{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:JLY26LK4GAWML7N2HKP7DE4J3N","short_pith_number":"pith:JLY26LK4","schema_version":"1.0","canonical_sha256":"4af1af2d5c302cc5fdba3a9ff19389db63c8a618b39e107e53da6b47c3ffd1fc","source":{"kind":"arxiv","id":"1306.1778","version":2},"attestation_state":"computed","paper":{"title":"Flux Calibration of Broadband Far Infrared and Submillimetre Photometric Instruments: Theory and Application to Herschel-SPIRE","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Amaral-Rogers, A. Conley, B. Schulz, B. Sibthorpe, B. Swinyard, C. D. Dowell, C. E. North, C. Pearson, G. Bendo, I. Valtchanov, J. Bock, J. Glenn, L. Conversi, L. Spencer, M. Ferlet, M. J. Griffin, M. Pohlen, T. Lim","submitted_at":"2013-06-07T17:05:36Z","abstract_excerpt":"Photometric instruments operating at far infrared to millimetre wavelengths often have broad spectral passbands (central wavelength/bandwidth ~ 3 or less), especially those operating in space. A broad passband can result in significant variation of the beam profile and aperture efficiency across the passband, effects which thus far have not generally been taken into account in the flux calibration of such instruments. With absolute calibration uncertainties associated with the brightness of primary calibration standards now in the region of 5% or less, variation of the beam properties across t"},"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":"1306.1778","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.IM","submitted_at":"2013-06-07T17:05:36Z","cross_cats_sorted":[],"title_canon_sha256":"c85d1f0f6764012d5276d440a7d7824aaf959f60b2154d06e4dc5dd9df262f5a","abstract_canon_sha256":"3d4fecda98e80bfca347d81ec6ec36c6af8531fd5468e4be7d4c210c621625fd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:45:23.382437Z","signature_b64":"A5/QQyZv12Ux4BU3FoSAHoAGg9sVTCt0e/YEBO3RB/RQ7ZS9W2yWTgmyO1fJGvYWItP+zp3Yo+01TmiM5AxTCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4af1af2d5c302cc5fdba3a9ff19389db63c8a618b39e107e53da6b47c3ffd1fc","last_reissued_at":"2026-05-18T02:45:23.381900Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:45:23.381900Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Flux Calibration of Broadband Far Infrared and Submillimetre Photometric Instruments: Theory and Application to Herschel-SPIRE","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Amaral-Rogers, A. Conley, B. Schulz, B. Sibthorpe, B. Swinyard, C. D. Dowell, C. E. North, C. Pearson, G. Bendo, I. Valtchanov, J. Bock, J. Glenn, L. Conversi, L. Spencer, M. Ferlet, M. J. Griffin, M. Pohlen, T. Lim","submitted_at":"2013-06-07T17:05:36Z","abstract_excerpt":"Photometric instruments operating at far infrared to millimetre wavelengths often have broad spectral passbands (central wavelength/bandwidth ~ 3 or less), especially those operating in space. A broad passband can result in significant variation of the beam profile and aperture efficiency across the passband, effects which thus far have not generally been taken into account in the flux calibration of such instruments. With absolute calibration uncertainties associated with the brightness of primary calibration standards now in the region of 5% or less, variation of the beam properties across t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.1778","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":"1306.1778","created_at":"2026-05-18T02:45:23.381975+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.1778v2","created_at":"2026-05-18T02:45:23.381975+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.1778","created_at":"2026-05-18T02:45:23.381975+00:00"},{"alias_kind":"pith_short_12","alias_value":"JLY26LK4GAWM","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"JLY26LK4GAWML7N2","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"JLY26LK4","created_at":"2026-05-18T12:27:49.015174+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/JLY26LK4GAWML7N2HKP7DE4J3N","json":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N.json","graph_json":"https://pith.science/api/pith-number/JLY26LK4GAWML7N2HKP7DE4J3N/graph.json","events_json":"https://pith.science/api/pith-number/JLY26LK4GAWML7N2HKP7DE4J3N/events.json","paper":"https://pith.science/paper/JLY26LK4"},"agent_actions":{"view_html":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N","download_json":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N.json","view_paper":"https://pith.science/paper/JLY26LK4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.1778&json=true","fetch_graph":"https://pith.science/api/pith-number/JLY26LK4GAWML7N2HKP7DE4J3N/graph.json","fetch_events":"https://pith.science/api/pith-number/JLY26LK4GAWML7N2HKP7DE4J3N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N/action/storage_attestation","attest_author":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N/action/author_attestation","sign_citation":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N/action/citation_signature","submit_replication":"https://pith.science/pith/JLY26LK4GAWML7N2HKP7DE4J3N/action/replication_record"}},"created_at":"2026-05-18T02:45:23.381975+00:00","updated_at":"2026-05-18T02:45:23.381975+00:00"}