{"paper":{"title":"Quasars in the Galactic Anti-Center Area from the LAMOST DR3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hai-Bo Yuan, Jian-Ling Wang, Jian-Nan Zhang, Jian-rong Shi, Mao-Sheng Xiang, Wei Zhang, Xiao-Wei Liu, Yang Huang, Yong-Hui Hou, Yong Zhang, Yue-Fei Wang, Yu-Zhong Wu, Zhi-ying Huo, Zi-Huang Cao","submitted_at":"2017-02-06T08:47:20Z","abstract_excerpt":"We present a sample of quasars discovered in the area of Galactic Anti-Center (GAC) of $150^{\\circ} \\leq l \\leq 210^{\\circ}$ and $|b| \\leq 30^{\\circ}$, based on the LAMOST Data Release 3 (DR3). The sample contains 151 spectroscopically confirmed quasars. Among them 80 are newly discovered with the LAMOST. All those quasars are very bright, with $i$ magnitudes peaking around 17.5\\, mag. All the newly quasars are discovered serendipitously, targeted originally with the LAMOST as stars of bluer colours, except for a few targeted as variable, young stellar object candidates. This bright quasar sam"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.01531","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"}