{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:5XGCWJ4WVBX2C4IA4CMIOX3XZS","short_pith_number":"pith:5XGCWJ4W","schema_version":"1.0","canonical_sha256":"edcc2b2796a86fa17100e098875f77cc95295e5d2e147f0283dc7eaba228105d","source":{"kind":"arxiv","id":"1410.3357","version":1},"attestation_state":"computed","paper":{"title":"Iron K and Compton hump reverberation in SWIFT J2127.4+5654 and NGC 1365 revealed by NuSTAR and XMM-Newton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. C. Fabian, A. Marinucci, A. Zoghbi, C. J. Hailey, C. S. Reynolds, D. J. Walton, D. Stern, E. Kara, F. A. Harrison, F. E. Christensen, F. Fuerst, G. Matt, G. Risaliti, M. L. Parker, S. E. Boggs, W. W. Zhang","submitted_at":"2014-10-13T15:40:11Z","abstract_excerpt":"In the past five years, a flurry of X-ray reverberation lag measurements of accreting supermassive black holes have been made using the XMM-Newton telescope in the 0.3-10 keV energy range. In this work, we use the NuSTAR telescope to extend the lag analysis up to higher energies for two Seyfert galaxies, SWIFT J2127.4+5654 and NGC 1365. X-ray reverberation lags are due to the light travel time delays between the direct continuum emission and the reprocessed emission from the inner radii of an ionised accretion disc. XMM-Newton has been particularly adept at measuring the lag associated with th"},"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":"1410.3357","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-10-13T15:40:11Z","cross_cats_sorted":[],"title_canon_sha256":"ff8278882bdd17c1f405c31e0df502700b99826b64e90af8822e283c3c8b7540","abstract_canon_sha256":"3b0817d9d55a9b3480cf7ec58493b5f782194b94e2cc71945cf5ece482cdc041"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:48.816472Z","signature_b64":"DpSly2CSaDGejrWGB5+joCjs87QOhx8YZ8T+4Ym6aiWuLbZH7rXlrNgz81jDGbKdgxfva43cEsHnp4jB+DTDCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"edcc2b2796a86fa17100e098875f77cc95295e5d2e147f0283dc7eaba228105d","last_reissued_at":"2026-05-18T01:41:48.815865Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:48.815865Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Iron K and Compton hump reverberation in SWIFT J2127.4+5654 and NGC 1365 revealed by NuSTAR and XMM-Newton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. C. Fabian, A. Marinucci, A. Zoghbi, C. J. Hailey, C. S. Reynolds, D. J. Walton, D. Stern, E. Kara, F. A. Harrison, F. E. Christensen, F. Fuerst, G. Matt, G. Risaliti, M. L. Parker, S. E. Boggs, W. W. Zhang","submitted_at":"2014-10-13T15:40:11Z","abstract_excerpt":"In the past five years, a flurry of X-ray reverberation lag measurements of accreting supermassive black holes have been made using the XMM-Newton telescope in the 0.3-10 keV energy range. In this work, we use the NuSTAR telescope to extend the lag analysis up to higher energies for two Seyfert galaxies, SWIFT J2127.4+5654 and NGC 1365. X-ray reverberation lags are due to the light travel time delays between the direct continuum emission and the reprocessed emission from the inner radii of an ionised accretion disc. XMM-Newton has been particularly adept at measuring the lag associated with th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.3357","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":"1410.3357","created_at":"2026-05-18T01:41:48.815980+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.3357v1","created_at":"2026-05-18T01:41:48.815980+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3357","created_at":"2026-05-18T01:41:48.815980+00:00"},{"alias_kind":"pith_short_12","alias_value":"5XGCWJ4WVBX2","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"5XGCWJ4WVBX2C4IA","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"5XGCWJ4W","created_at":"2026-05-18T12:28:16.859392+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22918","citing_title":"Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds","ref_index":145,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS","json":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS.json","graph_json":"https://pith.science/api/pith-number/5XGCWJ4WVBX2C4IA4CMIOX3XZS/graph.json","events_json":"https://pith.science/api/pith-number/5XGCWJ4WVBX2C4IA4CMIOX3XZS/events.json","paper":"https://pith.science/paper/5XGCWJ4W"},"agent_actions":{"view_html":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS","download_json":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS.json","view_paper":"https://pith.science/paper/5XGCWJ4W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.3357&json=true","fetch_graph":"https://pith.science/api/pith-number/5XGCWJ4WVBX2C4IA4CMIOX3XZS/graph.json","fetch_events":"https://pith.science/api/pith-number/5XGCWJ4WVBX2C4IA4CMIOX3XZS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS/action/storage_attestation","attest_author":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS/action/author_attestation","sign_citation":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS/action/citation_signature","submit_replication":"https://pith.science/pith/5XGCWJ4WVBX2C4IA4CMIOX3XZS/action/replication_record"}},"created_at":"2026-05-18T01:41:48.815980+00:00","updated_at":"2026-05-18T01:41:48.815980+00:00"}