{"paper":{"title":"Faint 6.7um Galaxies and their Contributions to the Stellar Mass Density in the Universe","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) U. Hawaii, (3) ISAS/Japan Aerospace Exploration Agency, (4) Gunma Astronomical Observatory, (5) Tohoku U., (6) Gifu U., 7), (7) MPE), David B. Sanders (2, Haruyuki Okuda (4), Hideo Matsuhara (3), Ken-ichi Wakamatsu (6) ((1) U. Tokyo, Kimiaki Kawara (1), Lennox L. Cowie (2), Yasunori Sato (1), Yoshiaki Sofue (2), Yoshiaki Taniguchi (5)","submitted_at":"2003-12-04T05:21:02Z","abstract_excerpt":"We discuss the nature of faint 6.7um galaxies detected with the mid-infrared camera ISOCAM on board the Infrared Space Observatory (ISO). The 23 hour integration on the Hawaii Deep Field SSA13 has provided a sample of 65 sources down to 6uJy at 6.7um. For 57 sources, optical or near-infrared counterparts were found with a statistical method. All four Chandra sources, three SCUBA sources, and one VLA/FIRST source in this field were detected at 6.7um with high significance. Using their optical to mid-infrared colors, we divided the 6.7um sample into three categories: low redshift galaxies with p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0312114","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"}