Macaulay, E; Nichol, RC; Bacon, D; Brout, D; Davis, TM; Zhang, B; Bassett, BA; Scolnic, D; Möller, A; D’Andrea, CB; Hinton, SR; Kessler, R; Kim, AG; Lasker, J; Lidman, C; Sako, M; Smith, M; Sullivan, M; Abbott, TMC; Allam, S; Annis, J; Asorey, J; Avila, S; Bechtol, K; Brooks, D; Brown, P; Burke, DL; Calcino, J; Rosell, A Carnero; Carollo, D; Kind, M Carrasco; Carretero, J; Castander, FJ; Collett, T; Crocce, M; Cunha, CE; da Costa, LN; Davis, C; De Vicente, J; Diehl, HT; Doel, P; Drlica-Wagner, A; Eifler, TF; Estrada, J; Evrard, AE; Filippenko, AV; Finley, DA; Flaugher, B; Foley, RJ; Fosalba, P; Frieman, J; Galbany, L; García-Bellido, J; Gaztanaga, E; Glazebrook, K; González-Gaitán, S; Gruen, D; Gruendl, RA; Gschwend, J; Gutierrez, G; Hartley, WG; Hollowood, DL; Honscheid, K; Hoormann, JK; Hoyle, B; Huterer, D; Jain, B; James, DJ; Jeltema, T; Kasai, E; Krause, E; Kuehn, K; Kuropatkin, N; Lahav, O; Lewis, GF; Li, TS; Lima, M; Lin, H; Maia, MAG; Marshall, JL; Martini, P; Miquel, R; Nugent, P; Palmese, A; Pan, Y-C

doi:10.1093/mnras/stz978

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First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant

2019

Macaulay, E;
Nichol, RC;
Bacon, D;
Brout, D;
Davis, TM;
Zhang, B;
Bassett, BA;
Scolnic, D;
Möller, A;
D’Andrea, CB;
Hinton, SR;
Kessler, R;
Kim, AG;
Lasker, J;
Lidman, C;
Sako, M;
Smith, M;
Sullivan, M;
Abbott, TMC;
Allam, S;
Annis, J;
Asorey, J;
Avila, S;
Bechtol, K;
Brooks, D;
Brown, P;
Burke, DL;
Calcino, J;
Rosell, A Carnero;
Carollo, D;
Kind, M Carrasco;
Carretero, J;
Castander, FJ;
Collett, T;
Crocce, M;
Cunha, CE;
da Costa, LN;
Davis, C;
De Vicente, J;
Diehl, HT;
Doel, P;
Drlica-Wagner, A;
Eifler, TF;
Estrada, J;
Evrard, AE;
Filippenko, AV;
Finley, DA;
Flaugher, B;
Foley, RJ;
Fosalba, P;
Frieman, J;
Galbany, L;
García-Bellido, J;
Gaztanaga, E;
Glazebrook, K;
González-Gaitán, S;
Gruen, D;
Gruendl, RA;
Gschwend, J;
Gutierrez, G;
Hartley, WG;
Hollowood, DL;
Honscheid, K;
Hoormann, JK;
Hoyle, B;
Huterer, D;
Jain, B;
James, DJ;
Jeltema, T;
Kasai, E;
Krause, E;
Kuehn, K;
Kuropatkin, N;
Lahav, O;
Lewis, GF;
Li, TS;
Lima, M;
Lin, H;
Maia, MAG;
Marshall, JL;
Martini, P;
Miquel, R;
Nugent, P;
Palmese, A;
Pan, Y-C;
Plazas, AA;
Romer, AK;
Roodman, A;
Sanchez, E;
Scarpine, V;
Schindler, R;
Schubnell, M;
Serrano, S;
Sevilla-Noarbe, I;
Sharp, R;
Soares-Santos, M;
Sobreira, F;
Sommer, NE;
Suchyta, E;
Swann, E;
Swanson, MEC;
Tarle, G;
Thomas, D;
Thomas, RC;
Tucker, BE;
Uddin, SA;
Vikram, V;
Walker, AR;
Wiseman, P
et al.

Published Web Location

https://doi.org/10.1093/mnras/stz978

Abstract

We present an improved measurement of the Hubble constant (H0) using the 'inverse distance ladder' method, which adds the information from 207 Type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) at redshift 0.018

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UC Santa Cruz

First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant

Published Web Location