{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:VXHTMONCIAN73MZ4PPOCH5DLO3","short_pith_number":"pith:VXHTMONC","schema_version":"1.0","canonical_sha256":"adcf3639a2401bfdb33c7bdc23f46b76f325f381f64eb6113f928b8452fd006b","source":{"kind":"arxiv","id":"1205.1804","version":1},"attestation_state":"computed","paper":{"title":"Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626-67","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Yoshida, K. Makishima, L. Angelini, M. Nakajima, M. S. Tashiro, S. Yamada, T. Enoto, T. Mihara, W. B. Iwakiri, Y. Terada","submitted_at":"2012-05-08T20:00:13Z","abstract_excerpt":"We present analysis of 4U 1626-67, a 7.7 s pulsar in a low-mass X-ray binary system, observed with the hard X-ray detector of the Japanese X-ray satellite Suzaku in March 2006 for a net exposure of \\sim88 ks. The source was detected at an average 10-60 keV flux of \\sim4 x10^-10 erg cm^-2 s^-1. The phase-averaged spectrum is reproduced well by combining a negative and positive power-law times exponential cutoff (NPEX) model modified at \\sim 37 keV by a cyclotron resonance scattering feature (CRSF). The phase-resolved analysis shows that the spectra at the bright phases are well fit by the NPEX "},"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":"1205.1804","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-05-08T20:00:13Z","cross_cats_sorted":[],"title_canon_sha256":"a690c3d5396ab518854d4ede78980bc1119f12bded1008a28d88327fcf755d3e","abstract_canon_sha256":"5bcce22405073d2081c0db8cc9515545d9adfa2377cba484997f783f448c54a9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:36.464075Z","signature_b64":"CJuVMPQiTjx5nicnE7JGre0YPFRVhUfdFTYzwsWgdHGHeyofr8oXbBatGo4v0pLUjEYcRrFvXSezysMYszymBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adcf3639a2401bfdb33c7bdc23f46b76f325f381f64eb6113f928b8452fd006b","last_reissued_at":"2026-05-18T01:57:36.463401Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:36.463401Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626-67","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Yoshida, K. Makishima, L. Angelini, M. Nakajima, M. S. Tashiro, S. Yamada, T. Enoto, T. Mihara, W. B. Iwakiri, Y. Terada","submitted_at":"2012-05-08T20:00:13Z","abstract_excerpt":"We present analysis of 4U 1626-67, a 7.7 s pulsar in a low-mass X-ray binary system, observed with the hard X-ray detector of the Japanese X-ray satellite Suzaku in March 2006 for a net exposure of \\sim88 ks. The source was detected at an average 10-60 keV flux of \\sim4 x10^-10 erg cm^-2 s^-1. The phase-averaged spectrum is reproduced well by combining a negative and positive power-law times exponential cutoff (NPEX) model modified at \\sim 37 keV by a cyclotron resonance scattering feature (CRSF). The phase-resolved analysis shows that the spectra at the bright phases are well fit by the NPEX "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.1804","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":"1205.1804","created_at":"2026-05-18T01:57:36.463512+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.1804v1","created_at":"2026-05-18T01:57:36.463512+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.1804","created_at":"2026-05-18T01:57:36.463512+00:00"},{"alias_kind":"pith_short_12","alias_value":"VXHTMONCIAN7","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"VXHTMONCIAN73MZ4","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"VXHTMONC","created_at":"2026-05-18T12:27:25.539911+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/VXHTMONCIAN73MZ4PPOCH5DLO3","json":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3.json","graph_json":"https://pith.science/api/pith-number/VXHTMONCIAN73MZ4PPOCH5DLO3/graph.json","events_json":"https://pith.science/api/pith-number/VXHTMONCIAN73MZ4PPOCH5DLO3/events.json","paper":"https://pith.science/paper/VXHTMONC"},"agent_actions":{"view_html":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3","download_json":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3.json","view_paper":"https://pith.science/paper/VXHTMONC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.1804&json=true","fetch_graph":"https://pith.science/api/pith-number/VXHTMONCIAN73MZ4PPOCH5DLO3/graph.json","fetch_events":"https://pith.science/api/pith-number/VXHTMONCIAN73MZ4PPOCH5DLO3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3/action/storage_attestation","attest_author":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3/action/author_attestation","sign_citation":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3/action/citation_signature","submit_replication":"https://pith.science/pith/VXHTMONCIAN73MZ4PPOCH5DLO3/action/replication_record"}},"created_at":"2026-05-18T01:57:36.463512+00:00","updated_at":"2026-05-18T01:57:36.463512+00:00"}