{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:4BZJQNNNPZR43GU3AM3HOZ2KYG","short_pith_number":"pith:4BZJQNNN","schema_version":"1.0","canonical_sha256":"e0729835ad7e63cd9a9b033677674ac19f32f37ad26dc5191f36a380e520f853","source":{"kind":"arxiv","id":"1311.0065","version":3},"attestation_state":"computed","paper":{"title":"New Coordinates for the Amplitude Parameter Space of Continuous Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Curt J. Cutler, John T. Whelan, Joshua L. Willis, Reinhard Prix","submitted_at":"2013-11-01T00:17:03Z","abstract_excerpt":"The parameter space for continuous gravitational waves (GWs) can be divided into amplitude parameters (signal amplitude, inclination and polarization angles describing the orientation of the source, and an initial phase) and phase-evolution parameters. The division is useful in part because the Jaranowski-Krolak-Schutz (JKS) coordinates on the four-dimensional amplitude parameter space allow the GW signal to be written as a linear combination of four template waveforms with the JKS coordinates as coefficients. We define a new set of coordinates on the amplitude parameter space, with the same p"},"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":"1311.0065","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2013-11-01T00:17:03Z","cross_cats_sorted":[],"title_canon_sha256":"78548147b22c988c237bfbf4aab7fa1f42a8cf179e8986286c43c27e7ccd5230","abstract_canon_sha256":"6783a50bb2dcaff223183f46e92e891c2504da0f44eb14ecc4b9b21121827fe0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:57:52.417089Z","signature_b64":"ZC6DQjt5UA0uZC1Yt+hkvgkThTEsI71TTvxhUlxQO5UlzoG1AwS+s2E5ddt2Oaz8Oik1QQo4proBkQZ8PBh/DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e0729835ad7e63cd9a9b033677674ac19f32f37ad26dc5191f36a380e520f853","last_reissued_at":"2026-05-18T02:57:52.416495Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:57:52.416495Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New Coordinates for the Amplitude Parameter Space of Continuous Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Curt J. Cutler, John T. Whelan, Joshua L. Willis, Reinhard Prix","submitted_at":"2013-11-01T00:17:03Z","abstract_excerpt":"The parameter space for continuous gravitational waves (GWs) can be divided into amplitude parameters (signal amplitude, inclination and polarization angles describing the orientation of the source, and an initial phase) and phase-evolution parameters. The division is useful in part because the Jaranowski-Krolak-Schutz (JKS) coordinates on the four-dimensional amplitude parameter space allow the GW signal to be written as a linear combination of four template waveforms with the JKS coordinates as coefficients. We define a new set of coordinates on the amplitude parameter space, with the same p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.0065","kind":"arxiv","version":3},"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":"1311.0065","created_at":"2026-05-18T02:57:52.416581+00:00"},{"alias_kind":"arxiv_version","alias_value":"1311.0065v3","created_at":"2026-05-18T02:57:52.416581+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.0065","created_at":"2026-05-18T02:57:52.416581+00:00"},{"alias_kind":"pith_short_12","alias_value":"4BZJQNNNPZR4","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"4BZJQNNNPZR43GU3","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"4BZJQNNN","created_at":"2026-05-18T12:27:32.513160+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.14849","citing_title":"A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences","ref_index":42,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG","json":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG.json","graph_json":"https://pith.science/api/pith-number/4BZJQNNNPZR43GU3AM3HOZ2KYG/graph.json","events_json":"https://pith.science/api/pith-number/4BZJQNNNPZR43GU3AM3HOZ2KYG/events.json","paper":"https://pith.science/paper/4BZJQNNN"},"agent_actions":{"view_html":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG","download_json":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG.json","view_paper":"https://pith.science/paper/4BZJQNNN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1311.0065&json=true","fetch_graph":"https://pith.science/api/pith-number/4BZJQNNNPZR43GU3AM3HOZ2KYG/graph.json","fetch_events":"https://pith.science/api/pith-number/4BZJQNNNPZR43GU3AM3HOZ2KYG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG/action/storage_attestation","attest_author":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG/action/author_attestation","sign_citation":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG/action/citation_signature","submit_replication":"https://pith.science/pith/4BZJQNNNPZR43GU3AM3HOZ2KYG/action/replication_record"}},"created_at":"2026-05-18T02:57:52.416581+00:00","updated_at":"2026-05-18T02:57:52.416581+00:00"}