{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:NDOYTFFX2D7CVPS6OULEXWO3CV","short_pith_number":"pith:NDOYTFFX","schema_version":"1.0","canonical_sha256":"68dd8994b7d0fe2abe5e75164bd9db1555d47c722ad7b0acde9ac5110bfc2f6a","source":{"kind":"arxiv","id":"1809.00814","version":1},"attestation_state":"computed","paper":{"title":"An INTEGRAL overview of High Mass X-ray Binaries: classes or transitions?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Adamantia Paizis (INAF/IASF-Milano, Italy), Lara Sidoli","submitted_at":"2018-09-04T07:11:20Z","abstract_excerpt":"We analyzed in a systematic way the public INTEGRAL observations spanning from December 2002 to September 2016, to investigate the hard X-ray properties of about 60 High Mass X-ray Binaries (HMXBs). We considered both persistent and transient sources, hosting either a Be star (Be/XRBs) or a blue supergiant companion (SgHMXBs, including Supergiant Fast X-ray Transients, SFXTs), a neutron star or a black hole. INTEGRAL X-ray light curves (18-50 keV), sampled at a bin time of about 2 ks, were extracted for all HMXBs to derive the cumulative distribution of their hard X-ray luminosity, their duty "},"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":"1809.00814","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-09-04T07:11:20Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"7919aea4d57d0dc07aa9fd8f8fc06affb9420130181adf385ddc94e97de72944","abstract_canon_sha256":"b70fb0aea56c271dd01a439983a0e7480aec11f460607d42c0583925d5d77593"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:06:00.806131Z","signature_b64":"4lFFkA718CV8rlkKYH79C8x70yr44TK5d/sqLfjFg/6WmZvtmJNYkBesPMg2x3z+cifECnUf9kES4UW5DN1VAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"68dd8994b7d0fe2abe5e75164bd9db1555d47c722ad7b0acde9ac5110bfc2f6a","last_reissued_at":"2026-05-18T00:06:00.805664Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:06:00.805664Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An INTEGRAL overview of High Mass X-ray Binaries: classes or transitions?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Adamantia Paizis (INAF/IASF-Milano, Italy), Lara Sidoli","submitted_at":"2018-09-04T07:11:20Z","abstract_excerpt":"We analyzed in a systematic way the public INTEGRAL observations spanning from December 2002 to September 2016, to investigate the hard X-ray properties of about 60 High Mass X-ray Binaries (HMXBs). We considered both persistent and transient sources, hosting either a Be star (Be/XRBs) or a blue supergiant companion (SgHMXBs, including Supergiant Fast X-ray Transients, SFXTs), a neutron star or a black hole. INTEGRAL X-ray light curves (18-50 keV), sampled at a bin time of about 2 ks, were extracted for all HMXBs to derive the cumulative distribution of their hard X-ray luminosity, their duty "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.00814","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":"1809.00814","created_at":"2026-05-18T00:06:00.805733+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.00814v1","created_at":"2026-05-18T00:06:00.805733+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.00814","created_at":"2026-05-18T00:06:00.805733+00:00"},{"alias_kind":"pith_short_12","alias_value":"NDOYTFFX2D7C","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_16","alias_value":"NDOYTFFX2D7CVPS6","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_8","alias_value":"NDOYTFFX","created_at":"2026-05-18T12:32:40.477152+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/NDOYTFFX2D7CVPS6OULEXWO3CV","json":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV.json","graph_json":"https://pith.science/api/pith-number/NDOYTFFX2D7CVPS6OULEXWO3CV/graph.json","events_json":"https://pith.science/api/pith-number/NDOYTFFX2D7CVPS6OULEXWO3CV/events.json","paper":"https://pith.science/paper/NDOYTFFX"},"agent_actions":{"view_html":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV","download_json":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV.json","view_paper":"https://pith.science/paper/NDOYTFFX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.00814&json=true","fetch_graph":"https://pith.science/api/pith-number/NDOYTFFX2D7CVPS6OULEXWO3CV/graph.json","fetch_events":"https://pith.science/api/pith-number/NDOYTFFX2D7CVPS6OULEXWO3CV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV/action/storage_attestation","attest_author":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV/action/author_attestation","sign_citation":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV/action/citation_signature","submit_replication":"https://pith.science/pith/NDOYTFFX2D7CVPS6OULEXWO3CV/action/replication_record"}},"created_at":"2026-05-18T00:06:00.805733+00:00","updated_at":"2026-05-18T00:06:00.805733+00:00"}