{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:4OSOAMGEUHOFRCNGLRM4U5DPLH","short_pith_number":"pith:4OSOAMGE","schema_version":"1.0","canonical_sha256":"e3a4e030c4a1dc5889a65c59ca746f59d99d095388036f91a654171005cfad26","source":{"kind":"arxiv","id":"1703.09722","version":2},"attestation_state":"computed","paper":{"title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA"],"primary_cat":"gr-qc","authors_text":"Alberto Sesana, Antoine Klein, Antoine Petiteau, Carlos F. Sopuerta, Christopher P. L. Berry, Emanuele Berti, Enrico Barausse, Jonathan Gair, Pau Amaro-Seoane, Stanislav Babak","submitted_at":"2017-03-28T18:00:17Z","abstract_excerpt":"The space-based Laser Interferometer Space Antenna (LISA) will be able to observe the gravitational-wave signals from systems comprised of a massive black hole and a stellar-mass compact object. These systems are known as extreme-mass-ratio inspirals (EMRIs) and are expected to complete $\\sim 10^4$-$10^5$ cycles in band, thus allowing exquisite measurements of their parameters. In this work, we attempt to quantify the astrophysical uncertainties affecting the predictions for the number of EMRIs detectable by LISA, and find that competing astrophysical assumptions produce a variance of about th"},"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":"1703.09722","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-03-28T18:00:17Z","cross_cats_sorted":["astro-ph.CO","astro-ph.GA"],"title_canon_sha256":"4552c7d468b6e3653f2366a2a317df12527b47f49a750c91582236a9bdee605e","abstract_canon_sha256":"85c5109696ab0768ed164796cd997d09460d7bcf44aedf5e785038bc3b5f0640"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:18:46.620715Z","signature_b64":"zDOctdcxVHhqY13ynmS4HvT+SustxjPRgKgToctXnxergiKwJZy09LACGEcCLih5qwt/89+dOhspi9Y4LwEjDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3a4e030c4a1dc5889a65c59ca746f59d99d095388036f91a654171005cfad26","last_reissued_at":"2026-05-18T00:18:46.611439Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:18:46.611439Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA"],"primary_cat":"gr-qc","authors_text":"Alberto Sesana, Antoine Klein, Antoine Petiteau, Carlos F. Sopuerta, Christopher P. L. Berry, Emanuele Berti, Enrico Barausse, Jonathan Gair, Pau Amaro-Seoane, Stanislav Babak","submitted_at":"2017-03-28T18:00:17Z","abstract_excerpt":"The space-based Laser Interferometer Space Antenna (LISA) will be able to observe the gravitational-wave signals from systems comprised of a massive black hole and a stellar-mass compact object. These systems are known as extreme-mass-ratio inspirals (EMRIs) and are expected to complete $\\sim 10^4$-$10^5$ cycles in band, thus allowing exquisite measurements of their parameters. In this work, we attempt to quantify the astrophysical uncertainties affecting the predictions for the number of EMRIs detectable by LISA, and find that competing astrophysical assumptions produce a variance of about th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.09722","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":"1703.09722","created_at":"2026-05-18T00:18:46.611679+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.09722v2","created_at":"2026-05-18T00:18:46.611679+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.09722","created_at":"2026-05-18T00:18:46.611679+00:00"},{"alias_kind":"pith_short_12","alias_value":"4OSOAMGEUHOF","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"4OSOAMGEUHOFRCNG","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"4OSOAMGE","created_at":"2026-05-18T12:31:00.734936+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":26,"internal_anchor_count":13,"sample":[{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":73,"is_internal_anchor":true},{"citing_arxiv_id":"2401.13668","citing_title":"Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites","ref_index":79,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22210","citing_title":"Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\\star$","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19673","citing_title":"Spin-Hair Induced Chaos of Spinning Test Particles in Rotating Hairy Black Holes","ref_index":70,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19197","citing_title":"CP-violating multi-field phase transitions and gravitational waves in a hidden NJL sector","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2508.16399","citing_title":"Constraints on the extreme mass-ratio inspiral population from LISA data","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2509.09986","citing_title":"Plunge spectra as discriminators of black hole mimickers","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2512.16322","citing_title":"First-time assessment of glitch-induced bias and uncertainty in inference of extreme mass ratio inspirals","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2602.11001","citing_title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2010.14529","citing_title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","ref_index":181,"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":86,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13847","citing_title":"Analytical Fluxes from Generic Schwarzschild Geodesics","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09250","citing_title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26011","citing_title":"Parameter-estimation bias induced by transient orbital resonances in extreme-mass-ratio inspirals","ref_index":7,"is_internal_anchor":false},{"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":14,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23163","citing_title":"Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole","ref_index":43,"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":24,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00976","citing_title":"Self-acceleration of Hardening Binaries","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19197","citing_title":"CP-violating multi-field phase transitions and gravitational waves in a hidden NJL sector","ref_index":9,"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":58,"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":24,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06009","citing_title":"Are Black Holes Fuzzballs? Probing Horizon-Scale Structure with LISA","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH","json":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH.json","graph_json":"https://pith.science/api/pith-number/4OSOAMGEUHOFRCNGLRM4U5DPLH/graph.json","events_json":"https://pith.science/api/pith-number/4OSOAMGEUHOFRCNGLRM4U5DPLH/events.json","paper":"https://pith.science/paper/4OSOAMGE"},"agent_actions":{"view_html":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH","download_json":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH.json","view_paper":"https://pith.science/paper/4OSOAMGE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.09722&json=true","fetch_graph":"https://pith.science/api/pith-number/4OSOAMGEUHOFRCNGLRM4U5DPLH/graph.json","fetch_events":"https://pith.science/api/pith-number/4OSOAMGEUHOFRCNGLRM4U5DPLH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH/action/storage_attestation","attest_author":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH/action/author_attestation","sign_citation":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH/action/citation_signature","submit_replication":"https://pith.science/pith/4OSOAMGEUHOFRCNGLRM4U5DPLH/action/replication_record"}},"created_at":"2026-05-18T00:18:46.611679+00:00","updated_at":"2026-05-18T00:18:46.611679+00:00"}