Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
- Abbott, T.M.C.
- Abdalla, F.B.
- Alarcon, A.
- Allam, S.
- Annis, J.
- Avila, S.
- Aylor, K.
- Banerji, M.
- Banik, N.
- Baxter, E.J.
- Bechtol, K.
- Becker, M.R.
- Benson, B.A.
- Bernstein, G.M.
- Bertin, E.
- Bianchini, F.
- Blazek, J.
- Bleem, L.E.
- Bridle, S.L.
- Brooks, D.
- Buckley-Geer, E.
- Burke, D.L.
- Carlstrom, J.E.
- Carnero Rosell, A.
- Carrasco Kind, M.
- Carretero, J.
- Castander, F.J.
- Cawthon, R.
- Chang, C.L.
- Cho, H-M.
- Choi, A.
- Chown, R.
- Crawford, T.M.
- Crites, A.T.
- Crocce, M.
- Cunha, C.E.
- D'Andrea, C.B.
- Da Costa, L.N.
- Davis, C.
- De Haan, T.
- DeRose, J.
- Desai, S.
- De Vicente, J.
- Diehl, H.T.
- Dietrich, J.P.
- Dobbs, M.A.
- Dodelson, S.
- Doel, P.
- Drlica-Wagner, A.
- Eifler, T.F.
- Elvin-Poole, J.
- Everett, W.B.
- Flaugher, B.
- Fosalba, P.
- Friedrich, O.
- Frieman, J.
- García-Bellido, J.
- Gatti, M.
- Gaztanaga, E.
- George, E.M.
- Gerdes, D.W.
- Giannantonio, T.
- Gruen, D.
- Gruendl, R.A.
- Gschwend, J.
- Gutierrez, G.
- Halverson, N.W.
- Harrington, N.L.
- Hartley, W.G.
- Holder, G.P.
- Hollowood, D.L.
- Holzapfel, W.L.
- Honscheid, K.
- Hou, Z.
- Hoyle, B.
- Hrubes, J.D.
- Huterer, D.
- Jain, B.
- James, D.J.
- Jarvis, M.
- Jeltema, T.
- Johnson, M.W.G.
- Johnson, M.D.
- Kent, S.
- Kirk, D.
- Knox, L.
- Kokron, N.
- Krause, E.
- Kuehn, K.
- Lahav, O.
- Lee, A.T.
- Leitch, E.M.
- Li, T.S.
- Lima, M.
- Lin, H.
- Luong-Van, D.
- MacCrann, N.
- Maia, M.A.G.
- Manzotti, A.
- Marrone, D.P.
- Marshall, J.L.
- Martini, P.
- McMahon, J.J.
- Menanteau, F.
- Meyer, S.S.
- Miquel, R.
- Mocanu, L.M.
- Mohr, J.J.
- Muir, J.
- Natoli, T.
- Nicola, A.
- Nord, B.
- Omori, Y.
- Padin, S.
- Pandey, S.
- Plazas, A.A.
- Porredon, A.
- Prat, J.
- Pryke, C.
- Rau, M.M.
- Reichardt, C.L.
- Rollins, R.P.
- Romer, A.K.
- Roodman, A.
- Ross, A.J.
- ROZO, E.
- Ruhl, J.E.
- Rykoff, E.S.
- Samuroff, S.
- Sánchez, C.
- Sanchez, E.
- Sayre, J.T.
- Scarpine, V.
- Schaffer, K.K.
- Secco, L.F.
- Serrano, S.
- Sevilla-Noarbe, I.
- Sheldon, E.
- Shirokoff, E.
- Simard, G.
- Smith, M.
- Soares-Santos, M.
- Sobreira, F.
- Staniszewski, Z.
- Stark, A.A.
- Story, K.T.
- Suchyta, E.
- Swanson, M.E.C.
- Tarle, G.
- Thomas, D.
- Troxel, M.A.
- Tucker, D.L.
- Vanderlinde, K.
- Vieira, J.D.
- Vielzeuf, P.
- Vikram, V.
- Walker, A.R.
- Wechsler, R.H.
- Weller, J.
- Williamson, R.
- Wu, W.L.K.
- Yanny, B.
- Zahn, O.
- Zhang, Y.
- Zuntz, J.
DOIAbstract
International audienceWe perform a joint analysis of the auto and cross-correlations between three cosmic fields: the galaxy density field, the galaxy weak lensing shear field, and the cosmic microwave background (CMB) weak lensing convergence field. These three fields are measured using roughly 1300 sq. deg. of overlapping optical imaging data from first year observations of the Dark Energy Survey (DES) and millimeter-wave observations of the CMB from both the South Pole Telescope Sunyaev-Zel’dovich survey and Planck. We present cosmological constraints from the joint analysis of the two-point correlation functions between galaxy density and galaxy shear with CMB lensing. We test for consistency between these measurements and the DES-only ...
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