{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:VT3DU6KOFGCFPM7LBDIO6JLPD4","short_pith_number":"pith:VT3DU6KO","schema_version":"1.0","canonical_sha256":"acf63a794e298457b3eb08d0ef256f1f3a835c78469fc62207f26668f5afb290","source":{"kind":"arxiv","id":"1005.5073","version":1},"attestation_state":"computed","paper":{"title":"In-flight calibration of the Herschel-SPIRE instrument","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Conley, A. Dowell, A. Glauser, A. J. Smith, A. Papageorgiou, A. Rykala, A. Schwartz, A. Woodcraft, B. M. Swinyard, B. Schulz, B. Sibthorpe, C. K. Xu, C. Pearson, D. Benielli, D. Brisbin, D. Dowell, D. Griffin, D. Naylor, D. Pouliquen, D. Rigopoulou, D. Shupe, E. Polehampton, G. J. Bendo, G. Makiwa, G. Savini, H. Aussel, H. Nguyen, H. Roussel, H. Triou, I. Valtchanov, J. Bock, J. Glenn, J-P. Baluteau, K. Isaak, K. King, L. Conversi, L. Levenson, L. Spencer, L. Zhang, M. Ferlet, M. Griffin, M. J. Barlow, M. Pohlen, M. Trichas, M. Zemcov, N. Lu, P. Ade, P. Imhof, P. Panuzzo, R. Wesson, S. Guest, S. Jones, S. Leeks, S. Oliver, S. Ronayette, S. Sidher, T. Fulton, T. L. Lim","submitted_at":"2010-05-27T13:51:11Z","abstract_excerpt":"SPIRE, the Spectral and Photometric Imaging Receiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. It contains a three-band imaging photometer operating at 250, 350 and 500 {\\mu}m, and an imaging Fourier transform spectrometer (FTS) covering 194-671 {\\mu}m (447-1550 GHz). In this paper we describe the initial approach taken to the absolute calibration of the SPIRE instrument using a combination of the emission from the Herschel telescope itself and the modelled continuum emission from solar system objects and other astronomical targets. We present the photometric,"},"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":"1005.5073","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2010-05-27T13:51:11Z","cross_cats_sorted":[],"title_canon_sha256":"5467c45be94444fe78b6c7d37da1e207cc64308a778f0e1616131417b95e13f1","abstract_canon_sha256":"30ad2e1b03b20acafe567a6275aba79000ff035ab52e92096e8472c1c91b5302"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:07.205656Z","signature_b64":"fGKN5EZAXvqSZ9sEhWbC8oOtFnErYhnLlBQlcZdd+AILuGajS54A9aq3fW/P3eWiXXRA/T1AFv+O/odvFckLBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"acf63a794e298457b3eb08d0ef256f1f3a835c78469fc62207f26668f5afb290","last_reissued_at":"2026-05-18T02:07:07.205023Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:07.205023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"In-flight calibration of the Herschel-SPIRE instrument","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Conley, A. Dowell, A. Glauser, A. J. Smith, A. Papageorgiou, A. Rykala, A. Schwartz, A. Woodcraft, B. M. Swinyard, B. Schulz, B. Sibthorpe, C. K. Xu, C. Pearson, D. Benielli, D. Brisbin, D. Dowell, D. Griffin, D. Naylor, D. Pouliquen, D. Rigopoulou, D. Shupe, E. Polehampton, G. J. Bendo, G. Makiwa, G. Savini, H. Aussel, H. Nguyen, H. Roussel, H. Triou, I. Valtchanov, J. Bock, J. Glenn, J-P. Baluteau, K. Isaak, K. King, L. Conversi, L. Levenson, L. Spencer, L. Zhang, M. Ferlet, M. Griffin, M. J. Barlow, M. Pohlen, M. Trichas, M. Zemcov, N. Lu, P. Ade, P. Imhof, P. Panuzzo, R. Wesson, S. Guest, S. Jones, S. Leeks, S. Oliver, S. Ronayette, S. Sidher, T. Fulton, T. L. Lim","submitted_at":"2010-05-27T13:51:11Z","abstract_excerpt":"SPIRE, the Spectral and Photometric Imaging Receiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. It contains a three-band imaging photometer operating at 250, 350 and 500 {\\mu}m, and an imaging Fourier transform spectrometer (FTS) covering 194-671 {\\mu}m (447-1550 GHz). In this paper we describe the initial approach taken to the absolute calibration of the SPIRE instrument using a combination of the emission from the Herschel telescope itself and the modelled continuum emission from solar system objects and other astronomical targets. We present the photometric,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.5073","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":"1005.5073","created_at":"2026-05-18T02:07:07.205120+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.5073v1","created_at":"2026-05-18T02:07:07.205120+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.5073","created_at":"2026-05-18T02:07:07.205120+00:00"},{"alias_kind":"pith_short_12","alias_value":"VT3DU6KOFGCF","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_16","alias_value":"VT3DU6KOFGCFPM7L","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_8","alias_value":"VT3DU6KO","created_at":"2026-05-18T12:26:15.391820+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/VT3DU6KOFGCFPM7LBDIO6JLPD4","json":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4.json","graph_json":"https://pith.science/api/pith-number/VT3DU6KOFGCFPM7LBDIO6JLPD4/graph.json","events_json":"https://pith.science/api/pith-number/VT3DU6KOFGCFPM7LBDIO6JLPD4/events.json","paper":"https://pith.science/paper/VT3DU6KO"},"agent_actions":{"view_html":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4","download_json":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4.json","view_paper":"https://pith.science/paper/VT3DU6KO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.5073&json=true","fetch_graph":"https://pith.science/api/pith-number/VT3DU6KOFGCFPM7LBDIO6JLPD4/graph.json","fetch_events":"https://pith.science/api/pith-number/VT3DU6KOFGCFPM7LBDIO6JLPD4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4/action/storage_attestation","attest_author":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4/action/author_attestation","sign_citation":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4/action/citation_signature","submit_replication":"https://pith.science/pith/VT3DU6KOFGCFPM7LBDIO6JLPD4/action/replication_record"}},"created_at":"2026-05-18T02:07:07.205120+00:00","updated_at":"2026-05-18T02:07:07.205120+00:00"}