{"paper":{"title":"Asteroid Distributions in the Ecliptic","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrea Dipaolo, Charles E. Woodward, Emanuele Giallongo, Erin L. Ryan, Fernando Pedichini, Jacopo Farinato, John Hill, Richard Pogge, Roberto Ragazzoni, Roland Gredel","submitted_at":"2009-03-25T21:53:41Z","abstract_excerpt":"We present analysis of the asteroid surface density distribution of main belt asteroids (mean perihelion $\\Delta \\simeq 2.404$ AU) in five ecliptic latitude fields, $-17 \\gtsimeq \\beta(\\degr) \\ltsimeq +15$, derived from deep \\textit{Large Binocular Telescope} (LBT) $V-$band (85% completeness limit $V = 21.3$ mag) and \\textit{Spitzer Space Telescope} IRAC 8.0 \\micron (80% completeness limit $\\sim 103 \\mu$Jy) fields enabling us to probe the 0.5--1.0 km diameter asteroid population. We discovered 58 new asteroids in the optical survey as well as 41 new bodies in the \\textit{Spitzer} fields. The d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0903.4479","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"}