{"paper":{"title":"The FMOS-COSMOS survey of star-forming galaxies at $z\\sim1.6$. V: Properties of dark matter halos containing H$\\alpha$ emitting galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alvio Renzini, Annagrazia Puglisi, Daichi Kashino, David B. Sanders, Emanuele Daddi, Francesco Valentino, Giulia Rodighiero, Jeyhan S. Kartaltepe, John D. Silverman, Masaru Kajisawa, Naoshi Sugiyama, Nobuo Arimoto, Olivier Le F\\`evre, Surhud More","submitted_at":"2017-03-24T09:38:41Z","abstract_excerpt":"We study the properties of dark matter halos that contain star-forming galaxies at $1.43 \\le z \\le 1.74$ using the FMOS-COSMOS survey. The sample consists of 516 objects with a detection of the H$\\alpha$ emission line, that represent the star-forming population at this epoch having a stellar mass range of $10^{9.57}\\le M_\\ast/M_\\odot \\lesssim 10^{11.4}$ and a star formation rate range of $15\\lesssim \\mathrm{SFR}/(M_\\odot \\mathrm{yr^{-1}}) \\lesssim 600$. We measure the projected two-point correlation function while carefully taking into account observational biases, and find a significant clust"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.08326","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"}