Skip to main content
Download PDF
- Main
Dark Energy Survey year 1 results: Galaxy-galaxy lensing
- Prat, J;
- Sánchez, C;
- Fang, Y;
- Gruen, D;
- Elvin-Poole, J;
- Kokron, N;
- Secco, LF;
- Jain, B;
- Miquel, R;
- MacCrann, N;
- Troxel, MA;
- Alarcon, A;
- Bacon, D;
- Bernstein, GM;
- Blazek, J;
- Cawthon, R;
- Chang, C;
- Crocce, M;
- Davis, C;
- De Vicente, J;
- Dietrich, JP;
- Drlica-Wagner, A;
- Friedrich, O;
- Gatti, M;
- Hartley, WG;
- Hoyle, B;
- Huff, EM;
- Jarvis, M;
- Rau, MM;
- Rollins, RP;
- Ross, AJ;
- Rozo, E;
- Rykoff, ES;
- Samuroff, S;
- Sheldon, E;
- Varga, TN;
- Vielzeuf, P;
- Zuntz, J;
- Abbott, TMC;
- Abdalla, FB;
- Allam, S;
- Annis, J;
- Bechtol, K;
- Benoit-Lévy, A;
- Bertin, E;
- Brooks, D;
- Buckley-Geer, E;
- Burke, DL;
- Rosell, A Carnero;
- Kind, M Carrasco;
- Carretero, J;
- Castander, FJ;
- Cunha, CE;
- D’Andrea, CB;
- da Costa, LN;
- Desai, S;
- Diehl, HT;
- Dodelson, S;
- Eifler, TF;
- Fernandez, E;
- Flaugher, B;
- Fosalba, P;
- Frieman, J;
- García-Bellido, J;
- Gaztanaga, E;
- Gerdes, DW;
- Giannantonio, T;
- Goldstein, DA;
- Gruendl, RA;
- Gschwend, J;
- Gutierrez, G;
- Honscheid, K;
- James, DJ;
- Jeltema, T;
- Johnson, MWG;
- Johnson, MD;
- Kirk, D;
- Krause, E;
- Kuehn, K;
- Kuhlmann, S;
- Lahav, O;
- Li, TS;
- Lima, M;
- Maia, MAG;
- March, M;
- Marshall, JL;
- Martini, P;
- Melchior, P;
- Menanteau, F;
- Mohr, JJ;
- Nichol, RC;
- Nord, B;
- Plazas, AA;
- Romer, AK;
- Roodman, A;
- Sako, M;
- Sanchez, E;
- Scarpine, V;
- Schindler, R;
- Schubnell, M;
- Sevilla-Noarbe, I;
- Smith, M;
- Smith, RC;
- Soares-Santos, M;
- Sobreira, F;
- Suchyta, E;
- Swanson, MEC;
- Tarle, G;
- Thomas, D;
- Tucker, DL;
- Vikram, V;
- Walker, AR;
- Wechsler, RH;
- Yanny, B;
- Zhang, Y
Published Web Location
https://doi.org/10.1103/physrevd.98.042005Abstract
We present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark Energy Survey (DES) Year 1 (Y1) data. The lens sample consists of a selection of 660,000 red galaxies with high-precision photometric redshifts, known as redMaGiC, split into five tomographic bins in the redshift range 0.15
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.