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Dark Energy Survey year 1 results: Galaxy clustering for combined probes

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journal contribution
posted on 2024-08-06, 11:42 authored by J. Elvin-Poole, M. Crocce, A. J. Ross, T. Giannantonio, E. Rozo, E. S. Rykoff, S. Avila, N. Banik, J. Blazek, S. L. Bridle, R. Cawthon, A. Drlica-Wagner, O. Friedrich, N. Kokron, E. Krause, N. Maccrann, J. Prat, C. Sánchez, L. F. Secco, I. Sevilla-Noarbe, M. A. Troxel, T. M.C. Abbott, F. B. Abdalla, S. Allam, J. Annis, Jacobo Asorey Barreiro, K. Bechtol, M. R. Becker, A. Benoit-Lévy, G. M. Bernstein, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, F. J. Castander, C. E. Cunha, C. B. D'Andrea, L. N. Da Costa, T. M. Davis, C. Davis, S. Desai, H. T. Diehl, J. P. Dietrich, S. Dodelson, P. Doel, T. F. Eifler, A. E. Evrard, E. Fernandez, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. W. Gerdes, Karl GlazebrookKarl Glazebrook, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, S. R. Hinton, K. Honscheid, J. K. Hoormann, B. Jain, D. J. James, M. Jarvis, T. Jeltema, M. W.G. Johnson, M. D. Johnson, A. King, K. Kuehn, S. Kuhlmann, N. Kuropatkin, O. Lahav, G. Lewis, T. S. Li, C. Lidman, M. Lima, H. Lin, E. Macaulay, M. March, J. L. Marshall, P. Martini, P. Melchior, F. Menanteau, R. Miquel, J. J. Mohr, Anais MollerAnais Moller, R. C. Nichol, B. Nord, C. R. O'Neill, W. J. Percival, D. Petravick, A. A. Plazas, A. K. Romer, M. Sako, E. Sanchez, V. Scarpine, R. Schindler, M. Schubnell, E. Sheldon, M. Smith, R. C. Smith, M. Soares-Santos, F. Sobreira, N. E. Sommer, E. Suchyta, M. E.C. Swanson, G. Tarle, D. Thomas, B. E. Tucker, D. L. Tucker, S. A. Uddin, V. Vikram, A. R. Walker, R. H. Wechsler, J. Weller, W. Wester, R. C. Wolf, F. Yuan, B. Zhang, J. Zuntz
We measure the clustering of DES year 1 galaxies that are intended to be combined with weak lensing samples in order to produce precise cosmological constraints from the joint analysis of large-scale structure and lensing correlations. Two-point correlation functions are measured for a sample of 6.6×105 luminous red galaxies selected using the redMaGiC algorithm over an area of 1321 square degrees, in the redshift range 0.15

Funding

ARC Centre of Excellence for All-sky Astrophysics

Australian Research Council

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PDF (Published version)

ISSN

2470-0029

Journal title

Physical Review D

Volume

98

Issue

4

Article number

article no. 042006

Pagination

042006-

Publisher

American Physical Society

Copyright statement

Copyright © 2018 American Physical Society. The published version is reproduced in accordance with the copyright policy of the publisher.

Language

eng

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