{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:LPRZOMELLQCVE2PSTPHGLIMB77","short_pith_number":"pith:LPRZOMEL","schema_version":"1.0","canonical_sha256":"5be397308b5c055269f29bce65a181ffebf32cd12bfc9533b5bc61f6a1afb3f7","source":{"kind":"arxiv","id":"1101.2835","version":2},"attestation_state":"computed","paper":{"title":"Review on latest progress on Supergiant Fast X-ray Transients and future direction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Italy), Lara Sidoli (INAF-IASF Milano","submitted_at":"2011-01-14T15:19:44Z","abstract_excerpt":"In the recent years, the discovery of a new class of Galactic transients with fast and bright flaring X-ray activity, the Supergiant Fast X-ray Transients, has completely changed our view and comprehension of massive X-ray binaries. These objects display X-ray outbursts which are difficult to be explained in the framework of standard theories for the accretion of matter onto compact objects, and could represent a dominant population of X-ray binaries. I will review their main observational properties (neutron star magnetic field, orbital and spin period, long term behavior, duty cycle, quiesce"},"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":"1101.2835","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-14T15:19:44Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"f0ee5b019ec25e791588d3c46ae3fc59d364f3fd9afc8e50f67857b4e990f7c2","abstract_canon_sha256":"75b7af1b186c72cc1d532e16ad613d0f7d770d2287be6c6ab836b413f9db1429"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:39.967674Z","signature_b64":"lJcApLXk6apSAkbE8O5u/AiE5KtjUI0ZMoFrN0fH0fXspLCqb4rYM1zKnlWnNavjg6ozwLNiFjsoRy0J9nzODA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5be397308b5c055269f29bce65a181ffebf32cd12bfc9533b5bc61f6a1afb3f7","last_reissued_at":"2026-05-18T02:03:39.967171Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:39.967171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Review on latest progress on Supergiant Fast X-ray Transients and future direction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Italy), Lara Sidoli (INAF-IASF Milano","submitted_at":"2011-01-14T15:19:44Z","abstract_excerpt":"In the recent years, the discovery of a new class of Galactic transients with fast and bright flaring X-ray activity, the Supergiant Fast X-ray Transients, has completely changed our view and comprehension of massive X-ray binaries. These objects display X-ray outbursts which are difficult to be explained in the framework of standard theories for the accretion of matter onto compact objects, and could represent a dominant population of X-ray binaries. I will review their main observational properties (neutron star magnetic field, orbital and spin period, long term behavior, duty cycle, quiesce"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.2835","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":""},"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":"1101.2835","created_at":"2026-05-18T02:03:39.967248+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.2835v2","created_at":"2026-05-18T02:03:39.967248+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.2835","created_at":"2026-05-18T02:03:39.967248+00:00"},{"alias_kind":"pith_short_12","alias_value":"LPRZOMELLQCV","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"LPRZOMELLQCVE2PS","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"LPRZOMEL","created_at":"2026-05-18T12:26:34.985390+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/LPRZOMELLQCVE2PSTPHGLIMB77","json":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77.json","graph_json":"https://pith.science/api/pith-number/LPRZOMELLQCVE2PSTPHGLIMB77/graph.json","events_json":"https://pith.science/api/pith-number/LPRZOMELLQCVE2PSTPHGLIMB77/events.json","paper":"https://pith.science/paper/LPRZOMEL"},"agent_actions":{"view_html":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77","download_json":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77.json","view_paper":"https://pith.science/paper/LPRZOMEL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.2835&json=true","fetch_graph":"https://pith.science/api/pith-number/LPRZOMELLQCVE2PSTPHGLIMB77/graph.json","fetch_events":"https://pith.science/api/pith-number/LPRZOMELLQCVE2PSTPHGLIMB77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77/action/storage_attestation","attest_author":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77/action/author_attestation","sign_citation":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77/action/citation_signature","submit_replication":"https://pith.science/pith/LPRZOMELLQCVE2PSTPHGLIMB77/action/replication_record"}},"created_at":"2026-05-18T02:03:39.967248+00:00","updated_at":"2026-05-18T02:03:39.967248+00:00"}