{"paper":{"title":"Cosmological Constraints from Multiple Probes in the Dark Energy Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. A. Plazas, A. Avelino, A. Campos, A. Carnero Rosell, A. Clocchiatti, A. Drlica-Wagner, A. E. Evrard, A. G. Kim, A. J. Ross, A. K. Romer, A. M\\\"oller, A. Palmese, A. Porredon, A. Roodman, A. R. Walker, A. V. Filippenko, B. A. Bassett, B. E. Tucker, B. Flaugher, B. Hoyle, B. Jain, B. Nord, B. Yanny, B. Zhang, C. B. D'Andrea, C. Chang, C. Davis, C. E. Cunha, C. Lidman, C. S\\'anchez, D. A. Goldstein, D. Bacon, D. Brooks, D. Brout, D. Carollo, DES Collaboration: T. M. C. Abbott, D. Gruen, D. Huterer, D. J. James, D. L. Burke, D. L. DePoy, D. L. Hollowood, D. Scolnic, D. Thomas, D. W. Gerdes, E. Baxter, E. Bertin, E. Fernandez, E. Gaztanaga, E. Kasai, E. Krause, E. Macaulay, E. Morganson, E. Neilsen, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Swann, F. Andrade-Oliveira, F. J. Castander, F. Menanteau, F. Sobreira, G. F. Lewis, G. Gutierrez, G. M. Bernstein, G. Tarle, H. Camacho, H. Lin, H. T. Diehl, H. V. Peiris, I. Sevilla-Noarbe, J. Annis, J. Asorey, J. Blazek, J. Calcino, J. Carretero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Estrada, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. J. Mohr, J. K. Hoormann, J. Lasker, J. L. Marshall, J. Marriner, J. Muir, J. P. Dietrich, J. Prat, J. Weller, J. Zuntz, K. Bechtol, K. C. Chan, K. Glazebrook, K. Honscheid, K. Kuehn, K. S. Mandel, L. F. Secco, L. Galbany, L. N. da Costa, M. A. G. Maia, M. A. Troxel, M. Carrasco Kind, M. Childress, M. Crocce, M. E. C. Swanson, M. Gatti, M. Jarvis, M. Lima, M. March, M. R. Becker, M. Schubnell, M. Smith, M. Soares-Santos, M. Wang, N. Banik, N. E. Sommer, N. Kokron, N. Kuropatkin, N. MacCrann, N. Weaverdyck, O. Lahav, P. Andersen, P. Challis, P. Doel, P. Fosalba, P. Lemos, P. Martini, P. Melchior, P. Vielzeuf, R. A. Gruendl, R. Cawthon, R. C. Nichol, R. C. Thomas, R. G. McMahon, R. H. Wechsler, R. J. Foley, R. Kessler, R. Kron, R. L. C. Ogando, R. Miquel, R. P. Kirshner, R. Rosenfeld, R. Schindler, R. Sharp, S. Allam, S. A. Uddin, S. Avila, S. Desai, S. Dodelson, S. Kent, S. L. Bridle, S. R. Hinton, S. Samuroff, S. Serrano, T. F. Eifler, T. Giannantonio, T. Jeltema, T. M. Davis, T. S. Li, V. Scarpine, W. G. Hartley, W. J. Percival, Y.-C. Pan, Y. Zhang","submitted_at":"2018-11-06T14:42:50Z","abstract_excerpt":"The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically--confirmed Type Ia supernova lightcurves; the baryon acoustic oscillation feature; weak gravitational lensing; and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, $w$, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave bac"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.02375","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}