{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:4DEV3I5BYC7D63JUMNZ7MBMAGR","short_pith_number":"pith:4DEV3I5B","schema_version":"1.0","canonical_sha256":"e0c95da3a1c0be3f6d346373f605803444265809a94ca1b2467b19e24e2b7d3a","source":{"kind":"arxiv","id":"1707.07281","version":1},"attestation_state":"computed","paper":{"title":"Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Christian Rab, Francois Menard, Inga Kamp, Peter Woitke, Sietske Bouma, Wing-Fai Thi","submitted_at":"2017-07-23T10:54:56Z","abstract_excerpt":"Aims. We define a small and large chemical network which can be used for the quantitative simultaneous analysis of molecular emission from the near-IR to the submm. We revise reactions of excited molecular hydrogen, which are not included in UMIST, to provide a homogeneous database for future applications. Methods. We use the thermo-chemical disk modeling code ProDiMo and a standard T Tauri disk model to evaluate the impact of various chemical networks, reaction rate databases and sets of adsorption energies on a large sample of chemical species and emerging line fluxes from the near-IR to the"},"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":"1707.07281","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-07-23T10:54:56Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"14f9bb2b9c4b8aa6aaee9016366b1489953903e9b5029fd8a6a78582eb8f2dc4","abstract_canon_sha256":"f1c84191e9d6847e59b36a8e5778ba491eff0addd6dfd726964d3639f4e3d554"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:30:43.772989Z","signature_b64":"cTSrHKgRXEzTjTbQF579pCyyudLXv/hsIlYhMbzfjwAoVlZPzqGX/p8YgLqJqt/yI+zG55MS9HBE9kEUP16TDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e0c95da3a1c0be3f6d346373f605803444265809a94ca1b2467b19e24e2b7d3a","last_reissued_at":"2026-05-18T00:30:43.772486Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:30:43.772486Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Christian Rab, Francois Menard, Inga Kamp, Peter Woitke, Sietske Bouma, Wing-Fai Thi","submitted_at":"2017-07-23T10:54:56Z","abstract_excerpt":"Aims. We define a small and large chemical network which can be used for the quantitative simultaneous analysis of molecular emission from the near-IR to the submm. We revise reactions of excited molecular hydrogen, which are not included in UMIST, to provide a homogeneous database for future applications. Methods. We use the thermo-chemical disk modeling code ProDiMo and a standard T Tauri disk model to evaluate the impact of various chemical networks, reaction rate databases and sets of adsorption energies on a large sample of chemical species and emerging line fluxes from the near-IR to the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.07281","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":"1707.07281","created_at":"2026-05-18T00:30:43.772570+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.07281v1","created_at":"2026-05-18T00:30:43.772570+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.07281","created_at":"2026-05-18T00:30:43.772570+00:00"},{"alias_kind":"pith_short_12","alias_value":"4DEV3I5BYC7D","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"4DEV3I5BYC7D63JU","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"4DEV3I5B","created_at":"2026-05-18T12:30:58.224056+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/4DEV3I5BYC7D63JUMNZ7MBMAGR","json":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR.json","graph_json":"https://pith.science/api/pith-number/4DEV3I5BYC7D63JUMNZ7MBMAGR/graph.json","events_json":"https://pith.science/api/pith-number/4DEV3I5BYC7D63JUMNZ7MBMAGR/events.json","paper":"https://pith.science/paper/4DEV3I5B"},"agent_actions":{"view_html":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR","download_json":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR.json","view_paper":"https://pith.science/paper/4DEV3I5B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.07281&json=true","fetch_graph":"https://pith.science/api/pith-number/4DEV3I5BYC7D63JUMNZ7MBMAGR/graph.json","fetch_events":"https://pith.science/api/pith-number/4DEV3I5BYC7D63JUMNZ7MBMAGR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR/action/storage_attestation","attest_author":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR/action/author_attestation","sign_citation":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR/action/citation_signature","submit_replication":"https://pith.science/pith/4DEV3I5BYC7D63JUMNZ7MBMAGR/action/replication_record"}},"created_at":"2026-05-18T00:30:43.772570+00:00","updated_at":"2026-05-18T00:30:43.772570+00:00"}