{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:UXZI6NJURFILSUGUUFEBRBO4DI","short_pith_number":"pith:UXZI6NJU","schema_version":"1.0","canonical_sha256":"a5f28f35348950b950d4a1481885dc1a19cfab2ab2d25c57f4ed0453c94d93d4","source":{"kind":"arxiv","id":"1409.7215","version":2},"attestation_state":"computed","paper":{"title":"Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Alberto Vecchio, Ben Aylott, Benjamin Farr, Carl-Johan Haster, Carl Rodriguez, Christian R\\\"over, Farhan Feroz, Ilya Mandel, John Veitch, Jonathan Gair, Kent Blackburn, Leslie Wade, Marc van der Sluys, Matthew Pitkin, Michael Coughlin, Nelson Christensen, Philip Graff, Richard O'Shaughnessy, Rory Smith, Salvatore Vitale, Trevor Sidery, Tyson Littenberg, Vicky Kalogera, Vivien Raymond, Walter Del Pozzo, Will M. Farr, Will Vousden","submitted_at":"2014-09-25T11:24:49Z","abstract_excerpt":"The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the coming years, with compact binary coalescence events a likely source for the first detections. The gravitational waveforms emitted directly encode information about the sources, including the masses and spins of the compact objects. Recovering the physical parameters of the sources from the GW observations is a key analysis task. This work describes the LALInference software library for Bayesian parameter estimation of compact binary signals, which builds on several previous methods to provide a "},"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":"1409.7215","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-09-25T11:24:49Z","cross_cats_sorted":["astro-ph.HE","astro-ph.IM"],"title_canon_sha256":"f8f82201f4873356148f88661fe65cfdf1de703d742c1bc46df8559857b2ff3c","abstract_canon_sha256":"3d953316961103aa25664e49aec8097b071ff51579f53d873375889432ba4681"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:27:05.237897Z","signature_b64":"C/bTBgpJ6jtUEYxo3U4Lr4um/kwiZfcNVLHlyAxWX7/poMwcZ/CahawQYXraiInX9Ng70FKk4M5KqcEwOVR1Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a5f28f35348950b950d4a1481885dc1a19cfab2ab2d25c57f4ed0453c94d93d4","last_reissued_at":"2026-05-18T02:27:05.237515Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:27:05.237515Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Alberto Vecchio, Ben Aylott, Benjamin Farr, Carl-Johan Haster, Carl Rodriguez, Christian R\\\"over, Farhan Feroz, Ilya Mandel, John Veitch, Jonathan Gair, Kent Blackburn, Leslie Wade, Marc van der Sluys, Matthew Pitkin, Michael Coughlin, Nelson Christensen, Philip Graff, Richard O'Shaughnessy, Rory Smith, Salvatore Vitale, Trevor Sidery, Tyson Littenberg, Vicky Kalogera, Vivien Raymond, Walter Del Pozzo, Will M. Farr, Will Vousden","submitted_at":"2014-09-25T11:24:49Z","abstract_excerpt":"The Advanced LIGO and Advanced Virgo gravitational wave (GW) detectors will begin operation in the coming years, with compact binary coalescence events a likely source for the first detections. The gravitational waveforms emitted directly encode information about the sources, including the masses and spins of the compact objects. Recovering the physical parameters of the sources from the GW observations is a key analysis task. This work describes the LALInference software library for Bayesian parameter estimation of compact binary signals, which builds on several previous methods to provide a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.7215","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":"1409.7215","created_at":"2026-05-18T02:27:05.237584+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.7215v2","created_at":"2026-05-18T02:27:05.237584+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.7215","created_at":"2026-05-18T02:27:05.237584+00:00"},{"alias_kind":"pith_short_12","alias_value":"UXZI6NJURFIL","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"UXZI6NJURFILSUGU","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"UXZI6NJU","created_at":"2026-05-18T12:28:52.271510+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":23,"internal_anchor_count":13,"sample":[{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":160,"is_internal_anchor":true},{"citing_arxiv_id":"2512.17550","citing_title":"GW231123: Overlapping Gravitational Wave Signals?","ref_index":49,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21531","citing_title":"Fisher Information Velocity: A New Geometric Channel for Precision Glitch Identification in Gravitational-Wave Detectors","ref_index":67,"is_internal_anchor":true},{"citing_arxiv_id":"2505.20996","citing_title":"Parameter inference of millilensed gravitational waves using neural spline flows","ref_index":77,"is_internal_anchor":true},{"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":11,"is_internal_anchor":true},{"citing_arxiv_id":"2512.10344","citing_title":"Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"1905.00869","citing_title":"Testing the no-hair theorem with GW150914","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2108.01045","citing_title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","ref_index":138,"is_internal_anchor":true},{"citing_arxiv_id":"2507.08219","citing_title":"GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\\odot}$","ref_index":142,"is_internal_anchor":true},{"citing_arxiv_id":"1905.09300","citing_title":"Surrogate models for precessing binary black hole simulations with unequal masses","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2603.06010","citing_title":"Accelerated Time-domain Analysis for Gravitational Wave Astronomy","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"1903.04467","citing_title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","ref_index":38,"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":120,"is_internal_anchor":true},{"citing_arxiv_id":"2004.06503","citing_title":"Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2010.14527","citing_title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","ref_index":177,"is_internal_anchor":false},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":145,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04579","citing_title":"The Impact of Spin Priors on Parameterized Tests of General Relativity","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2111.03606","citing_title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","ref_index":111,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07388","citing_title":"GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog","ref_index":83,"is_internal_anchor":false},{"citing_arxiv_id":"2604.04546","citing_title":"Inference of recoil kicks from binary black hole mergers up to GWTC--4 and their astrophysical implications","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11903","citing_title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","ref_index":138,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13580","citing_title":"Investigating the effect of sensitivity of KAGRA on sky localization of gravitational-wave sources from compact binary coalescences","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2007.05579","citing_title":"Inferring the properties of a population of compact binaries in presence of selection effects","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI","json":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI.json","graph_json":"https://pith.science/api/pith-number/UXZI6NJURFILSUGUUFEBRBO4DI/graph.json","events_json":"https://pith.science/api/pith-number/UXZI6NJURFILSUGUUFEBRBO4DI/events.json","paper":"https://pith.science/paper/UXZI6NJU"},"agent_actions":{"view_html":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI","download_json":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI.json","view_paper":"https://pith.science/paper/UXZI6NJU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.7215&json=true","fetch_graph":"https://pith.science/api/pith-number/UXZI6NJURFILSUGUUFEBRBO4DI/graph.json","fetch_events":"https://pith.science/api/pith-number/UXZI6NJURFILSUGUUFEBRBO4DI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI/action/storage_attestation","attest_author":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI/action/author_attestation","sign_citation":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI/action/citation_signature","submit_replication":"https://pith.science/pith/UXZI6NJURFILSUGUUFEBRBO4DI/action/replication_record"}},"created_at":"2026-05-18T02:27:05.237584+00:00","updated_at":"2026-05-18T02:27:05.237584+00:00"}