{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:Z4IIOXZL6YCFQZD6BLTNN63L6P","short_pith_number":"pith:Z4IIOXZL","schema_version":"1.0","canonical_sha256":"cf10875f2bf60458647e0ae6d6fb6bf3ef19eab3445831d0e48a318c598bfdbe","source":{"kind":"arxiv","id":"1201.2230","version":3},"attestation_state":"computed","paper":{"title":"Far-infrared line and dust emission from H II regions and photodissociation regions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jiali. Zhu, M. Huang","submitted_at":"2012-01-11T03:16:03Z","abstract_excerpt":"We explore the effect of varying the spectral energy distribution of the incident continuum, by simultaneously and self-consistently computing the structure of an H II region and a photodissociation region that are in pressure equilibrium. The results of the calculations are applied to extragalactic observations. The intensity ratio diagrams of far-infrared (FIR) emission for Herschel bands (70, 110, 160, 250, 350, and 500 {\\mu}m) and the contribution from H II regions for these specific FIR emissions are presented for the first time. With these diagrams, we compare the predicted FIR continuum"},"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":"1201.2230","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-01-11T03:16:03Z","cross_cats_sorted":[],"title_canon_sha256":"a837a3a0b50466fbf7b97e7fe482966ccc2b610563615535917ff438a9dcf03a","abstract_canon_sha256":"44135756d26061610b9cab0836366ede6a9f7b762c499c506936fbc5a382a647"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:03:57.067515Z","signature_b64":"0HWLUL55QWEvKW5VnR+RVkQPU5cdlPl1ww+ALXBHviMt3mU9X76RFafiTsVPmAMCAnOPELr7KMj7+/vwo8yfCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf10875f2bf60458647e0ae6d6fb6bf3ef19eab3445831d0e48a318c598bfdbe","last_reissued_at":"2026-05-18T03:03:57.066813Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:03:57.066813Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Far-infrared line and dust emission from H II regions and photodissociation regions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jiali. Zhu, M. Huang","submitted_at":"2012-01-11T03:16:03Z","abstract_excerpt":"We explore the effect of varying the spectral energy distribution of the incident continuum, by simultaneously and self-consistently computing the structure of an H II region and a photodissociation region that are in pressure equilibrium. The results of the calculations are applied to extragalactic observations. The intensity ratio diagrams of far-infrared (FIR) emission for Herschel bands (70, 110, 160, 250, 350, and 500 {\\mu}m) and the contribution from H II regions for these specific FIR emissions are presented for the first time. With these diagrams, we compare the predicted FIR continuum"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.2230","kind":"arxiv","version":3},"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":"1201.2230","created_at":"2026-05-18T03:03:57.066922+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.2230v3","created_at":"2026-05-18T03:03:57.066922+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.2230","created_at":"2026-05-18T03:03:57.066922+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z4IIOXZL6YCF","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z4IIOXZL6YCFQZD6","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z4IIOXZL","created_at":"2026-05-18T12:27:30.460161+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/Z4IIOXZL6YCFQZD6BLTNN63L6P","json":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P.json","graph_json":"https://pith.science/api/pith-number/Z4IIOXZL6YCFQZD6BLTNN63L6P/graph.json","events_json":"https://pith.science/api/pith-number/Z4IIOXZL6YCFQZD6BLTNN63L6P/events.json","paper":"https://pith.science/paper/Z4IIOXZL"},"agent_actions":{"view_html":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P","download_json":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P.json","view_paper":"https://pith.science/paper/Z4IIOXZL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.2230&json=true","fetch_graph":"https://pith.science/api/pith-number/Z4IIOXZL6YCFQZD6BLTNN63L6P/graph.json","fetch_events":"https://pith.science/api/pith-number/Z4IIOXZL6YCFQZD6BLTNN63L6P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P/action/storage_attestation","attest_author":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P/action/author_attestation","sign_citation":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P/action/citation_signature","submit_replication":"https://pith.science/pith/Z4IIOXZL6YCFQZD6BLTNN63L6P/action/replication_record"}},"created_at":"2026-05-18T03:03:57.066922+00:00","updated_at":"2026-05-18T03:03:57.066922+00:00"}