{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:LL4PVLOXI662SWGAOGERZYTINS","short_pith_number":"pith:LL4PVLOX","schema_version":"1.0","canonical_sha256":"5af8faadd747bda958c071891ce2686c8c91ff6c73fd7eb171f25e7e0a22bfb4","source":{"kind":"arxiv","id":"gr-qc/0409034","version":2},"attestation_state":"computed","paper":{"title":"Time-Delay Interferometry","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Massimo Tinto, Sanjeev V. Dhurandhar","submitted_at":"2004-09-07T23:19:46Z","abstract_excerpt":"Equal-arm interferometric detectors of gravitational radiation allow phase measurements many orders of magnitude below the intrinsic phase stability of the laser injecting light into their arms. This is because the noise in the laser light is common to both arms, experiencing exactly the same delay, and thus cancels when it is differenced at the photo detector. In this situation, much lower level secondary noises then set overall performance. If, however, the two arms have different lengths (as will necessarily be the case with space-borne interferometers), the laser noise experiences differen"},"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/0409034","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2004-09-07T23:19:46Z","cross_cats_sorted":[],"title_canon_sha256":"e8f60f7c8be09fc6fcd48fad97d433be84eaadeeacca1aeaa70f4a0cd29b4155","abstract_canon_sha256":"a5cfcc4e5dbb27ae77ac6f31cb23e4459be006febb3f6a41f209a54a0a2d740c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:26:09.387540Z","signature_b64":"S3/mAEXHqDciR/z/+l/C+HLJ6QbDjvkgq+BsVa0iRgWyp1/FQck6AugyTHvzxZUyrBlkSYTCWDFNjrRrBIMOCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5af8faadd747bda958c071891ce2686c8c91ff6c73fd7eb171f25e7e0a22bfb4","last_reissued_at":"2026-07-05T02:26:09.387031Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:26:09.387031Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Time-Delay Interferometry","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Massimo Tinto, Sanjeev V. Dhurandhar","submitted_at":"2004-09-07T23:19:46Z","abstract_excerpt":"Equal-arm interferometric detectors of gravitational radiation allow phase measurements many orders of magnitude below the intrinsic phase stability of the laser injecting light into their arms. This is because the noise in the laser light is common to both arms, experiencing exactly the same delay, and thus cancels when it is differenced at the photo detector. In this situation, much lower level secondary noises then set overall performance. If, however, the two arms have different lengths (as will necessarily be the case with space-borne interferometers), the laser noise experiences differen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0409034","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/gr-qc/0409034/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0409034","created_at":"2026-07-05T02:26:09.387090+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0409034v2","created_at":"2026-07-05T02:26:09.387090+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0409034","created_at":"2026-07-05T02:26:09.387090+00:00"},{"alias_kind":"pith_short_12","alias_value":"LL4PVLOXI662","created_at":"2026-07-05T02:26:09.387090+00:00"},{"alias_kind":"pith_short_16","alias_value":"LL4PVLOXI662SWGA","created_at":"2026-07-05T02:26:09.387090+00:00"},{"alias_kind":"pith_short_8","alias_value":"LL4PVLOX","created_at":"2026-07-05T02:26:09.387090+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.01318","citing_title":"Impact of Spacecraft Orbit Uncertainties and Velocity Mismodeling on the LISA Gravitational-Wave Response","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09713","citing_title":"PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28071","citing_title":"Construction of Sensitivity Curves for Dynamic LISA and Taiji","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2510.19047","citing_title":"Global time-frequency search for stellar-mass binary black holes in LISA","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2511.00996","citing_title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","ref_index":37,"is_internal_anchor":false},{"citing_arxiv_id":"2511.21488","citing_title":"Bayesian analysis of the complex singlet model with phase transition gravitational waves","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2601.00169","citing_title":"Isotropic stochastic gravitational wave background reconstruction for Taiji constellation","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2602.18560","citing_title":"Inferring the population properties of galactic binaries from LISA's stochastic foreground","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2603.28689","citing_title":"Probing soft signals of gravitational-wave memory with space-based interferometers","ref_index":83,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05537","citing_title":"Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS","json":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS.json","graph_json":"https://pith.science/api/pith-number/LL4PVLOXI662SWGAOGERZYTINS/graph.json","events_json":"https://pith.science/api/pith-number/LL4PVLOXI662SWGAOGERZYTINS/events.json","paper":"https://pith.science/paper/LL4PVLOX"},"agent_actions":{"view_html":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS","download_json":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS.json","view_paper":"https://pith.science/paper/LL4PVLOX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0409034&json=true","fetch_graph":"https://pith.science/api/pith-number/LL4PVLOXI662SWGAOGERZYTINS/graph.json","fetch_events":"https://pith.science/api/pith-number/LL4PVLOXI662SWGAOGERZYTINS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS/action/storage_attestation","attest_author":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS/action/author_attestation","sign_citation":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS/action/citation_signature","submit_replication":"https://pith.science/pith/LL4PVLOXI662SWGAOGERZYTINS/action/replication_record"}},"created_at":"2026-07-05T02:26:09.387090+00:00","updated_at":"2026-07-05T02:26:09.387090+00:00"}