{"paper":{"title":"The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\\sim2$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akira Konno, Haruka Kusakabe, John D. Silverman, Kazuhiro Shimasaku, Kimihiko Nakajima, Masami Ouchi, Peter L. Capak, Ryosuke Goto, Takuya Hashimoto, Yuichi Harikane","submitted_at":"2017-07-28T18:01:36Z","abstract_excerpt":"We present average stellar population properties and dark matter halo masses of $z \\sim 2$ \\lya emitters (LAEs) from SED fitting and clustering analysis, respectively, using $\\simeq$ $1250$ objects ($NB387\\le25.5$) in four separate fields of $\\simeq 1$ deg$^2$ in total. With an average stellar mass of $10.2\\, \\pm\\, 1.8\\times 10^8\\ {\\mathrm M_\\odot}$ and star formation rate of $3.4\\, \\pm\\, 0.4\\ {\\mathrm M_\\odot}\\ {\\rm yr^{-1}}$, the LAEs lie on an extrapolation of the star-formation main sequence (MS) to low stellar mass. Their effective dark matter halo mass is estimated to be $4.0_{-2.9}^{+5."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.09373","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"}