LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY

G. Narayan; A. Rest; B. E. Tucker; R. J. Foley; W. M. Wood-Vasey; P. Challis; C. Stubbs; R. P. Kirshner; C. Aguilera; A. C. Becker; S. Blondin; A. Clocchiatti; R. Covarrubias; G. Damke; T. M. Davis; A. V. Filippenko; M. Ganeshalingam; A. Garg; P. M. Garnavich; M. Hicken; S. W. Jha; K. Krisciunas; B. Leibundgut; W. Li; T. Matheson; G. Miknaitis; G. Pignata; J. L. Prieto; A. G. Riess; B. P. Schmidt; J. M. Silverman; R. C. Smith; J. Sollerman; J. Spyromilio; N. B. Suntzeff; J. L. Tonry; A. Zenteno

doi:10.3847/0067-0049/224/1/3

LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY

G. Narayan, A. Rest, B. E. Tucker, R. J. Foley, W. M. Wood-Vasey, P. Challis, C. Stubbs, R. P. Kirshner, C. Aguilera, A. C. Becker, S. Blondin, A. Clocchiatti, R. Covarrubias, G. Damke, T. M. Davis, A. V. Filippenko, M. Ganeshalingam, A. Garg, P. M. Garnavich, M. HickenS. W. Jha, K. Krisciunas, B. Leibundgut, W. Li, T. Matheson, G. Miknaitis, G. Pignata, J. L. Prieto, A. G. Riess, B. P. Schmidt, J. M. Silverman, R. C. Smith, J. Sollerman, J. Spyromilio, N. B. Suntzeff, J. L. Tonry, A. Zenteno

Astronomy

Research output: Contribution to journal › Review article › peer-review

Abstract

The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R- and I-band photometry, measured from images obtained using the MOSAIC II camera at the CTIO Blanco, along with rapid-response spectroscopy for each object. We use our spectroscopic follow-up observations to determine an accurate, quantitative classification, and precise redshift. Through an extensive calibration program we have improved the precision of the CTIO Blanco natural photometric system. We use several empirical metrics to measure our internal photometric consistency and our absolute calibration of the survey. We assess the effect of various potential sources of systematic bias on our measured fluxes, and estimate the dominant term in the systematic error budget from the photometric calibration on our absolute fluxes is ∼1%.

Original language	English (US)
Article number	3
Journal	Astrophysical Journal, Supplement Series
Volume	224
Issue number	1
DOIs	https://doi.org/10.3847/0067-0049/224/1/3
State	Published - May 2016

Keywords

cosmology: observations
methods: data analysis
supernovae: general
surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/0067-0049/224/1/3

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Narayan, G., Rest, A., Tucker, B. E., Foley, R. J., Wood-Vasey, W. M., Challis, P., Stubbs, C., Kirshner, R. P., Aguilera, C., Becker, A. C., Blondin, S., Clocchiatti, A., Covarrubias, R., Damke, G., Davis, T. M., Filippenko, A. V., Ganeshalingam, M., Garg, A., Garnavich, P. M., ... Zenteno, A. (2016). LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY. Astrophysical Journal, Supplement Series, 224(1), [3]. https://doi.org/10.3847/0067-0049/224/1/3

LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY. / Narayan, G.; Rest, A.; Tucker, B. E.; Foley, R. J.; Wood-Vasey, W. M.; Challis, P.; Stubbs, C.; Kirshner, R. P.; Aguilera, C.; Becker, A. C.; Blondin, S.; Clocchiatti, A.; Covarrubias, R.; Damke, G.; Davis, T. M.; Filippenko, A. V.; Ganeshalingam, M.; Garg, A.; Garnavich, P. M.; Hicken, M.; Jha, S. W.; Krisciunas, K.; Leibundgut, B.; Li, W.; Matheson, T.; Miknaitis, G.; Pignata, G.; Prieto, J. L.; Riess, A. G.; Schmidt, B. P.; Silverman, J. M.; Smith, R. C.; Sollerman, J.; Spyromilio, J.; Suntzeff, N. B.; Tonry, J. L.; Zenteno, A.

