{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:FUSNKBNHZKKMVXCWG7UWAYJ3KV","short_pith_number":"pith:FUSNKBNH","schema_version":"1.0","canonical_sha256":"2d24d505a7ca94cadc5637e960613b5561ae5e1254ae60848bde7721c608dbcd","source":{"kind":"arxiv","id":"gr-qc/0607007","version":2},"attestation_state":"computed","paper":{"title":"\"Kludge\" gravitational waveforms for a test-body orbiting a Kerr black hole","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"gr-qc","authors_text":"Hua Fang, Jonathan R. Gair, Kostas Glampedakis, Scott A. Hughes, Stanislav Babak","submitted_at":"2006-07-03T11:58:31Z","abstract_excerpt":"One of the most exciting potential sources of gravitational waves for low-frequency, space-based gravitational wave (GW) detectors such as the proposed Laser Interferometer Space Antenna (LISA) is the inspiral of compact objects into massive black holes in the centers of galaxies. The detection of waves from such \"extreme mass ratio inspiral\" systems (EMRIs) and extraction of information from those waves require template waveforms. The systems' extreme mass ratio means that their waveforms can be determined accurately using black hole perturbation theory. Such calculations are computationally "},"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":"gr-qc/0607007","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2006-07-03T11:58:31Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"233e772ac3a1f814ad058561ecd12c4ce7eafceaac9f3f6920fca79ef64989b0","abstract_canon_sha256":"ee4ac1d01622aa8601ad02b9e65f1566077396acdd0fa39f0b7abe2ec478a19b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:37:27.136414Z","signature_b64":"C1QlKSvcBYzPS4luXlr98Q7Pb9nRqzhnjkvQsjbHyfIa1hH3V/hUbt6Zv5HFlf2NuwgNz4kRH0ufylPBZB4KDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2d24d505a7ca94cadc5637e960613b5561ae5e1254ae60848bde7721c608dbcd","last_reissued_at":"2026-05-18T02:37:27.135917Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:37:27.135917Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"\"Kludge\" gravitational waveforms for a test-body orbiting a Kerr black hole","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"gr-qc","authors_text":"Hua Fang, Jonathan R. Gair, Kostas Glampedakis, Scott A. Hughes, Stanislav Babak","submitted_at":"2006-07-03T11:58:31Z","abstract_excerpt":"One of the most exciting potential sources of gravitational waves for low-frequency, space-based gravitational wave (GW) detectors such as the proposed Laser Interferometer Space Antenna (LISA) is the inspiral of compact objects into massive black holes in the centers of galaxies. The detection of waves from such \"extreme mass ratio inspiral\" systems (EMRIs) and extraction of information from those waves require template waveforms. The systems' extreme mass ratio means that their waveforms can be determined accurately using black hole perturbation theory. Such calculations are computationally "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0607007","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":"gr-qc/0607007","created_at":"2026-05-18T02:37:27.135996+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0607007v2","created_at":"2026-05-18T02:37:27.135996+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0607007","created_at":"2026-05-18T02:37:27.135996+00:00"},{"alias_kind":"pith_short_12","alias_value":"FUSNKBNHZKKM","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"FUSNKBNHZKKMVXCW","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"FUSNKBNH","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":6,"sample":[{"citing_arxiv_id":"2605.19121","citing_title":"Ringdown Signatures of Dehnen Dark Matter Halos: Fluid Modes and Detectability with Space-Based Detectors","ref_index":63,"is_internal_anchor":true},{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2509.23318","citing_title":"Gravitational waveforms from periodic orbits around a novel regular black hole","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"2512.11911","citing_title":"Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity","ref_index":102,"is_internal_anchor":true},{"citing_arxiv_id":"2601.00550","citing_title":"Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":98,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24413","citing_title":"Gravitational waves of extreme-mass-ratio inspirals in a rotating black hole with Dehnen dark matter halo","ref_index":82,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05362","citing_title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11866","citing_title":"Equatorial periodic orbits and gravitational wave signatures in Euler-Heisenberg black holes surrounded by perfect fluid dark matter","ref_index":68,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05362","citing_title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":132,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13564","citing_title":"Topologically equivalent yet radiatively distinct orbits in EMRI system","ref_index":30,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV","json":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV.json","graph_json":"https://pith.science/api/pith-number/FUSNKBNHZKKMVXCWG7UWAYJ3KV/graph.json","events_json":"https://pith.science/api/pith-number/FUSNKBNHZKKMVXCWG7UWAYJ3KV/events.json","paper":"https://pith.science/paper/FUSNKBNH"},"agent_actions":{"view_html":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV","download_json":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV.json","view_paper":"https://pith.science/paper/FUSNKBNH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0607007&json=true","fetch_graph":"https://pith.science/api/pith-number/FUSNKBNHZKKMVXCWG7UWAYJ3KV/graph.json","fetch_events":"https://pith.science/api/pith-number/FUSNKBNHZKKMVXCWG7UWAYJ3KV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV/action/storage_attestation","attest_author":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV/action/author_attestation","sign_citation":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV/action/citation_signature","submit_replication":"https://pith.science/pith/FUSNKBNHZKKMVXCWG7UWAYJ3KV/action/replication_record"}},"created_at":"2026-05-18T02:37:27.135996+00:00","updated_at":"2026-05-18T02:37:27.135996+00:00"}