{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BGFMH4GAW5R6CWQCVI6QWBPCA3","short_pith_number":"pith:BGFMH4GA","schema_version":"1.0","canonical_sha256":"098ac3f0c0b763e15a02aa3d0b05e206d3b84893179d96f8f61695577327e662","source":{"kind":"arxiv","id":"1410.0958","version":1},"attestation_state":"computed","paper":{"title":"Research Update on Extreme-Mass-Ratio Inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Adam Pound, Carlos F. Sopuerta, Jonathan R. Gair, Pau Amaro-Seoane, Scott A. Hughes","submitted_at":"2014-10-03T20:00:01Z","abstract_excerpt":"The inspirals of stellar-mass mass compact objects into massive black holes in the centres of galaxies are one of the most important sources of gravitational radiation for space-based detectors like LISA or eLISA. These extreme-mass-ratio inspirals (EMRIs) will enable an ambitious research program with implications for astrophysics, cosmology, and fundamental physics. This article is a summary of the talks delivered at the plenary session on EMRIs at the 10th International LISA Symposium. It contains research updates on the following topics: astrophysics of EMRIs; EMRI science potential; and E"},"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":"1410.0958","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-03T20:00:01Z","cross_cats_sorted":["astro-ph.GA","gr-qc"],"title_canon_sha256":"cc6642048a97883413b3055bbcd835b7f2965d116b8bd33ef7539c5abc5d9d55","abstract_canon_sha256":"ff27baac9402ee91d7cfa73270c1d6efd1d3ed0af310d937fb5bde19b62a4d23"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:33.548192Z","signature_b64":"r10GyI94XBJCVdXNkRUxVSlQB/vv7y4MXEHdl6gWCbtjAojqVgsamJV8jtAyteZtZmjnvUa5NAZxbGWyYtsLCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"098ac3f0c0b763e15a02aa3d0b05e206d3b84893179d96f8f61695577327e662","last_reissued_at":"2026-05-18T01:55:33.547657Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:33.547657Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Research Update on Extreme-Mass-Ratio Inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Adam Pound, Carlos F. Sopuerta, Jonathan R. Gair, Pau Amaro-Seoane, Scott A. Hughes","submitted_at":"2014-10-03T20:00:01Z","abstract_excerpt":"The inspirals of stellar-mass mass compact objects into massive black holes in the centres of galaxies are one of the most important sources of gravitational radiation for space-based detectors like LISA or eLISA. These extreme-mass-ratio inspirals (EMRIs) will enable an ambitious research program with implications for astrophysics, cosmology, and fundamental physics. This article is a summary of the talks delivered at the plenary session on EMRIs at the 10th International LISA Symposium. It contains research updates on the following topics: astrophysics of EMRIs; EMRI science potential; and E"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.0958","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":"1410.0958","created_at":"2026-05-18T01:55:33.547741+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.0958v1","created_at":"2026-05-18T01:55:33.547741+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.0958","created_at":"2026-05-18T01:55:33.547741+00:00"},{"alias_kind":"pith_short_12","alias_value":"BGFMH4GAW5R6","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BGFMH4GAW5R6CWQC","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BGFMH4GA","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":30,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3","json":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3.json","graph_json":"https://pith.science/api/pith-number/BGFMH4GAW5R6CWQCVI6QWBPCA3/graph.json","events_json":"https://pith.science/api/pith-number/BGFMH4GAW5R6CWQCVI6QWBPCA3/events.json","paper":"https://pith.science/paper/BGFMH4GA"},"agent_actions":{"view_html":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3","download_json":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3.json","view_paper":"https://pith.science/paper/BGFMH4GA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.0958&json=true","fetch_graph":"https://pith.science/api/pith-number/BGFMH4GAW5R6CWQCVI6QWBPCA3/graph.json","fetch_events":"https://pith.science/api/pith-number/BGFMH4GAW5R6CWQCVI6QWBPCA3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3/action/storage_attestation","attest_author":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3/action/author_attestation","sign_citation":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3/action/citation_signature","submit_replication":"https://pith.science/pith/BGFMH4GAW5R6CWQCVI6QWBPCA3/action/replication_record"}},"created_at":"2026-05-18T01:55:33.547741+00:00","updated_at":"2026-05-18T01:55:33.547741+00:00"}