In: Astrophysical Journal, Supplement Series, Vol. 224, No. 1, 3, 05.2016.

Research output: Contribution to journal › Review article › peer-review

Narayan, G, Rest, A, Tucker, BE, Foley, RJ, Wood-Vasey, WM, Challis, P, Stubbs, C, Kirshner, RP, Aguilera, C, Becker, AC, Blondin, S, Clocchiatti, A, Covarrubias, R, Damke, G, Davis, TM, Filippenko, AV, Ganeshalingam, M, Garg, A, Garnavich, PM, Hicken, M, Jha, SW, Krisciunas, K, Leibundgut, B, Li, W, Matheson, T, Miknaitis, G, Pignata, G, Prieto, JL, Riess, AG, Schmidt, BP, Silverman, JM, Smith, RC, Sollerman, J, Spyromilio, J, Suntzeff, NB, Tonry, JL & Zenteno, A 2016, 'LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY', Astrophysical Journal, Supplement Series, vol. 224, no. 1, 3. https://doi.org/10.3847/0067-0049/224/1/3

Narayan, G. ; Rest, A. ; Tucker, B. E. ; Foley, R. J. ; Wood-Vasey, W. M. ; Challis, P. ; Stubbs, C. ; Kirshner, R. P. ; Aguilera, C. ; Becker, A. C. ; Blondin, S. ; Clocchiatti, A. ; Covarrubias, R. ; Damke, G. ; Davis, T. M. ; Filippenko, A. V. ; Ganeshalingam, M. ; Garg, A. ; Garnavich, P. M. ; Hicken, M. ; Jha, S. W. ; Krisciunas, K. ; Leibundgut, B. ; Li, W. ; Matheson, T. ; Miknaitis, G. ; Pignata, G. ; Prieto, J. L. ; Riess, A. G. ; Schmidt, B. P. ; Silverman, J. M. ; Smith, R. C. ; Sollerman, J. ; Spyromilio, J. ; Suntzeff, N. B. ; Tonry, J. L. ; Zenteno, A. / LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY. In: Astrophysical Journal, Supplement Series. 2016 ; Vol. 224, No. 1.

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title = "LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY",

abstract = "The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R- and I-band photometry, measured from images obtained using the MOSAIC II camera at the CTIO Blanco, along with rapid-response spectroscopy for each object. We use our spectroscopic follow-up observations to determine an accurate, quantitative classification, and precise redshift. Through an extensive calibration program we have improved the precision of the CTIO Blanco natural photometric system. We use several empirical metrics to measure our internal photometric consistency and our absolute calibration of the survey. We assess the effect of various potential sources of systematic bias on our measured fluxes, and estimate the dominant term in the systematic error budget from the photometric calibration on our absolute fluxes is ∼1%.",

keywords = "cosmology: observations, methods: data analysis, supernovae: general, surveys",

author = "G. Narayan and A. Rest and Tucker, {B. E.} and Foley, {R. J.} and Wood-Vasey, {W. M.} and P. Challis and C. Stubbs and Kirshner, {R. P.} and C. Aguilera and Becker, {A. C.} and S. Blondin and A. Clocchiatti and R. Covarrubias and G. Damke and Davis, {T. M.} and Filippenko, {A. V.} and M. Ganeshalingam and A. Garg and Garnavich, {P. M.} and M. Hicken and Jha, {S. W.} and K. Krisciunas and B. Leibundgut and W. Li and T. Matheson and G. Miknaitis and G. Pignata and Prieto, {J. L.} and Riess, {A. G.} and Schmidt, {B. P.} and Silverman, {J. M.} and Smith, {R. C.} and J. Sollerman and J. Spyromilio and Suntzeff, {N. B.} and Tonry, {J. L.} and A. Zenteno",

