{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ZRK3BYMDYOJHAURDLKKSQ5R5S2","short_pith_number":"pith:ZRK3BYMD","schema_version":"1.0","canonical_sha256":"cc55b0e183c3927052235a9528763d96960c0c2ae1c20c56d8aaeeea8dbfe215","source":{"kind":"arxiv","id":"1603.09357","version":1},"attestation_state":"computed","paper":{"title":"Constraining turbulence mixing strength in transitional discs with planets using SPHERE and ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"C. Dominik, M. de Juan Ovelar, M. Min, P. Pinilla, T. Birnstiel","submitted_at":"2016-03-30T20:03:15Z","abstract_excerpt":"We investigate the effect that the turbulent mixing strength parameter $\\alpha_{\\rm{turb}}$ plays on near-infrared polarimetric and sub-millimetre interferometric imaging observations of transitional discs (TDs) with a gap carved by a planet. We generate synthetic observations of these objects with ALMA and VLT/SPHERE-ZIMPOL by combining hydrodynamical, dust evolution, radiative transfer and instrument models for values of $\\alpha_{\\rm{turb}}=[10^{-4}, 10^{-3}, 10^{-2}]$. We find that, through a combination of effects on the viscosity of the gas, the turbulent mixing and dust evolution process"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1603.09357","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-03-30T20:03:15Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"a8e6e7d8510f03bb0f0eb8ca9942406a1a545b35144d766b0283c9845aaa5193","abstract_canon_sha256":"acec59a7fe7691d02a9b2c3b30ebf0c63064a30afd50c90542cadd1f8241561f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:58.891487Z","signature_b64":"kpEzkianF4qWIIaThVuJC3s/BaUUeUeTuRf0aoH/EHY8z6vJnvVzIt4vR/nHjVJBf8qpfTaubZuSy7ziw/3TDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc55b0e183c3927052235a9528763d96960c0c2ae1c20c56d8aaeeea8dbfe215","last_reissued_at":"2026-05-18T01:17:58.890765Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:58.890765Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining turbulence mixing strength in transitional discs with planets using SPHERE and ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"C. Dominik, M. de Juan Ovelar, M. Min, P. Pinilla, T. Birnstiel","submitted_at":"2016-03-30T20:03:15Z","abstract_excerpt":"We investigate the effect that the turbulent mixing strength parameter $\\alpha_{\\rm{turb}}$ plays on near-infrared polarimetric and sub-millimetre interferometric imaging observations of transitional discs (TDs) with a gap carved by a planet. We generate synthetic observations of these objects with ALMA and VLT/SPHERE-ZIMPOL by combining hydrodynamical, dust evolution, radiative transfer and instrument models for values of $\\alpha_{\\rm{turb}}=[10^{-4}, 10^{-3}, 10^{-2}]$. We find that, through a combination of effects on the viscosity of the gas, the turbulent mixing and dust evolution process"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.09357","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1603.09357","created_at":"2026-05-18T01:17:58.890868+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.09357v1","created_at":"2026-05-18T01:17:58.890868+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.09357","created_at":"2026-05-18T01:17:58.890868+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRK3BYMDYOJH","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRK3BYMDYOJHAURD","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRK3BYMD","created_at":"2026-05-18T12:30:55.937587+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2","json":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2.json","graph_json":"https://pith.science/api/pith-number/ZRK3BYMDYOJHAURDLKKSQ5R5S2/graph.json","events_json":"https://pith.science/api/pith-number/ZRK3BYMDYOJHAURDLKKSQ5R5S2/events.json","paper":"https://pith.science/paper/ZRK3BYMD"},"agent_actions":{"view_html":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2","download_json":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2.json","view_paper":"https://pith.science/paper/ZRK3BYMD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.09357&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRK3BYMDYOJHAURDLKKSQ5R5S2/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRK3BYMDYOJHAURDLKKSQ5R5S2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2/action/storage_attestation","attest_author":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2/action/author_attestation","sign_citation":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2/action/citation_signature","submit_replication":"https://pith.science/pith/ZRK3BYMDYOJHAURDLKKSQ5R5S2/action/replication_record"}},"created_at":"2026-05-18T01:17:58.890868+00:00","updated_at":"2026-05-18T01:17:58.890868+00:00"}