{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:4MTG77CMO737DLOFAPDCT5IN5N","short_pith_number":"pith:4MTG77CM","schema_version":"1.0","canonical_sha256":"e3266ffc4c77f7f1adc503c629f50deb6b086712aeca1d853e73b706d5e78fed","source":{"kind":"arxiv","id":"1208.1904","version":2},"attestation_state":"computed","paper":{"title":"Swift XRT Timing Observations of the Black-Hole Binary SWIFTJ1753.5-0127: Disk-Diluted Fluctuations in the Outburst Peak","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Diego Altamirano, Maithili Kalamkar, Michiel van der Klis, Phil Uttley, Rudy Wijnands","submitted_at":"2012-08-09T13:32:25Z","abstract_excerpt":"After a careful analysis of the instrumental effects on the Poisson noise to demonstrate the feasibility of detailed stochastic variability studies with the Swift X-Ray Telescope (XRT), we analyze the variability of the black hole X-ray binary SWIFT J1753.5-0127 in all XRT observations during 2005-2010. We present the evolution of the power spectral components along the outburst in two energy bands: soft (0.5-2 keV) and hard (2-10 keV), and in the hard band find results consistent with those from the Rossi X-ray Timing Explorer (RXTE). The advantage of the XRT is that we can also explore the 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":"1208.1904","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-08-09T13:32:25Z","cross_cats_sorted":[],"title_canon_sha256":"b56992d055cbeba5dadae2309873764bfd4db0c5353e76caed53977631779e55","abstract_canon_sha256":"b8b41e9b8852b6380a7da56dcb23e8037a52d3e994265ec101cb1e18e206afd6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:17.173490Z","signature_b64":"3ODXc+znzVzt27zL1I9aJOd94E8JaZnHrvOoBQi4I4y+lUpaN+bGQVO60JtyvUUEq5tMFAXrkbdoTZ1sR4U3Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3266ffc4c77f7f1adc503c629f50deb6b086712aeca1d853e73b706d5e78fed","last_reissued_at":"2026-05-18T01:55:17.172995Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:17.172995Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Swift XRT Timing Observations of the Black-Hole Binary SWIFTJ1753.5-0127: Disk-Diluted Fluctuations in the Outburst Peak","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Diego Altamirano, Maithili Kalamkar, Michiel van der Klis, Phil Uttley, Rudy Wijnands","submitted_at":"2012-08-09T13:32:25Z","abstract_excerpt":"After a careful analysis of the instrumental effects on the Poisson noise to demonstrate the feasibility of detailed stochastic variability studies with the Swift X-Ray Telescope (XRT), we analyze the variability of the black hole X-ray binary SWIFT J1753.5-0127 in all XRT observations during 2005-2010. We present the evolution of the power spectral components along the outburst in two energy bands: soft (0.5-2 keV) and hard (2-10 keV), and in the hard band find results consistent with those from the Rossi X-ray Timing Explorer (RXTE). The advantage of the XRT is that we can also explore the s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.1904","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":"1208.1904","created_at":"2026-05-18T01:55:17.173068+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.1904v2","created_at":"2026-05-18T01:55:17.173068+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.1904","created_at":"2026-05-18T01:55:17.173068+00:00"},{"alias_kind":"pith_short_12","alias_value":"4MTG77CMO737","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"4MTG77CMO737DLOF","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"4MTG77CM","created_at":"2026-05-18T12:26:53.410803+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/4MTG77CMO737DLOFAPDCT5IN5N","json":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N.json","graph_json":"https://pith.science/api/pith-number/4MTG77CMO737DLOFAPDCT5IN5N/graph.json","events_json":"https://pith.science/api/pith-number/4MTG77CMO737DLOFAPDCT5IN5N/events.json","paper":"https://pith.science/paper/4MTG77CM"},"agent_actions":{"view_html":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N","download_json":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N.json","view_paper":"https://pith.science/paper/4MTG77CM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.1904&json=true","fetch_graph":"https://pith.science/api/pith-number/4MTG77CMO737DLOFAPDCT5IN5N/graph.json","fetch_events":"https://pith.science/api/pith-number/4MTG77CMO737DLOFAPDCT5IN5N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N/action/storage_attestation","attest_author":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N/action/author_attestation","sign_citation":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N/action/citation_signature","submit_replication":"https://pith.science/pith/4MTG77CMO737DLOFAPDCT5IN5N/action/replication_record"}},"created_at":"2026-05-18T01:55:17.173068+00:00","updated_at":"2026-05-18T01:55:17.173068+00:00"}