{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:C2M3UN655CSS5QWYEKOIWKHAPO","short_pith_number":"pith:C2M3UN65","schema_version":"1.0","canonical_sha256":"1699ba37dde8a52ec2d8229c8b28e07bb18eb32b7390742cc18f17bcc72eaebb","source":{"kind":"arxiv","id":"1504.05897","version":2},"attestation_state":"computed","paper":{"title":"High-J CO Versus Far-Infrared Relations in Normal and Starburst Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chentao Yang, Daizhong Liu, Emanuele Daddi, Kate Isaak, Nanyao Lu, Paul van der Werf, Yu Gao","submitted_at":"2015-04-22T17:40:37Z","abstract_excerpt":"We present correlations between 9 CO transition ($J=4-3$ to $12-11$) and beam-matched far-infrared (Far-IR) luminosities ($L_{\\mathrm{FIR},\\,b}$) among 167 local galaxies, using {\\it{Herschel}} Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (SPIRE; FTS) spectroscopic data and Photoconductor Array Camera and Spectrometer (PACS) photometry data. We adopt entire-galaxy FIR luminosities ($L_{\\mathrm{FIR},\\,e}$) from the {\\it{IRAS}} Revised Bright Galaxy Sample and correct to $L_{\\mathrm{FIR},\\,b}$ using PACS images to match the varying FTS beam sizes. All 9 correlations b"},"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":"1504.05897","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-04-22T17:40:37Z","cross_cats_sorted":[],"title_canon_sha256":"d387f78c2f0a8b07eccb09435cc55488936e12fa209b6a4133a252a1f178a02b","abstract_canon_sha256":"972871ee7d32c7d20626f4eb0849d202f458c38bc7f7b051d50837ab0af4ac83"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:30:08.005330Z","signature_b64":"C2a9vkKTFDeh/XqMulxCEEQ8inSYOfk+8aQNBstsoTSIcn2OuzQT6uKSSa05cT3bHaYqL0Qof9I5xmE+TZaxBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1699ba37dde8a52ec2d8229c8b28e07bb18eb32b7390742cc18f17bcc72eaebb","last_reissued_at":"2026-05-18T01:30:08.004879Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:30:08.004879Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-J CO Versus Far-Infrared Relations in Normal and Starburst Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chentao Yang, Daizhong Liu, Emanuele Daddi, Kate Isaak, Nanyao Lu, Paul van der Werf, Yu Gao","submitted_at":"2015-04-22T17:40:37Z","abstract_excerpt":"We present correlations between 9 CO transition ($J=4-3$ to $12-11$) and beam-matched far-infrared (Far-IR) luminosities ($L_{\\mathrm{FIR},\\,b}$) among 167 local galaxies, using {\\it{Herschel}} Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (SPIRE; FTS) spectroscopic data and Photoconductor Array Camera and Spectrometer (PACS) photometry data. We adopt entire-galaxy FIR luminosities ($L_{\\mathrm{FIR},\\,e}$) from the {\\it{IRAS}} Revised Bright Galaxy Sample and correct to $L_{\\mathrm{FIR},\\,b}$ using PACS images to match the varying FTS beam sizes. All 9 correlations b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.05897","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":"1504.05897","created_at":"2026-05-18T01:30:08.004944+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.05897v2","created_at":"2026-05-18T01:30:08.004944+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.05897","created_at":"2026-05-18T01:30:08.004944+00:00"},{"alias_kind":"pith_short_12","alias_value":"C2M3UN655CSS","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_16","alias_value":"C2M3UN655CSS5QWY","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_8","alias_value":"C2M3UN65","created_at":"2026-05-18T12:29:14.074870+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/C2M3UN655CSS5QWYEKOIWKHAPO","json":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO.json","graph_json":"https://pith.science/api/pith-number/C2M3UN655CSS5QWYEKOIWKHAPO/graph.json","events_json":"https://pith.science/api/pith-number/C2M3UN655CSS5QWYEKOIWKHAPO/events.json","paper":"https://pith.science/paper/C2M3UN65"},"agent_actions":{"view_html":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO","download_json":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO.json","view_paper":"https://pith.science/paper/C2M3UN65","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.05897&json=true","fetch_graph":"https://pith.science/api/pith-number/C2M3UN655CSS5QWYEKOIWKHAPO/graph.json","fetch_events":"https://pith.science/api/pith-number/C2M3UN655CSS5QWYEKOIWKHAPO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO/action/storage_attestation","attest_author":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO/action/author_attestation","sign_citation":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO/action/citation_signature","submit_replication":"https://pith.science/pith/C2M3UN655CSS5QWYEKOIWKHAPO/action/replication_record"}},"created_at":"2026-05-18T01:30:08.004944+00:00","updated_at":"2026-05-18T01:30:08.004944+00:00"}