{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:OGIFX34FDVI3N35G6JUT2HI2BB","short_pith_number":"pith:OGIFX34F","schema_version":"1.0","canonical_sha256":"71905bef851d51b6efa6f2693d1d1a086c445429d1cf86655de2b6636452e7f0","source":{"kind":"arxiv","id":"0907.2290","version":2},"attestation_state":"computed","paper":{"title":"GRB afterglow plateaus and Gravitational Waves: multi-messenger signature of a millisecond magnetar?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Alessandra Corsi, Peter Meszaros","submitted_at":"2009-07-14T05:38:06Z","abstract_excerpt":"The existence of a shallow decay phase in the early X-ray afterglows of gamma-ray bursts is a common feature. Here we investigate the possibility that this is connected to the formation of a highly magnetized millisecond pulsar, pumping energy into the fireball on timescales longer than the prompt emission. In this scenario the nascent neutron star could undergo a secular bar-mode instability, leading to gravitational wave losses which would affect the neutron star spin-down. In this case, nearby gamma-ray bursts with isotropic energies of the order of 1e50 ergs would produce a detectable grav"},"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":"0907.2290","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-07-14T05:38:06Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"259d055335bcc58c97220adfdfffb7ff444becef4ccb5cf31bd95e829834fc76","abstract_canon_sha256":"d90a4200bfe760ad302412399e6412cde263becb7131795542a7caa56d33654f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:51:54.739962Z","signature_b64":"dfklKO+U+im3sytxNgZKBy0jVodIo9ReXtm0r+yhhUyQUQTUvAFNbcWu06pNmr5oKr+be/6OuSOxMwL6t/ifCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"71905bef851d51b6efa6f2693d1d1a086c445429d1cf86655de2b6636452e7f0","last_reissued_at":"2026-07-04T15:51:54.739610Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:51:54.739610Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GRB afterglow plateaus and Gravitational Waves: multi-messenger signature of a millisecond magnetar?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Alessandra Corsi, Peter Meszaros","submitted_at":"2009-07-14T05:38:06Z","abstract_excerpt":"The existence of a shallow decay phase in the early X-ray afterglows of gamma-ray bursts is a common feature. Here we investigate the possibility that this is connected to the formation of a highly magnetized millisecond pulsar, pumping energy into the fireball on timescales longer than the prompt emission. In this scenario the nascent neutron star could undergo a secular bar-mode instability, leading to gravitational wave losses which would affect the neutron star spin-down. In this case, nearby gamma-ray bursts with isotropic energies of the order of 1e50 ergs would produce a detectable grav"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0907.2290","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/0907.2290/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":"0907.2290","created_at":"2026-07-04T15:51:54.739670+00:00"},{"alias_kind":"arxiv_version","alias_value":"0907.2290v2","created_at":"2026-07-04T15:51:54.739670+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0907.2290","created_at":"2026-07-04T15:51:54.739670+00:00"},{"alias_kind":"pith_short_12","alias_value":"OGIFX34FDVI3","created_at":"2026-07-04T15:51:54.739670+00:00"},{"alias_kind":"pith_short_16","alias_value":"OGIFX34FDVI3N35G","created_at":"2026-07-04T15:51:54.739670+00:00"},{"alias_kind":"pith_short_8","alias_value":"OGIFX34F","created_at":"2026-07-04T15:51:54.739670+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.09878","citing_title":"GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB","json":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB.json","graph_json":"https://pith.science/api/pith-number/OGIFX34FDVI3N35G6JUT2HI2BB/graph.json","events_json":"https://pith.science/api/pith-number/OGIFX34FDVI3N35G6JUT2HI2BB/events.json","paper":"https://pith.science/paper/OGIFX34F"},"agent_actions":{"view_html":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB","download_json":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB.json","view_paper":"https://pith.science/paper/OGIFX34F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0907.2290&json=true","fetch_graph":"https://pith.science/api/pith-number/OGIFX34FDVI3N35G6JUT2HI2BB/graph.json","fetch_events":"https://pith.science/api/pith-number/OGIFX34FDVI3N35G6JUT2HI2BB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB/action/storage_attestation","attest_author":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB/action/author_attestation","sign_citation":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB/action/citation_signature","submit_replication":"https://pith.science/pith/OGIFX34FDVI3N35G6JUT2HI2BB/action/replication_record"}},"created_at":"2026-07-04T15:51:54.739670+00:00","updated_at":"2026-07-04T15:51:54.739670+00:00"}