{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:E6SUUOIBYHJM5DSMJGUOTXMV6L","short_pith_number":"pith:E6SUUOIB","schema_version":"1.0","canonical_sha256":"27a54a3901c1d2ce8e4c49a8e9dd95f2c09554aefdc71719d43ed0ccf5063ff0","source":{"kind":"arxiv","id":"1711.07210","version":1},"attestation_state":"computed","paper":{"title":"Central Compact Objects in Supernova Remnants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea De Luca (INAF/IASF Milano)","submitted_at":"2017-11-20T09:05:13Z","abstract_excerpt":"Central Compact Objects (CCOs) are a handful of sources located close to the geometrical center of young supernova remnants. They only show thermal-like, soft X-ray emission and have no counterparts at any other wavelength. While the first observed CCO turned out to be a very peculiar magnetar, discovery that three members of the family are weakly magnetised Isolated Neutron Stars (INSs) set the basis for an interpretation of the class. However, the phenomeology of CCOs and their relationship with other classes of INSs, possibly ruled by supernova fall-back accretion, are still far from being "},"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":"1711.07210","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-20T09:05:13Z","cross_cats_sorted":[],"title_canon_sha256":"6141c1e75859cdd0f32393c1a1851f8f328d90a39dfcef2ccf2d5a85b8c463dc","abstract_canon_sha256":"efc41346289b483e2aaae2a3d87730056de6c65bd6f2e8e28ef5a45549b90cb7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:25:51.430357Z","signature_b64":"ko2sZtvqn0O+tPc0r5hwqC8qE1WHG4scWALbVIa++TkGwPFLY5IfxKdaDBYCU7HSCQeu6WoCqLxcPZzalCrAAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"27a54a3901c1d2ce8e4c49a8e9dd95f2c09554aefdc71719d43ed0ccf5063ff0","last_reissued_at":"2026-05-18T00:25:51.429742Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:25:51.429742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Central Compact Objects in Supernova Remnants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea De Luca (INAF/IASF Milano)","submitted_at":"2017-11-20T09:05:13Z","abstract_excerpt":"Central Compact Objects (CCOs) are a handful of sources located close to the geometrical center of young supernova remnants. They only show thermal-like, soft X-ray emission and have no counterparts at any other wavelength. While the first observed CCO turned out to be a very peculiar magnetar, discovery that three members of the family are weakly magnetised Isolated Neutron Stars (INSs) set the basis for an interpretation of the class. However, the phenomeology of CCOs and their relationship with other classes of INSs, possibly ruled by supernova fall-back accretion, are still far from being "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.07210","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":"1711.07210","created_at":"2026-05-18T00:25:51.429829+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.07210v1","created_at":"2026-05-18T00:25:51.429829+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.07210","created_at":"2026-05-18T00:25:51.429829+00:00"},{"alias_kind":"pith_short_12","alias_value":"E6SUUOIBYHJM","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"E6SUUOIBYHJM5DSM","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"E6SUUOIB","created_at":"2026-05-18T12:31:12.930513+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2311.10903","citing_title":"Probing Low-Luminosity Gamma-Ray Emission from SNR G296.5+10.0 and CCO 1E 1207.4-5209 with CTAO","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2512.17214","citing_title":"Pulsed radio emission from a Central Compact Object","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L","json":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L.json","graph_json":"https://pith.science/api/pith-number/E6SUUOIBYHJM5DSMJGUOTXMV6L/graph.json","events_json":"https://pith.science/api/pith-number/E6SUUOIBYHJM5DSMJGUOTXMV6L/events.json","paper":"https://pith.science/paper/E6SUUOIB"},"agent_actions":{"view_html":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L","download_json":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L.json","view_paper":"https://pith.science/paper/E6SUUOIB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.07210&json=true","fetch_graph":"https://pith.science/api/pith-number/E6SUUOIBYHJM5DSMJGUOTXMV6L/graph.json","fetch_events":"https://pith.science/api/pith-number/E6SUUOIBYHJM5DSMJGUOTXMV6L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L/action/storage_attestation","attest_author":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L/action/author_attestation","sign_citation":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L/action/citation_signature","submit_replication":"https://pith.science/pith/E6SUUOIBYHJM5DSMJGUOTXMV6L/action/replication_record"}},"created_at":"2026-05-18T00:25:51.429829+00:00","updated_at":"2026-05-18T00:25:51.429829+00:00"}