{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SEOP7WXFFDPZ43HTUVFRBJZ6KX","short_pith_number":"pith:SEOP7WXF","schema_version":"1.0","canonical_sha256":"911cffdae528df9e6cf3a54b10a73e55de8d8061fba72776a6e3767f18276103","source":{"kind":"arxiv","id":"1310.5349","version":1},"attestation_state":"computed","paper":{"title":"First results with the boloSource() algorithm: Photometry of faint standard stars observed by Herschel/PACS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Csaba Kiss, G\\'abor Marton, Roland Vavrek, Thomas G. M\\\"uller","submitted_at":"2013-10-20T17:01:08Z","abstract_excerpt":"The boloSource() algorithm is a tool to separate the signal of compact sources from that of the diffuse background in the timeline of far-infrared measurements performed by the PACS camera of the Herschel Space Observatory. An important characteristic and quality indicator of this method is that how well it can reproduce the flux of faint standard stars which have reliable flux estimates. For this propose we selected a few calibrator targets and constructed light curves by extracting point source flux for each repetition of the measurements independently using standard aperture photometry meth"},"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":"1310.5349","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2013-10-20T17:01:08Z","cross_cats_sorted":[],"title_canon_sha256":"42c74c0d7d3d90fb2f0a0fbf87b63f052bc40b1b9509aa6ffbe4b44c9213d144","abstract_canon_sha256":"acd3779b7e2e4dd6cf409e139117bbfe3670fd324b712f8727682962460f1c1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:57.338431Z","signature_b64":"o2kSRfyzf3xuPsTaWYUwTJnJLn4kf5cVwwA+ddJYedHl8CZbZcs69vvVCgiVbn0HaVWxJnMmoYPHrkzUVPCzDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"911cffdae528df9e6cf3a54b10a73e55de8d8061fba72776a6e3767f18276103","last_reissued_at":"2026-05-18T01:46:57.337410Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:57.337410Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"First results with the boloSource() algorithm: Photometry of faint standard stars observed by Herschel/PACS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Csaba Kiss, G\\'abor Marton, Roland Vavrek, Thomas G. M\\\"uller","submitted_at":"2013-10-20T17:01:08Z","abstract_excerpt":"The boloSource() algorithm is a tool to separate the signal of compact sources from that of the diffuse background in the timeline of far-infrared measurements performed by the PACS camera of the Herschel Space Observatory. An important characteristic and quality indicator of this method is that how well it can reproduce the flux of faint standard stars which have reliable flux estimates. For this propose we selected a few calibrator targets and constructed light curves by extracting point source flux for each repetition of the measurements independently using standard aperture photometry meth"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.5349","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":"1310.5349","created_at":"2026-05-18T01:46:57.337529+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.5349v1","created_at":"2026-05-18T01:46:57.337529+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.5349","created_at":"2026-05-18T01:46:57.337529+00:00"},{"alias_kind":"pith_short_12","alias_value":"SEOP7WXFFDPZ","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SEOP7WXFFDPZ43HT","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SEOP7WXF","created_at":"2026-05-18T12:27:59.945178+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/SEOP7WXFFDPZ43HTUVFRBJZ6KX","json":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX.json","graph_json":"https://pith.science/api/pith-number/SEOP7WXFFDPZ43HTUVFRBJZ6KX/graph.json","events_json":"https://pith.science/api/pith-number/SEOP7WXFFDPZ43HTUVFRBJZ6KX/events.json","paper":"https://pith.science/paper/SEOP7WXF"},"agent_actions":{"view_html":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX","download_json":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX.json","view_paper":"https://pith.science/paper/SEOP7WXF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.5349&json=true","fetch_graph":"https://pith.science/api/pith-number/SEOP7WXFFDPZ43HTUVFRBJZ6KX/graph.json","fetch_events":"https://pith.science/api/pith-number/SEOP7WXFFDPZ43HTUVFRBJZ6KX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX/action/storage_attestation","attest_author":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX/action/author_attestation","sign_citation":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX/action/citation_signature","submit_replication":"https://pith.science/pith/SEOP7WXFFDPZ43HTUVFRBJZ6KX/action/replication_record"}},"created_at":"2026-05-18T01:46:57.337529+00:00","updated_at":"2026-05-18T01:46:57.337529+00:00"}