{"paper":{"title":"A Uniform Analysis of Debris Disks with the Gemini Planet Imager II: Constraints on Dust Density Distribution Using Empirically-Informed Scattering Phase Functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Alycia J. Weinberger, Amaya Moro-Martin, A. Meredith Hughes, Bin B. Ren, Brenda C. Matthews, Briley L. Lewis, Christine H. Chen, Christopher C. Stark, David J. Wilner, Dean C. Hines, Deborah Padgett, Eileen C. Gonzales, Elodie Choquet, Eric L. Nielsen, Erika Nesvold, Franck Marchis, Frederik Rantakyr\\\"o, Gaspard Duch\\^ene, Glenn Schneider, Inseok Song, Jennifer Patience, Jessica Donaldson, Johan Mazoyer, John Debes, Justin Hom, Katie A. Crotts, Laurent Pueyo, Ludmilla Kolokolova, Malena Rice, Marshall D. Perrin, Maxwell A. Millar-Blanchaer, Michael P. Fitzgerald, Paul Kalas, Rebecca Oppenheimer, Rem\\'i Soummer, Robert J. De Rosa, Ronald A. L\\'opez, Sasha Hinkley, Schuyler G. Wolff, Sebasti\\'an Bruzzone, Stanimir Metchev, Thomas M. Esposito, Zachary Draper","submitted_at":"2024-01-31T22:27:36Z","abstract_excerpt":"Spatially-resolved images of debris disks are necessary to determine disk morphological properties and the scattering phase function (SPF) which quantifies the brightness of scattered light as a function of phase angle. Current high-contrast imaging instruments have successfully resolved several dozens of debris disks around other stars, but few studies have investigated trends in the scattered-light, resolved population of debris disks in a uniform and consistent manner. We have combined Karhunen-Loeve Image Projection (KLIP) with radiative-transfer disk forward modeling in order to obtain th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.00214","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2402.00214/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}