{"paper":{"title":"Kuiper Belts Around Nearby Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"1), 10) ((1) Department of Astronomy, (10) Science, (2) Onsala Space Observatory, (3) ESA Astrophysics Missions Division, (4) SRON, (5) ESA/ESTEC Space Environment, (6) Universit\\'e Joseph Fourier/CNRS, (7) Dpto. F\\'isica Te\\'orica, (8) Observatoire de Paris, (9) Department of Physics, A. Brandeker (1), Astronomy, C. Eiroa (7), Chalmers University of Technology, C. Risacher (4), Didcot, Effects Section, ESTEC, Facultad de Ciencias, France, G. J. White (9, G. L. Pilbratt (3), G. Olofsson (1), Grenoble, Groningen, J.-C. Augereau (6), J. Rodmann (5), Laboratoire d'Astrophysique de Grenoble, Madrid, M. Fridlund (3), Milton Keynes, Noordwijk, Onsala, Open University, P. Bergman (2), P. Th\\'ebault (8, R. Liseau (2), R. Nilsson (1), Rutherford Appleton Laboratory, section de Meudon, Spain, Stockholm, Stockholm University, Sweden, Technology Facilities Council, The Netherlands, UK, UK), Universidad Aut\\'onoma de Madrid","submitted_at":"2010-05-18T14:42:13Z","abstract_excerpt":"In order to detect and characterise cold extended circumstellar dust originating from collisions of planetesimal bodies in disks, belts, or rings at Kuiper-Belt distances (30-50 AU or beyond) sensitive submillimetre observations are essential. Measurements of the flux densities at these wavelengths will extend existing IR photometry and permit more detailed modelling of the Rayleigh-Jeans tail of the disks spectral energy distribution (SED), effectively constraining dust properties and disk extensions. By observing stars spanning from a few up to several hundred Myr, the evolution of debris di"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.3215","kind":"arxiv","version":2},"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"}