{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:Z7QCEQBJNIXNUG3QSCJSQHWRLP","short_pith_number":"pith:Z7QCEQBJ","schema_version":"1.0","canonical_sha256":"cfe02240296a2eda1b709093281ed15beb1437035944fff88711aadd9c0ac225","source":{"kind":"arxiv","id":"1003.2174","version":1},"attestation_state":"computed","paper":{"title":"Detection of the 158 micron [CII] Transition at z=1.3: Evidence for a Galaxy-Wide Starburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"C. E. Tucker, D. J. Benford, G. J. Stacey, J. G. Staguhn, S. C. Parshley, S. Hailey-Dunsheath, T. E. Oberst, T. Nikola","submitted_at":"2010-03-10T18:57:54Z","abstract_excerpt":"We report the detection of 158 micron [CII] fine-structure line emission from MIPS J142824.0+352619, a hyperluminous (L_IR ~ 10^13 L_sun) starburst galaxy at z=1.3. The line is bright, and corresponds to a fraction L_[CII]/L_FIR = 2 x 10^-3 of the far-IR (FIR) continuum. The [CII], CO, and FIR continuum emission may be modeled as arising from photodissociation regions (PDRs) that have a characteristic gas density of n ~ 10^4.2 cm^-3, and that are illuminated by a far-UV radiation field ~10^3.2 times more intense than the local interstellar radiation field. The mass in these PDRs accounts for a"},"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":"1003.2174","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-10T18:57:54Z","cross_cats_sorted":[],"title_canon_sha256":"05f21bcabedbf8e0908bbd68c1e060caa71adf090ffb30eff54a17027a634dac","abstract_canon_sha256":"688d4c685a9dfc84bb7681d04464a31cc93ed6cfa4f5ca80312b89c7a2d06e04"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:35.368826Z","signature_b64":"33UJOJMF4WDRuOdD+O0HcS4l0MJopbBUm3+IKgtXLYSGKTkoI6l0GELo1qgxmi957oVr84DplgiwlSMdPvB+AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cfe02240296a2eda1b709093281ed15beb1437035944fff88711aadd9c0ac225","last_reissued_at":"2026-05-18T02:08:35.367883Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:35.367883Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of the 158 micron [CII] Transition at z=1.3: Evidence for a Galaxy-Wide Starburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"C. E. Tucker, D. J. Benford, G. J. Stacey, J. G. Staguhn, S. C. Parshley, S. Hailey-Dunsheath, T. E. Oberst, T. Nikola","submitted_at":"2010-03-10T18:57:54Z","abstract_excerpt":"We report the detection of 158 micron [CII] fine-structure line emission from MIPS J142824.0+352619, a hyperluminous (L_IR ~ 10^13 L_sun) starburst galaxy at z=1.3. The line is bright, and corresponds to a fraction L_[CII]/L_FIR = 2 x 10^-3 of the far-IR (FIR) continuum. The [CII], CO, and FIR continuum emission may be modeled as arising from photodissociation regions (PDRs) that have a characteristic gas density of n ~ 10^4.2 cm^-3, and that are illuminated by a far-UV radiation field ~10^3.2 times more intense than the local interstellar radiation field. The mass in these PDRs accounts for a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.2174","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":"1003.2174","created_at":"2026-05-18T02:08:35.368009+00:00"},{"alias_kind":"arxiv_version","alias_value":"1003.2174v1","created_at":"2026-05-18T02:08:35.368009+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.2174","created_at":"2026-05-18T02:08:35.368009+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z7QCEQBJNIXN","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z7QCEQBJNIXNUG3Q","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z7QCEQBJ","created_at":"2026-05-18T12:26:17.028572+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/Z7QCEQBJNIXNUG3QSCJSQHWRLP","json":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP.json","graph_json":"https://pith.science/api/pith-number/Z7QCEQBJNIXNUG3QSCJSQHWRLP/graph.json","events_json":"https://pith.science/api/pith-number/Z7QCEQBJNIXNUG3QSCJSQHWRLP/events.json","paper":"https://pith.science/paper/Z7QCEQBJ"},"agent_actions":{"view_html":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP","download_json":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP.json","view_paper":"https://pith.science/paper/Z7QCEQBJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1003.2174&json=true","fetch_graph":"https://pith.science/api/pith-number/Z7QCEQBJNIXNUG3QSCJSQHWRLP/graph.json","fetch_events":"https://pith.science/api/pith-number/Z7QCEQBJNIXNUG3QSCJSQHWRLP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP/action/storage_attestation","attest_author":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP/action/author_attestation","sign_citation":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP/action/citation_signature","submit_replication":"https://pith.science/pith/Z7QCEQBJNIXNUG3QSCJSQHWRLP/action/replication_record"}},"created_at":"2026-05-18T02:08:35.368009+00:00","updated_at":"2026-05-18T02:08:35.368009+00:00"}