{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:C4OZH4QN7KB43EC3SJXAHXZYST","short_pith_number":"pith:C4OZH4QN","schema_version":"1.0","canonical_sha256":"171d93f20dfa83cd905b926e03df3894fa021f44e6d93fa728f715bf0546c6df","source":{"kind":"arxiv","id":"1405.5759","version":2},"attestation_state":"computed","paper":{"title":"Star Formation Rates from [CII] 158 um and Mid Infrared Emission Lines for Starbursts and AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anahit Samsonyan, Daniel Weedman, Donald Barry, Henrik Spoon, James Houck, Jeronimo Bernard-Salas, Lusine Sargsyan, Vianney Lebouteiller","submitted_at":"2014-05-22T14:04:07Z","abstract_excerpt":"A summary is presented for 130 galaxies observed with the Herschel PACS instrument to measure fluxes for the [CII] 158 um emission line. Sources cover a wide range of active galactic nucleus to starburst classifications, as derived from polycyclic aromatic hydrocarbon (PAH) strength measured with the Spitzer Infrared Spectrograph. Redshifts from [CII] and line to continuum strengths (equivalent width of [CII]) are given for the full sample, which includes 18 new [CII] flux measures. Calibration of L([CII)]) as a star formation rate (SFR) indicator is determined by comparing [CII] luminosities "},"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":"1405.5759","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-05-22T14:04:07Z","cross_cats_sorted":[],"title_canon_sha256":"c074b512f6d610767cf221814ad733d26e3683d400f7c37224288b50498ab38b","abstract_canon_sha256":"9dcbed508d7adb0c55d27d5c45566cd79d56b4ef7a6eab3cd6406ab1a6fb5f88"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:09.241887Z","signature_b64":"oHGLbzHPlXs39nrlU+MeSBqv3vuShKCnLNmzHeOzPOZ4Cd01zeLzwL33+0Rc1pdGqmdibe+e1zHoZL8A51QRCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"171d93f20dfa83cd905b926e03df3894fa021f44e6d93fa728f715bf0546c6df","last_reissued_at":"2026-05-18T01:43:09.241156Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:09.241156Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star Formation Rates from [CII] 158 um and Mid Infrared Emission Lines for Starbursts and AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anahit Samsonyan, Daniel Weedman, Donald Barry, Henrik Spoon, James Houck, Jeronimo Bernard-Salas, Lusine Sargsyan, Vianney Lebouteiller","submitted_at":"2014-05-22T14:04:07Z","abstract_excerpt":"A summary is presented for 130 galaxies observed with the Herschel PACS instrument to measure fluxes for the [CII] 158 um emission line. Sources cover a wide range of active galactic nucleus to starburst classifications, as derived from polycyclic aromatic hydrocarbon (PAH) strength measured with the Spitzer Infrared Spectrograph. Redshifts from [CII] and line to continuum strengths (equivalent width of [CII]) are given for the full sample, which includes 18 new [CII] flux measures. Calibration of L([CII)]) as a star formation rate (SFR) indicator is determined by comparing [CII] luminosities "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.5759","kind":"arxiv","version":2},"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":"1405.5759","created_at":"2026-05-18T01:43:09.241256+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.5759v2","created_at":"2026-05-18T01:43:09.241256+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.5759","created_at":"2026-05-18T01:43:09.241256+00:00"},{"alias_kind":"pith_short_12","alias_value":"C4OZH4QN7KB4","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"C4OZH4QN7KB43EC3","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"C4OZH4QN","created_at":"2026-05-18T12:28:22.404517+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/C4OZH4QN7KB43EC3SJXAHXZYST","json":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST.json","graph_json":"https://pith.science/api/pith-number/C4OZH4QN7KB43EC3SJXAHXZYST/graph.json","events_json":"https://pith.science/api/pith-number/C4OZH4QN7KB43EC3SJXAHXZYST/events.json","paper":"https://pith.science/paper/C4OZH4QN"},"agent_actions":{"view_html":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST","download_json":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST.json","view_paper":"https://pith.science/paper/C4OZH4QN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.5759&json=true","fetch_graph":"https://pith.science/api/pith-number/C4OZH4QN7KB43EC3SJXAHXZYST/graph.json","fetch_events":"https://pith.science/api/pith-number/C4OZH4QN7KB43EC3SJXAHXZYST/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST/action/storage_attestation","attest_author":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST/action/author_attestation","sign_citation":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST/action/citation_signature","submit_replication":"https://pith.science/pith/C4OZH4QN7KB43EC3SJXAHXZYST/action/replication_record"}},"created_at":"2026-05-18T01:43:09.241256+00:00","updated_at":"2026-05-18T01:43:09.241256+00:00"}