note = "Funding Information: A.V.F.'s group at UC Berkeley received additional assistance from NSF grants AST-0908886 and AST-1211916, the TABASGO foundation, and the Christopher R. Redlich fund. The Dark Cosmology Centre is funded by the Danish National Research Foundation. The ESSENCE survey team is very grateful to the scientific and technical staff at the observatories we have been privileged to use. Publisher Copyright: {\textcopyright} 2016. The American Astronomical Society. All rights reserved.",

year = "2016",

month = may,

doi = "10.3847/0067-0049/224/1/3",

language = "English (US)",

volume = "224",

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T1 - LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY

AU - Narayan, G.

AU - Rest, A.

AU - Tucker, B. E.

AU - Foley, R. J.

AU - Wood-Vasey, W. M.

AU - Challis, P.

AU - Stubbs, C.

AU - Kirshner, R. P.

AU - Aguilera, C.

AU - Becker, A. C.

AU - Blondin, S.

AU - Clocchiatti, A.

AU - Covarrubias, R.

AU - Damke, G.

AU - Davis, T. M.

AU - Filippenko, A. V.

AU - Ganeshalingam, M.

AU - Garg, A.

AU - Garnavich, P. M.

AU - Hicken, M.

AU - Jha, S. W.

AU - Krisciunas, K.

AU - Leibundgut, B.

AU - Li, W.

AU - Matheson, T.

AU - Miknaitis, G.

AU - Pignata, G.

AU - Prieto, J. L.

AU - Riess, A. G.

AU - Schmidt, B. P.

AU - Silverman, J. M.

AU - Smith, R. C.

AU - Sollerman, J.

AU - Spyromilio, J.

AU - Suntzeff, N. B.

AU - Tonry, J. L.

AU - Zenteno, A.

N1 - Funding Information: A.V.F.'s group at UC Berkeley received additional assistance from NSF grants AST-0908886 and AST-1211916, the TABASGO foundation, and the Christopher R. Redlich fund. The Dark Cosmology Centre is funded by the Danish National Research Foundation. The ESSENCE survey team is very grateful to the scientific and technical staff at the observatories we have been privileged to use. Publisher Copyright: © 2016. The American Astronomical Society. All rights reserved.

PY - 2016/5

Y1 - 2016/5

N2 - The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R- and I-band photometry, measured from images obtained using the MOSAIC II camera at the CTIO Blanco, along with rapid-response spectroscopy for each object. We use our spectroscopic follow-up observations to determine an accurate, quantitative classification, and precise redshift. Through an extensive calibration program we have improved the precision of the CTIO Blanco natural photometric system. We use several empirical metrics to measure our internal photometric consistency and our absolute calibration of the survey. We assess the effect of various potential sources of systematic bias on our measured fluxes, and estimate the dominant term in the systematic error budget from the photometric calibration on our absolute fluxes is ∼1%.

AB - The ESSENCE survey discovered 213 Type Ia supernovae at redshifts 0.1 < z < 0.81 between 2002 and 2008. We present their R- and I-band photometry, measured from images obtained using the MOSAIC II camera at the CTIO Blanco, along with rapid-response spectroscopy for each object. We use our spectroscopic follow-up observations to determine an accurate, quantitative classification, and precise redshift. Through an extensive calibration program we have improved the precision of the CTIO Blanco natural photometric system. We use several empirical metrics to measure our internal photometric consistency and our absolute calibration of the survey. We assess the effect of various potential sources of systematic bias on our measured fluxes, and estimate the dominant term in the systematic error budget from the photometric calibration on our absolute fluxes is ∼1%.

KW - cosmology: observations

KW - methods: data analysis

KW - supernovae: general

KW - surveys

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U2 - 10.3847/0067-0049/224/1/3

DO - 10.3847/0067-0049/224/1/3

M3 - Review article

AN - SCOPUS:84977641697

VL - 224

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

SN - 0067-0049

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M1 - 3

ER -

LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY

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