{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IWBAEJ3TQ2WZZ7W63PEPV5GOUY","short_pith_number":"pith:IWBAEJ3T","schema_version":"1.0","canonical_sha256":"458202277386ad9cfededbc8faf4cea61807de602ddfd9da7c9be13675afe227","source":{"kind":"arxiv","id":"1806.01312","version":1},"attestation_state":"computed","paper":{"title":"Broadband High-Energy Emissions of the Redback Millisecond Pulsar PSR J2129-0429","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. K. H. Kong, C. Y. Hui, J. Takata, J. Zhao, K. L. Li, P. H. T. Tam","submitted_at":"2018-06-04T18:20:46Z","abstract_excerpt":"We present the first results from a joint XMM-Newton and NuSTAR observation of the gamma-ray emitting millisecond pulsar compact binary PSR J2129-0429. X-ray emission up to about 40 keV is detected and the joint spectrum can be modeled with a power-law plus a neutron star atmosphere model. At a distance of 1.4 kpc, the 0.3-79 keV luminosity is $3.56\\times10^{32}$ erg s$^{-1}$. We also detected the 0.64-day binary orbital period with a double-peaked structure across the wavebands. By combining the updated Fermi GeV data, we modeled the broadband spectral energy distribution as well as the X-ray"},"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":"1806.01312","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-06-04T18:20:46Z","cross_cats_sorted":[],"title_canon_sha256":"5425fba8a5191a9b6424dc276dc6f3a84494830e87b4b8df89eb9fcc9a20bc21","abstract_canon_sha256":"1fad46703586eb7ddd354f3d7c4f470788a964a7d56c6bdf75ca74fb12098ac3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:04.623647Z","signature_b64":"a+f1YbAEU5KO4yzntdVD8DHliiorpILXz5i3NGimQ/noAWlLE/5etb+RJGfC+YDqnumIIo9Rov6lUxo5uYxZDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"458202277386ad9cfededbc8faf4cea61807de602ddfd9da7c9be13675afe227","last_reissued_at":"2026-05-18T00:11:04.622998Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:04.622998Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Broadband High-Energy Emissions of the Redback Millisecond Pulsar PSR J2129-0429","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. K. H. Kong, C. Y. Hui, J. Takata, J. Zhao, K. L. Li, P. H. T. Tam","submitted_at":"2018-06-04T18:20:46Z","abstract_excerpt":"We present the first results from a joint XMM-Newton and NuSTAR observation of the gamma-ray emitting millisecond pulsar compact binary PSR J2129-0429. X-ray emission up to about 40 keV is detected and the joint spectrum can be modeled with a power-law plus a neutron star atmosphere model. At a distance of 1.4 kpc, the 0.3-79 keV luminosity is $3.56\\times10^{32}$ erg s$^{-1}$. We also detected the 0.64-day binary orbital period with a double-peaked structure across the wavebands. By combining the updated Fermi GeV data, we modeled the broadband spectral energy distribution as well as the X-ray"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.01312","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":"1806.01312","created_at":"2026-05-18T00:11:04.623094+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.01312v1","created_at":"2026-05-18T00:11:04.623094+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.01312","created_at":"2026-05-18T00:11:04.623094+00:00"},{"alias_kind":"pith_short_12","alias_value":"IWBAEJ3TQ2WZ","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"IWBAEJ3TQ2WZZ7W6","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"IWBAEJ3T","created_at":"2026-05-18T12:32:31.084164+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/IWBAEJ3TQ2WZZ7W63PEPV5GOUY","json":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY.json","graph_json":"https://pith.science/api/pith-number/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/graph.json","events_json":"https://pith.science/api/pith-number/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/events.json","paper":"https://pith.science/paper/IWBAEJ3T"},"agent_actions":{"view_html":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY","download_json":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY.json","view_paper":"https://pith.science/paper/IWBAEJ3T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.01312&json=true","fetch_graph":"https://pith.science/api/pith-number/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/graph.json","fetch_events":"https://pith.science/api/pith-number/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/action/storage_attestation","attest_author":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/action/author_attestation","sign_citation":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/action/citation_signature","submit_replication":"https://pith.science/pith/IWBAEJ3TQ2WZZ7W63PEPV5GOUY/action/replication_record"}},"created_at":"2026-05-18T00:11:04.623094+00:00","updated_at":"2026-05-18T00:11:04.623094+00:00"}