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---
description: '

Time-series dataset from Dark Energy Survey Year 3 SN Ia (DES Y3 SNe Ia).

' homepage: https://des.ncsa.illinois.edu/releases/sn version: 0.0.1 citation: "% % ACKNOWLEDGEMENTS\n% From https://www.darkenergysurvey.org/the-des-project/data-access/\ \ :\n% \n% We request that all papers that use DES public data include the acknowledgement
\ below. In addition, we would appreciate if authors of all such papers would cite
\ the following papers where appropriate:\n% \n% DR1\n% The Dark Energy Survey Data
\ Release 1, DES Collaboration (2018)\n% The Dark Energy Survey Image Processing
\ Pipeline, E. Morganson, et al. (2018)\n% The Dark Energy Camera, B. Flaugher,
\ et al, AJ, 150, 150 (2015)\n% \n% This project used public archival data from
\ the Dark Energy Survey (DES). Funding for the DES Projects has been provided by
\ the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry
\ of Science and Education of Spain, the Science and Technology FacilitiesCouncil
\ of the United Kingdom, the Higher Education Funding Council for England, the National
\ Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign,
\ the Kavli Institute of Cosmological Physics at the University of Chicago, the
\ Center for Cosmology and Astro-Particle Physics at the Ohio State University,
\ the Mitchell Institute for Fundamental Physics and Astronomy at Texas A\&M University,
\ Financiadora de Estudos e Projetos, Funda{\c c}{\a}o Carlos Chagas Filho de
\ Amparo {\`a} Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento
\ Cient{\'i}fico e Tecnol{\'o}gico and the Minist{\'e}rio da Ci{\^e}ncia, Tecnologia
\ e Inova{\c c}{\
a}o, the Deutsche Forschungsgemeinschaft, and the Collaborating
\ Institutions in the Dark Energy Survey.\n% \n% The Collaborating Institutions
\ are Argonne National Laboratory, the University of California at Santa Cruz, the
\ University of Cambridge, Centro de Investigaciones Energ{\'e}ticas, Medioambientales
\ y Tecnol{\'o}gicas-Madrid, the University of Chicago, University College London,
\ the DES-Brazil Consortium, the University of Edinburgh, the Eidgen{\"o}ssische
\ Technische Hochschule (ETH) Z{\"u}rich, Fermi National Accelerator Laboratory,
\ the University of Illinois at Urbana-Champaign, the Institut de Ci{\`e}ncies
\ de l'Espai (IEEC/CSIC), the Institut de F{\'i}sica d'Altes Energies, Lawrence
\ Berkeley National Laboratory, the Ludwig-Maximilians Universit{\"a}t M{\"
u}nchen and the associated Excellence Cluster Universe, the University of Michigan,
\ the National Optical Astronomy Observatory, the University of Nottingham, The
\ Ohio State University, the OzDES Membership Consortium, the University of Pennsylvania,
\ the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University,
\ the University of Sussex, and Texas A\&M University.\n% Based in part on observations
\ at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory,
\ which is operated by the Association of Universities for Research in Astronomy
\ (AURA) under a cooperative agreement with the National Science Foundation.\n%
\ \n% CITATION\n@ARTICLE{2019ApJ...874..106B,\n author = {{Brout}, D. and
\ {Sako}, M. and {Scolnic}, D. and {Kessler}, R. and {D'Andrea}, C.B. and {Davis},
\ T.
M. and {Hinton}, S.R. and {Kim}, A.G. and {Lasker}, J. and {Macaulay}, E.
\ and {M{\"o}ller}, A. and {Nichol}, R.C. and {Smith}, M. and {Sullivan}, M.
\ and {Wolf}, R.
C. and {Allam}, S. and {Bassett}, B.A. and {Brown}, P. and {Castander},
\ F.
J. and {Childress}, M. and {Foley}, R.J. and {Galbany}, L. and {Herner}, K.
\ and {Kasai}, E. and {March}, M. and {Morganson}, E. and {Nugent}, P. and {Pan},
\ Y. -C. and {Thomas}, R.
C. and {Tucker}, B.E. and {Wester}, W. and {Abbott},
\ T.
M.C. and {Annis}, J. and {Avila}, S. and {Bertin}, E. and {Brooks}, D. and
\ {Burke}, D.
L. and {Carnero Rosell}, A. and {Carrasco Kind}, M. and {Carretero},
\ J. and {Crocce}, M. and {Cunha}, C.E. and {da Costa}, L.N. and {Davis}, C. and
\ {De Vicente}, J. and {Desai}, S. and {Diehl}, H.T. and {Doel}, P. and {Eifler},
\ T.
F. and {Flaugher}, B. and {Fosalba}, P. and {Frieman}, J. and {Garc{\'\i}a-Bellido},
\ J. and {Gaztanaga}, E. and {Gerdes}, D.W. and {Goldstein}, D.A. and {Gruen},
\ D. and {Gruendl}, R.A. and {Gschwend}, J. and {Gutierrez}, G. and {Hartley},
\ W.
G. and {Hollowood}, D.L. and {Honscheid}, K. and {James}, D.J. and {Kuehn},
\ K. and {Kuropatkin}, N. and {Lahav}, O. and {Li}, T.S. and {Lima}, M. and {Marshall},
\ J.
L. and {Martini}, P. and {Miquel}, R. and {Nord}, B. and {Plazas}, A.A. and
\ {Roodman}, A. and {Rykoff}, E.
S. and {Sanchez}, E. and {Scarpine}, V. and {Schindler},
\ R. and {Schubnell}, M. and {Serrano}, S. and {Sevilla-Noarbe}, I. and {Soares-Santos},
\ M. and {Sobreira}, F. and {Suchyta}, E. and {Swanson}, M.E.C. and {Tarle}, G.
\ and {Thomas}, D. and {Tucker}, D.L. and {Walker}, A.R. and {Yanny}, B. and {Zhang},
\ Y. and {DES COLLABORATION}},\n title = "{First Cosmology Results Using
\ Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve
\ Data Release}",\n journal = {\apj},\n keywords = {cosmology: observations,
\ supernovae: general, techniques: photometric, Astrophysics - Instrumentation and
\ Methods for Astrophysics},\n year = 2019,\n month = mar,\n
\ volume = {874},\n number = {1},\n eid = {106},\n pages
\ = {106},\n doi = {10.3847/1538-4357/ab06c1},\narchivePrefix = {arXiv},\n
\ eprint = {1811.02378},\n primaryClass = {astro-ph.IM},\n adsurl =
\ {https://ui.adsabs.harvard.edu/abs/2019ApJ...874..106B},\n adsnote = {Provided
\ by the SAO/NASA Astrophysics Data System}\n}\n" ---

