{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:QAMRSDVIG3YKA5Q6YCUP2RRNK7","short_pith_number":"pith:QAMRSDVI","schema_version":"1.0","canonical_sha256":"8019190ea836f0a0761ec0a8fd462d57d79514a32184b345746b09653b579cab","source":{"kind":"arxiv","id":"1201.1453","version":1},"attestation_state":"computed","paper":{"title":"Probing the turbulent mixing strength in protoplanetary disks across the stellar mass range: no significant variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Carsten Dominik, Gijs D. Mulders","submitted_at":"2012-01-06T17:17:36Z","abstract_excerpt":"Dust settling and grain growth are the first steps in the planet-formation process in protoplanetary disks. These disks are observed around stars with different spectral types, and there are indications that the disks around lower mass stars are significantly flatter, which could indicate that they settle and evolve faster, or in a different way.\n  We aim to test this assumption by modeling the median spectral energy distributions (SEDs) of three samples of protoplanetary disks: around Herbig stars, T Tauri stars and brown dwarfs. We focus on the turbulent mixing strength to avoid a strong obs"},"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":"1201.1453","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-01-06T17:17:36Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"6794b29b10826f08174459d887126d7554a4f2d246c82646be93a517b762d07f","abstract_canon_sha256":"b1bd204a2698bf33e52f30ffb88ce676c7af9deb1150a11bacf457b2970c40ae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:54.843823Z","signature_b64":"RCtUkAnG3sB5xr9QafUJjiK0R2D/latx5D+DkNiYMLMAvYKa6x1GTwIbrbySiqNZFluCkIPdOsBc1mjs3JHfBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8019190ea836f0a0761ec0a8fd462d57d79514a32184b345746b09653b579cab","last_reissued_at":"2026-05-18T01:58:54.843023Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:54.843023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing the turbulent mixing strength in protoplanetary disks across the stellar mass range: no significant variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Carsten Dominik, Gijs D. Mulders","submitted_at":"2012-01-06T17:17:36Z","abstract_excerpt":"Dust settling and grain growth are the first steps in the planet-formation process in protoplanetary disks. These disks are observed around stars with different spectral types, and there are indications that the disks around lower mass stars are significantly flatter, which could indicate that they settle and evolve faster, or in a different way.\n  We aim to test this assumption by modeling the median spectral energy distributions (SEDs) of three samples of protoplanetary disks: around Herbig stars, T Tauri stars and brown dwarfs. We focus on the turbulent mixing strength to avoid a strong obs"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1453","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":"1201.1453","created_at":"2026-05-18T01:58:54.843186+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.1453v1","created_at":"2026-05-18T01:58:54.843186+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1453","created_at":"2026-05-18T01:58:54.843186+00:00"},{"alias_kind":"pith_short_12","alias_value":"QAMRSDVIG3YK","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_16","alias_value":"QAMRSDVIG3YKA5Q6","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_8","alias_value":"QAMRSDVI","created_at":"2026-05-18T12:27:18.751474+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/QAMRSDVIG3YKA5Q6YCUP2RRNK7","json":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7.json","graph_json":"https://pith.science/api/pith-number/QAMRSDVIG3YKA5Q6YCUP2RRNK7/graph.json","events_json":"https://pith.science/api/pith-number/QAMRSDVIG3YKA5Q6YCUP2RRNK7/events.json","paper":"https://pith.science/paper/QAMRSDVI"},"agent_actions":{"view_html":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7","download_json":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7.json","view_paper":"https://pith.science/paper/QAMRSDVI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.1453&json=true","fetch_graph":"https://pith.science/api/pith-number/QAMRSDVIG3YKA5Q6YCUP2RRNK7/graph.json","fetch_events":"https://pith.science/api/pith-number/QAMRSDVIG3YKA5Q6YCUP2RRNK7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7/action/storage_attestation","attest_author":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7/action/author_attestation","sign_citation":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7/action/citation_signature","submit_replication":"https://pith.science/pith/QAMRSDVIG3YKA5Q6YCUP2RRNK7/action/replication_record"}},"created_at":"2026-05-18T01:58:54.843186+00:00","updated_at":"2026-05-18T01:58:54.843186+00:00"}