{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:6RHXGQBVEI2TBTMOY33Y33AEGF","short_pith_number":"pith:6RHXGQBV","schema_version":"1.0","canonical_sha256":"f44f734035223530cd8ec6f78dec043146296b8cae2fc94db6c0f1641f00697e","source":{"kind":"arxiv","id":"1612.09110","version":1},"attestation_state":"computed","paper":{"title":"The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hai-Hui Zhao, Jing-Ping Cai, Jin-Lu Qu, Qi-Rong Yuan, Shan-Shan Weng","submitted_at":"2016-12-29T11:56:16Z","abstract_excerpt":"The spectral and temporal evolution during X-ray outbursts give important clues on the accretion process and radiation mechanism in black-hole X-ray binaries (BH XRBs). A set of Swift and RXTE observations were executed to monitor the 2008 outburst of the black-hole candidate Swift J1842.5-1124. We investigate these data to explore the accretion physics in BH XRBs. We carry out a comprehensive spectral and timing analysis on all the available pointing observations, including fitting both X-ray spectra and power density spectra, measuring the optical and near-ultraviolet flux density. We also s"},"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":"1612.09110","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-29T11:56:16Z","cross_cats_sorted":[],"title_canon_sha256":"9b485e3497e9b8e20f5a48a92302b335cd11a2f5b12bbe5958af5a802fb23644","abstract_canon_sha256":"8658cc1a0e5b90e19f76c7d29f987aec7fd9e9ef53e4a25699c2f805c284995a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:29.159283Z","signature_b64":"LNHAYOkRDlntNllmt5L8L1174lhKVupfA1CmbEhNvxndCiXUI+Ti3eQTQWCj1FGnf6kqmmqWU8cMS03B1TfZAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f44f734035223530cd8ec6f78dec043146296b8cae2fc94db6c0f1641f00697e","last_reissued_at":"2026-05-18T00:53:29.158817Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:29.158817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hai-Hui Zhao, Jing-Ping Cai, Jin-Lu Qu, Qi-Rong Yuan, Shan-Shan Weng","submitted_at":"2016-12-29T11:56:16Z","abstract_excerpt":"The spectral and temporal evolution during X-ray outbursts give important clues on the accretion process and radiation mechanism in black-hole X-ray binaries (BH XRBs). A set of Swift and RXTE observations were executed to monitor the 2008 outburst of the black-hole candidate Swift J1842.5-1124. We investigate these data to explore the accretion physics in BH XRBs. We carry out a comprehensive spectral and timing analysis on all the available pointing observations, including fitting both X-ray spectra and power density spectra, measuring the optical and near-ultraviolet flux density. We also s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.09110","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":"1612.09110","created_at":"2026-05-18T00:53:29.158889+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.09110v1","created_at":"2026-05-18T00:53:29.158889+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.09110","created_at":"2026-05-18T00:53:29.158889+00:00"},{"alias_kind":"pith_short_12","alias_value":"6RHXGQBVEI2T","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"6RHXGQBVEI2TBTMO","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"6RHXGQBV","created_at":"2026-05-18T12:30:01.593930+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/6RHXGQBVEI2TBTMOY33Y33AEGF","json":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF.json","graph_json":"https://pith.science/api/pith-number/6RHXGQBVEI2TBTMOY33Y33AEGF/graph.json","events_json":"https://pith.science/api/pith-number/6RHXGQBVEI2TBTMOY33Y33AEGF/events.json","paper":"https://pith.science/paper/6RHXGQBV"},"agent_actions":{"view_html":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF","download_json":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF.json","view_paper":"https://pith.science/paper/6RHXGQBV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.09110&json=true","fetch_graph":"https://pith.science/api/pith-number/6RHXGQBVEI2TBTMOY33Y33AEGF/graph.json","fetch_events":"https://pith.science/api/pith-number/6RHXGQBVEI2TBTMOY33Y33AEGF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF/action/storage_attestation","attest_author":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF/action/author_attestation","sign_citation":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF/action/citation_signature","submit_replication":"https://pith.science/pith/6RHXGQBVEI2TBTMOY33Y33AEGF/action/replication_record"}},"created_at":"2026-05-18T00:53:29.158889+00:00","updated_at":"2026-05-18T00:53:29.158889+00:00"}