# Des_y3_sne_ia Dataset

CC BY-NC-ND 4.0

Time-series dataset from Dark Energy Survey Year 3 SN Ia (DES Y3 SNe Ia).

% % ACKNOWLEDGEMENTS

% From https://www.darkenergysurvey.org/the-des-project/data-access/ : % % We request that all papers that use DES public data include the acknowledgement below. In addition, we would appreciate if authors of all such papers would cite the following papers where appropriate: % % DR1 % The Dark Energy Survey Data Release 1, DES Collaboration (2018) % The Dark Energy Survey Image Processing Pipeline, E. Morganson, et al. (2018) % The Dark Energy Camera, B. Flaugher, et al, AJ, 150, 150 (2015) % % This project used public archival data from the Dark Energy Survey (DES). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology FacilitiesCouncil of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Funda{\c c}{~a}o Carlos Chagas Filho de Amparo {`a} Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient{'i}fico e Tecnol{'o}gico and the Minist{'e}rio da Ci{^e}ncia, Tecnologia e Inova{\c c}{~a}o, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. % % The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energ{'e}ticas, Medioambientales y Tecnol{'o}gicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgen{"o}ssische Technische Hochschule (ETH) Z{"u}rich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci{`e}ncies de l'Espai (IEEC/CSIC), the Institut de F{'i}sica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universit{"a}t M{"u}nchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the OzDES Membership Consortium, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University. % Based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. % % CITATION @ARTICLE{2019ApJ...874..106B, author = {{Brout}, D. and {Sako}, M. and {Scolnic}, D. and {Kessler}, R. and {D'Andrea}, C.B. and {Davis}, T.M. and {Hinton}, S.R. and {Kim}, A.G. and {Lasker}, J. and {Macaulay}, E. and {M{"o}ller}, A. and {Nichol}, R.C. and {Smith}, M. and {Sullivan}, M. and {Wolf}, R.C. and {Allam}, S. and {Bassett}, B.A. and {Brown}, P. and {Castander}, F.J. and {Childress}, M. and {Foley}, R.J. and {Galbany}, L. and {Herner}, K. and {Kasai}, E. and {March}, M. and {Morganson}, E. and {Nugent}, P. and {Pan}, Y. -C. and {Thomas}, R.C. and {Tucker}, B.E. and {Wester}, W. and {Abbott}, T.M.C. and {Annis}, J. and {Avila}, S. and {Bertin}, E. and {Brooks}, D. and {Burke}, D.L. and {Carnero Rosell}, A. and {Carrasco Kind}, M. and {Carretero}, J. and {Crocce}, M. and {Cunha}, C.E. and {da Costa}, L.N. and {Davis}, C. and {De Vicente}, J. and {Desai}, S. and {Diehl}, H.T. and {Doel}, P. and {Eifler}, T.F. and {Flaugher}, B. and {Fosalba}, P. and {Frieman}, J. and {Garc{'\i}a-Bellido}, J. and {Gaztanaga}, E. and {Gerdes}, D.W. and {Goldstein}, D.A. and {Gruen}, D. and {Gruendl}, R.A. and {Gschwend}, J. and {Gutierrez}, G. and {Hartley}, W.G. and {Hollowood}, D.L. and {Honscheid}, K. and {James}, D.J. and {Kuehn}, K. and {Kuropatkin}, N. and {Lahav}, O. and {Li}, T.S. and {Lima}, M. and {Marshall}, J.L. and {Martini}, P. and {Miquel}, R. and {Nord}, B. and {Plazas}, A.A. and {Roodman}, A. and {Rykoff}, E.S. and {Sanchez}, E. and {Scarpine}, V. and {Schindler}, R. and {Schubnell}, M. and {Serrano}, S. and {Sevilla-Noarbe}, I. and {Soares-Santos}, M. and {Sobreira}, F. and {Suchyta}, E. and {Swanson}, M.E.C. and {Tarle}, G. and {Thomas}, D. and {Tucker}, D.L. and {Walker}, A.R. and {Yanny}, B. and {Zhang}, Y. and {DES COLLABORATION}}, title = "{First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release}", journal = {\apj}, keywords = {cosmology: observations, supernovae: general, techniques: photometric, Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2019, month = mar, volume = {874}, number = {1}, eid = {106}, pages = {106}, doi = {10.3847/1538-4357/ab06c1}, archivePrefix = {arXiv}, eprint = {1811.02378}, primaryClass = {astro-ph.IM}, adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...874..106B}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }