{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:IKBJRPX2H35KYZXT33QEARINM7","short_pith_number":"pith:IKBJRPX2","schema_version":"1.0","canonical_sha256":"428298befa3efaac66f3dee040450d67dc3f955a08efc0d89e152ed9353b94b9","source":{"kind":"arxiv","id":"astro-ph/0206132","version":2},"attestation_state":"computed","paper":{"title":"Molecular Beam Dumps as Tracers of Hadronic Cosmic Ray Sources: the Case of SNR IC443","license":"","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph","authors_text":"Diego F. Torres, Gustavo E. Romero, Jorge A. Combi, Thomas M. Dame, Yousaf M. Butt","submitted_at":"2002-06-09T18:18:16Z","abstract_excerpt":"The gamma-ray & neutrino visibility of cosmic ray (CR) accelerators will be dramatically increased by the presence of molecular material abutting such sites due to the increased probability of pion production -- and, in the case of neutral pions, subsequent gamma-decay. This was recognized by Pinkau, Montmerle, and Black & Fazio, and others in the 1970's. In an effort to examine the long-standing -- but unproven -- conjecture that galactic supernova remnants (SNRs) are indeed the sites of nucleonic CR acceleration to <~300TeV/n we have carried out a 3-way coincidence search between the SNRs in"},"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":"astro-ph/0206132","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-06-09T18:18:16Z","cross_cats_sorted":["hep-ex","hep-ph"],"title_canon_sha256":"99b84c72f11fdc47a1264d9275d4aa0d2f91816fe75d308192526561f60d0085","abstract_canon_sha256":"eac8bac59625dbc8ebfbf823f784318c0af460e83093d7bd077f0325a7ee750e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:12:03.022469Z","signature_b64":"6wjJz+B4wsObLieiZZukBYu4l5da8YsSOx2eXspFvcNbLErLUsFWAF8k2igfEg/jVh0FrJirJDb58PRBlmCXAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"428298befa3efaac66f3dee040450d67dc3f955a08efc0d89e152ed9353b94b9","last_reissued_at":"2026-07-04T14:12:03.022034Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:12:03.022034Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular Beam Dumps as Tracers of Hadronic Cosmic Ray Sources: the Case of SNR IC443","license":"","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph","authors_text":"Diego F. Torres, Gustavo E. Romero, Jorge A. Combi, Thomas M. Dame, Yousaf M. Butt","submitted_at":"2002-06-09T18:18:16Z","abstract_excerpt":"The gamma-ray & neutrino visibility of cosmic ray (CR) accelerators will be dramatically increased by the presence of molecular material abutting such sites due to the increased probability of pion production -- and, in the case of neutral pions, subsequent gamma-decay. This was recognized by Pinkau, Montmerle, and Black & Fazio, and others in the 1970's. In an effort to examine the long-standing -- but unproven -- conjecture that galactic supernova remnants (SNRs) are indeed the sites of nucleonic CR acceleration to <~300TeV/n we have carried out a 3-way coincidence search between the SNRs in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0206132","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0206132/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0206132","created_at":"2026-07-04T14:12:03.022098+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0206132v2","created_at":"2026-07-04T14:12:03.022098+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0206132","created_at":"2026-07-04T14:12:03.022098+00:00"},{"alias_kind":"pith_short_12","alias_value":"IKBJRPX2H35K","created_at":"2026-07-04T14:12:03.022098+00:00"},{"alias_kind":"pith_short_16","alias_value":"IKBJRPX2H35KYZXT","created_at":"2026-07-04T14:12:03.022098+00:00"},{"alias_kind":"pith_short_8","alias_value":"IKBJRPX2","created_at":"2026-07-04T14:12:03.022098+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/IKBJRPX2H35KYZXT33QEARINM7","json":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7.json","graph_json":"https://pith.science/api/pith-number/IKBJRPX2H35KYZXT33QEARINM7/graph.json","events_json":"https://pith.science/api/pith-number/IKBJRPX2H35KYZXT33QEARINM7/events.json","paper":"https://pith.science/paper/IKBJRPX2"},"agent_actions":{"view_html":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7","download_json":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7.json","view_paper":"https://pith.science/paper/IKBJRPX2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0206132&json=true","fetch_graph":"https://pith.science/api/pith-number/IKBJRPX2H35KYZXT33QEARINM7/graph.json","fetch_events":"https://pith.science/api/pith-number/IKBJRPX2H35KYZXT33QEARINM7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7/action/storage_attestation","attest_author":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7/action/author_attestation","sign_citation":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7/action/citation_signature","submit_replication":"https://pith.science/pith/IKBJRPX2H35KYZXT33QEARINM7/action/replication_record"}},"created_at":"2026-07-04T14:12:03.022098+00:00","updated_at":"2026-07-04T14:12:03.022098+00:00"}