C, Freedman, WL, Hoeflich, P, Persson, SE, Piro, AL, Suntzeff, NB, Uddin, SA, Anais, J, Baron, E, Busta, L, Campillay, A, Castellón, S, Corco, C, Diamond, T, Gall, C, Gonzalez, C, Holmbo, S, Krisciunas, K, Roth, M, Serón, J, Taddia, F, Torres, S, Anderson, JP, Baltay, C, Folatelli, G, Galbany, L, Goobar, A, Hadjiyska, E, Hamuy, M, Kasliwal, M, Lidman, C, Nugent, PE, Perlmutter, S, Rabinowitz, D, Ryder, SD, Schmidt, BP, Shappee, BJ & Walker, ES 2019, 'Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ^∗', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995. https://doi.org/10.1088/1538-3873/aae8bd

TY - JOUR

T1 - Carnegie supernova project-II

T2 - Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ∗

AU - Phillips, M. M.

AU - Contreras, Carlos

AU - Hsiao, E. Y.

AU - Morrell, Nidia

AU - Burns, Christopher R.

AU - Stritzinger, Maximilian

AU - Ashall, C.

AU - Freedman, Wendy L.

AU - Hoeflich, P.

AU - Persson, S. E.

AU - Piro, Anthony L.

AU - Suntzeff, Nicholas B.

AU - Uddin, Syed A.

AU - Anais, Jorge

AU - Baron, E.

AU - Busta, Luis

AU - Campillay, Abdo

AU - Castellón, Sergio

AU - Corco, Carlos

AU - Diamond, T.

AU - Gall, Christa

AU - Gonzalez, Consuelo

AU - Holmbo, Simon

AU - Krisciunas, Kevin

AU - Roth, Miguel

AU - Serón, Jacqueline

AU - Taddia, F.

AU - Torres, Simón

AU - Anderson, J. P.

AU - Baltay, C.

AU - Folatelli, Gastón

AU - Galbany, L.

AU - Goobar, A.

AU - Hadjiyska, Ellie

AU - Hamuy, Mario

AU - Kasliwal, Mansi

AU - Lidman, C.

AU - Nugent, Peter E.

AU - Perlmutter, S.

AU - Rabinowitz, David

AU - Ryder, Stuart D.

AU - Schmidt, Brian P.

AU - Shappee, B. J.

AU - Walker, Emma S.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - 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 TypeIa supernovae located in the smooth Hubble flow (0.03<z<0.10). Light curves were also obtained of a “Physics” sample composed of 90 nearby TypeIa supernovae at z≤0.04 selected for near-infrared spectroscopic timeseries 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.

AB - 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 TypeIa supernovae located in the smooth Hubble flow (0.03<z<0.10). Light curves were also obtained of a “Physics” sample composed of 90 nearby TypeIa supernovae at z≤0.04 selected for near-infrared spectroscopic timeseries 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.

KW - (stars:) supernovae: general

KW - Cosmology: observations

KW - Galaxies: distances and redshifts

UR - https://www.scopus.com/pages/publications/85061981054

U2 - 10.1088/1538-3873/aae8bd

DO - 10.1088/1538-3873/aae8bd

M3 - Article

SN - 0004-6280

VL - 131

JO - Publications of the Astronomical Society of the Pacific

JF - Publications of the Astronomical Society of the Pacific

IS - 995

ER -

Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ^∗

Abstract

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