{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:5FDZYNQRW5E4FJJGB5JNQIIQUV","short_pith_number":"pith:5FDZYNQR","schema_version":"1.0","canonical_sha256":"e9479c3611b749c2a5260f52d82110a56eb92b07f526fc80f0d1350add5d8ce2","source":{"kind":"arxiv","id":"1608.05055","version":1},"attestation_state":"computed","paper":{"title":"The Advanced LIGO Photon Calibrators","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"(10) Kenyon College, 11), (11) Syracuse University), 2), (2) LIGO Hanford Observatory, 3), (3) University of Texas Rio Grande Valley, (4) University of Missisipi, 5) B. P. Abbott (6), (5) LIGO Livingston Observatory, 6), (6) California Institute of Technology, (7) Louisiana State University, (8) University of Florida, 9), (9) University of Pisa, A. J. Weinstein (6), A. Sottile (2, C. Cahillane (6), C. Conley (2, D. Tuyenbayev (2, E. Goetz (2, E. H. Anders (2), FL, Gainesville, G. Mendell (2), H. P. Daveloza (3), J. Berliner (2), J. Betzwieser (5), J. R. Gleason (8), J. S. Kissel (2), K. Izumi (2), L. Canete (2), M. Rodruck (2), M. Wade (10), M. West (2, P. B. Schwinberg (2), R. L. Savage (2) ((1) University of Oregon, S. Kandhasamy (4, S. Karki (1, S. Sachdev (6), T. D. Abbott (7), T. Sadecki (2), USA, V. Quetschke (3)","submitted_at":"2016-08-17T19:27:18Z","abstract_excerpt":"The two interferometers of the Laser Interferometry Gravitaional-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events, and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as Photon Calibrators. These systems, which were completely redesigned for Advanced LIGO, in"},"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":"1608.05055","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2016-08-17T19:27:18Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"570803d811dfdb72637709859718e8ed9cfefb120002cda885e4f83982245d91","abstract_canon_sha256":"5e1cb2062765aa6de2766e88055bf8c12ce3763eff7352f3a1cfa34c84e248ce"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:34.793986Z","signature_b64":"Bu6skAiMPaHAehrJzAKfvAQskNeQOGQf4cGarWXm5wUtbRFnI4X9Pc2KMOFaYgEJmk4ildGkjo7ba0b0uwpHBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e9479c3611b749c2a5260f52d82110a56eb92b07f526fc80f0d1350add5d8ce2","last_reissued_at":"2026-05-18T00:54:34.793503Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:34.793503Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Advanced LIGO Photon Calibrators","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"(10) Kenyon College, 11), (11) Syracuse University), 2), (2) LIGO Hanford Observatory, 3), (3) University of Texas Rio Grande Valley, (4) University of Missisipi, 5) B. P. Abbott (6), (5) LIGO Livingston Observatory, 6), (6) California Institute of Technology, (7) Louisiana State University, (8) University of Florida, 9), (9) University of Pisa, A. J. Weinstein (6), A. Sottile (2, C. Cahillane (6), C. Conley (2, D. Tuyenbayev (2, E. Goetz (2, E. H. Anders (2), FL, Gainesville, G. Mendell (2), H. P. Daveloza (3), J. Berliner (2), J. Betzwieser (5), J. R. Gleason (8), J. S. Kissel (2), K. Izumi (2), L. Canete (2), M. Rodruck (2), M. Wade (10), M. West (2, P. B. Schwinberg (2), R. L. Savage (2) ((1) University of Oregon, S. Kandhasamy (4, S. Karki (1, S. Sachdev (6), T. D. Abbott (7), T. Sadecki (2), USA, V. Quetschke (3)","submitted_at":"2016-08-17T19:27:18Z","abstract_excerpt":"The two interferometers of the Laser Interferometry Gravitaional-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucial for the observation of these events, and the extraction of parameters of the sources. The principal tools used to calibrate the responses of the second-generation (Advanced) LIGO detectors to gravitational waves are systems based on radiation pressure and referred to as Photon Calibrators. These systems, which were completely redesigned for Advanced LIGO, in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.05055","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":"1608.05055","created_at":"2026-05-18T00:54:34.793571+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.05055v1","created_at":"2026-05-18T00:54:34.793571+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.05055","created_at":"2026-05-18T00:54:34.793571+00:00"},{"alias_kind":"pith_short_12","alias_value":"5FDZYNQRW5E4","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_16","alias_value":"5FDZYNQRW5E4FJJG","created_at":"2026-05-18T12:30:01.593930+00:00"},{"alias_kind":"pith_short_8","alias_value":"5FDZYNQR","created_at":"2026-05-18T12:30:01.593930+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2508.13923","citing_title":"Hunting for new glitches in LIGO data using community science","ref_index":36,"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":32,"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":62,"is_internal_anchor":true},{"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":71,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11703","citing_title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","ref_index":38,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV","json":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV.json","graph_json":"https://pith.science/api/pith-number/5FDZYNQRW5E4FJJGB5JNQIIQUV/graph.json","events_json":"https://pith.science/api/pith-number/5FDZYNQRW5E4FJJGB5JNQIIQUV/events.json","paper":"https://pith.science/paper/5FDZYNQR"},"agent_actions":{"view_html":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV","download_json":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV.json","view_paper":"https://pith.science/paper/5FDZYNQR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.05055&json=true","fetch_graph":"https://pith.science/api/pith-number/5FDZYNQRW5E4FJJGB5JNQIIQUV/graph.json","fetch_events":"https://pith.science/api/pith-number/5FDZYNQRW5E4FJJGB5JNQIIQUV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV/action/storage_attestation","attest_author":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV/action/author_attestation","sign_citation":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV/action/citation_signature","submit_replication":"https://pith.science/pith/5FDZYNQRW5E4FJJGB5JNQIIQUV/action/replication_record"}},"created_at":"2026-05-18T00:54:34.793571+00:00","updated_at":"2026-05-18T00:54:34.793571+00:00"}