{"paper":{"title":"IGRINS Spectral Library","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chan Park, Daniel T. Jaffe, Gregory N. Mace, Hwihyun Kim, In-Soo Yuk, Jae-Joon Lee, Jae Sok Oh, Jeong-Eun Lee, Kang-Min Kim, Kyle F. Kaplan, Moo-Young Chun, Sang-Gak Lee, Sungho Lee, Sunkyung Park, Wonseok Kang","submitted_at":"2018-08-20T18:04:56Z","abstract_excerpt":"We present a library of high-resolution (R $\\equiv$ $\\lambda$/$\\Delta$$\\lambda$ $\\sim$ 45,000) and high signal-to-noise ratio (S/N $\\geq$ 200) near-infrared spectra for stars of a wide range of spectral types and luminosity classes. The spectra were obtained with the Immersion GRating INfrared Spectrograph (IGRINS) covering the full range of the H (1.496-1.780 $\\mu$m) and K (2.080-2.460 $\\mu$m) atmospheric windows. The targets were primarily selected for being MK standard stars covering a wide range of effective temperatures and surface gravities with metallicities close to the Solar value. Cu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.06629","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"}