{"paper":{"title":"Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas, A. Carnero Rosell, A. Drlica-Wagner, A. E. Evrard, A. J. Ross, A. Manzotti, A. R. Liddle, A. Roodman, A. R. Walker, B. A. Benson, B. Flaugher, B. Hoyle, B. Jain, C. B. D'Andrea, C. Davis, C. E. Cunha, C. L. Chang, C. L. Reichardt, D. Brooks, DES Collaboration: T. M. C. Abbott, D. Gruen, D. J. James, D. L. Burke, D. Thomas, D. W. Gerdes, E. Bertin, E. Fernandez, E. Gaztanaga, E. Krause, E. Rozo, E. Sanchez, E. S. Rykoff, E. Suchyta, F. B. Abdalla, F. J. Castander, F. Sobreira, G. Gutierrez, G. M. Bernstein, G. Tarle, H. Lin, H. T. Diehl, I. Sevilla-Noarbe, J. Annis, J. Carretero, J. Frieman, J. Garcia-Bellido, J. Gschwend, J. J. Mohr, J. L. Marshall, J. P. Dietrich, J. Weller, J. W. Henning, J. Zuntz, K. Bechtol, K. Honscheid, K. Kuehn, K. Reil, L. N. da Costa, M. A. G. Maia, M. A. Troxel, M. Carrasco Kind, M. D. Johnson, M. Jarvis, M. Lima, M. March, M. Schubnell, M. Smith, M. Soares-Santos, M. W. G. Johnson, N. Kuropatkin, O. Lahav, P. Doel, P. Nugent, R. A. Bernstein, R. A. Gruendl, R. C. Smith, R. H. Wechsler, R. L. C. Ogando, R. Miquel, S. Desai, S. Kuhlmann, T. Giannantonio, T. Jeltema, T. M. Crawford, T. Natoli, V. Scarpine, W. G. Hartley, W. L. K. Wu, W. Wester, Y. Park","submitted_at":"2017-11-01T15:42:57Z","abstract_excerpt":"We combine Dark Energy Survey Year 1 clustering and weak lensing data with Baryon Acoustic Oscillations (BAO) and Big Bang Nucleosynthesis (BBN) experiments to constrain the Hubble constant. Assuming a flat $\\Lambda$CDM model with minimal neutrino mass ($\\sum m_\\nu = 0.06$ eV) we find $H_0=67.2^{+1.2}_{-1.0}$ km/s/Mpc (68% CL). This result is completely independent of Hubble constant measurements based on the distance ladder, Cosmic Microwave Background (CMB) anisotropies (both temperature and polarization), and strong lensing constraints. There are now five data sets that: a) have no shared o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.00403","kind":"arxiv","version":1},"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"}