{"paper":{"title":"The ALHAMBRA survey: evolution of galaxy clustering since $z \\sim 1$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(10) Univ. of Missouri, (11) ON-MCT, (12) UPV/EHU, (13) Univ. de Sevilla, (14) PUC, (2) OAUV, 3), (3) IFCA, (4) IAA, (5) UCL, 6), (6) IAC, (7) ICE, (8) CEFCA, (9) Univ. of Utah, A. del Olmo (4), A. D. Montero-Dorta (9), A. Fern\\'andez-Soto (3), A. I. Merson (5), A. Molino (4), Barcelona, B. Ascaso (4), Bilbao, C. Husillos (4), C. L\\'opez-Sanjuan (8), D. Crist\\'obal-Hornillos (8), Durham, E. Alfaro (4), F. J. Castander (7), F. Prada (4), Granada, I. M\\'arquez (4), J. A. L. Aguerri (6), J. Cabrera-Ca\\~no (13), J. Cepa (6), J. Masegosa (4), J. M. Quintana (4) ((1) ICC, J. Perea (4), La Laguna, L. Hurtado-Gil (2, L. Infante (14), London, M. Cervi\\~no (4, M. Moles (8), M. Povi\\'c (4), M. Stefanon (10), N. Ben\\'itez (4), P. Arnalte-Mur (1), P. Norberg (1), Rio de Janeiro, R. M. Gonz\\'alez Delgado (4), Santander, Santiago), T. Aparicio-Villegas (11), T. Broadhurst (12), Teruel, Val\\`encia, V. J. Mart\\'inez (2)","submitted_at":"2013-11-13T20:23:46Z","abstract_excerpt":"We study the clustering of galaxies as function of luminosity and redshift in the range $0.35 < z < 1.25$ using data from the Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) survey. The ALHAMBRA data used in this work cover $2.38 \\mathrm{deg}^2$ in 7 independent fields, after applying a detailed angular selection mask, with accurate photometric redshifts, $\\sigma_z \\lesssim 0.014 (1+z)$, down to $I_{\\rm AB} < 24$. Given the depth of the survey, we select samples in $B$-band luminosity down to $L^{\\rm th} \\simeq 0.16 L^{*}$ at $z = 0.9$. We measure the real-space cl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.3280","kind":"arxiv","version":2},"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"}