First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation
- Brout, D.
- Scolnic, D.
- Kessler, R.
- D'Andrea, C.B.
- Davis, T.M.
- Gupta, R.R.
- Hinton, S.R.
- Kim, A.G.
- Lasker, J.
- Lidman, C.
- Macaulay, E.
- Möller, A.
- Nichol, R.C.
- Sako, M.
- Smith, M.
- Sullivan, M.
- Zhang, B.
- Andersen, P.
- Asorey, J.
- Avelino, A.
- Bassett, B.A.
- Brown, P.
- Calcino, J.
- Carollo, D.
- Challis, P.
- Childress, M.
- Clocchiatti, A.
- Filippenko, A.V.
- Foley, R.J.
- Galbany, L.
- Glazebrook, K.
- Hoormann, J.K.
- Kasai, E.
- Kirshner, R.P.
- Kuehn, K.
- Kuhlmann, S.
- Lewis, G.F.
- Mandel, K.S.
- March, M.
- Miranda, V.
- Morganson, E.
- Muthukrishna, D.
- Nugent, P.
- Palmese, A.
- Pan, Y.-C.
- Sharp, R.
- Sommer, N.E.
- Swann, E.
- Thomas, R.C.
- Tucker, B.E.
- Uddin, S.A.
- Wester, W.
- Abbott, T.M.C.
- Allam, S.
- Annis, J.
- Avila, S.
- Bechtol, K.
- Bernstein, G.M.
- Bertin, E.
- Brooks, D.
- Burke, D.L.
- Carnero Rosell, A.
- Carrasco Kind, M.
- Carretero, J.
- Castander, F.J.
- Cunha, C.E.
- Da Costa, L.N.
- Davis, C.
- De Vicente, J.
- Depoy, D.L.
- Desai, S.
- Diehl, H.T.
- Doel, P.
- Drlica-Wagner, A.
- Eifler, T.F.
- Estrada, J.
- Fernandez, E.
- Flaugher, B.
- Fosalba, P.
- Frieman, J.
- García-Bellido, J.
- Gruen, D.
- Gruendl, R.A.
- Gutierrez, G.
- Hartley, W.G.
- Hollowood, D.L.
- Honscheid, K.
- Hoyle, B.
- James, D.J.
- Jarvis, M.
- Jeltema, T.
- Krause, E.
- Lahav, O.
- Li, T.S.
- Lima, M.
- Maia, M.A.G.
- Marriner, J.
- Marshall, J.L.
- Martini, P.
- Menanteau, F.
- Miller, C.J.
- Miquel, R.
- Ogando, R.L.C.
- Plazas, A.A.
- Romer, A.K.
- Roodman, A.
- Rykoff, E.S.
- Sanchez, E.
- Santiago, B.
- Scarpine, V.
- Schubnell, M.
- Serrano, S.
- Sevilla-Noarbe, I.
- Smith, R.C.
- Soares-Santos, M.
- Sobreira, F.
- Suchyta, E.
- Swanson, M.E.C.
- Tarle, G.
- Thomas, D.
- Troxel, M.A.
- Tucker, D.L.
- Vikram, V.
- Walker, A.R.
- Zhang, Y.
DOIAbstract
International audienceWe present the analysis underpinning the measurement of cosmological parameters from 207 spectroscopically classified type Ia supernovae (SNe Ia) from the first three years of the Dark Energy Survey Supernova Program (DES-SN), spanning a redshift range of 0.01
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