{"paper":{"title":"Spitzer Observations of the North Ecliptic Pole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, A. Lanz, C. Pearson, D. H. Lee, D. L. Clements, H. Matsuhara, H. M. Lee, H. Nayyeri, J. Bock, J. Smidt, K. Tsumura, M. G. Kim, M. Im, M. Malkan, M. Zemcov, N. Ghotbi, P. Korngut, S. Matsuura, S. Serjeant, T. Matsumoto, T. Wada, U. W. Nam","submitted_at":"2017-12-04T19:00:02Z","abstract_excerpt":"We present a photometric catalog for Spitzer Space Telescope warm mission observations of the North Ecliptic Pole (NEP; centered at $\\rm R.A.=18^h00^m00^s$, $\\rm Decl.=66^d33^m38^s.552$). The observations are conducted with IRAC in 3.6 $\\mu$m and 4.5 $\\mu$m bands over an area of 7.04 deg$^2$ reaching 1$\\sigma$ depths of 1.29 $\\mu$Jy and 0.79 $\\mu$Jy in the 3.6 $\\mu$m and 4.5 $\\mu$m bands respectively. The photometric catalog contains 380,858 sources with 3.6 $\\mu$m and 4.5 $\\mu$m band photometry over the full-depth NEP mosaic. Point source completeness simulations show that the catalog is 80% "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.01290","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"}