Dark Energy Survey Year 3 results: galaxy clustering and systematics treatment for lens galaxy samples
- Rodriguez-Monroy, M.
- Weaverdyck, N.
- Elvin-Poole, J.
- Crocce, M.
- Carnero Rosell, A.
- Andrade-Oliveira, F.
- Avila, S.
- Bechtol, K.
- Bernstein, G. M.
- Blazek, J.
- Camacho, H.
- Cawthon, R.
- De Vicente, J.
- DeRose, J.
- Dodelson, S.
- Everett, S.
- Fang, X.
- Ferrero, I
- Ferte, A.
- Friedrich, O.
- Gaztanaga, E.
- Giannini, G.
- Gruendl, R. A.
- Hartley, W. G.
- Herner, K.
- Huff, E. M.
- Jarvis, M.
- Krause, E.
- MacCrann, N.
- Mena-Fernandez, J.
- Muir, J.
- Pandey, S.
- Park, Y.
- Porredon, A.
- Prat, J.
- Rosenfeld, R.
- Ross, A. J.
- Rozo, E.
- Rykoff, E. S.
- Sanchez, E.
- Sanchez Cid, D.
- Sevilla-Noarbe, I
- Tabbutt, M.
- To, C.
- Wagoner, E. L.
- Wechsler, R. H.
- Aguena, M.
- Allam, S.
- Amon, A.
- Annis, J.
- Bacon, D.
- Baxter, E.
- Bertin, E.
- Bhargava, S.
- Brooks, D.
- Burke, D. L.
- Carrasco Kind, M.
- Carretero, J.
- Castander, F. J.
- Choi, A.
- Conselice, C.
- Costanzi, M.
- da Costa, L. N.
- Pereira, M. E. S.
- Desai, S.
- Diehl, H. T.
- Flaugher, B.
- Fosalba, P.
- Frieman, J.
- Garcia-Bellido, J.
- Giannantonio, T.
- Gruen, D.
- Gschwend, J.
- Gutierrez, G.
- Hinton, S. R.
- Hollowood, D. L.
- Honscheid, K.
- Huterer, D.
- Jain, B.
- James, D. J.
- Kuehn, K.
- Kuropatkin, N.
- Lima, M.
- Maia, M. A. G.
- March, M.
- Marshall, J. L.
- Melchior, P.
- Menanteau, F.
- Miller, C. J.
- Miquel, R.
- Mohr, J. J.
- Morgan, R.
- Palmese, A.
- Paz-Chinchon, F.
- Pieres, A.
- Plazas Malagon, A. A.
- Roodman, A.
- Scarpine, V
- Serrano, S.
- Smith, M.
- Soares-Santos, M.
- Suchyta, E.
- Tarle, G.
- Thomas, D.
- Varga, T. N.
DOIAbstract
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a magnitude-limited sample optimized for the measurement of cosmological parameters, MAGLIM, and a sample of luminous red galaxies selected with the REDMAGIC algorithm. MAGLIM/REDMAGIC sample contains over 10 million/2.5 million galaxies and is divided into six/five photometric redshift bins spanning the range z is an element of [0.20, 1.05]/z is an element of [0.15, 0.90]. Both samples cover 4143 deg(2) over which we perform our analysis blind, measuring the angular correlation function with an S/N similar to 63 for both samples. In a companion paper, these measurements of galaxy clustering are combined with the correlation functions of cosmic s...
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