{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:BXHOPHMBEG2DMERQ3JK3Y7DX5R","short_pith_number":"pith:BXHOPHMB","schema_version":"1.0","canonical_sha256":"0dcee79d8121b4361230da55bc7c77ec61fac7aa234ec3979938f2e79c2fb7ff","source":{"kind":"arxiv","id":"2301.02821","version":2},"attestation_state":"computed","paper":{"title":"Confusion noise from Galactic binaries for Taiji","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Chang Liu, Wen-Hong Ruan, Zong-Kuan Guo","submitted_at":"2023-01-07T09:51:01Z","abstract_excerpt":"Gravitational waves (GWs) from tens of millions of compact binaries in our Milky Way enter the milli-Hertz band of space-based detection. The majority of them cannot be resolved individually, resulting in a foreground confusion noise for Laser Interferometer Space Antenna (LISA). The concept of Taiji mission is similar to LISA's with slightly better sensitivity, which means that the galactic GW signals will also affect the detection with Taiji. Here we generate the GW signals from 29.8 million galactic binaries for Taiji and subtract the `resolvable' sources. The confusion noise is estimated 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":"2301.02821","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2023-01-07T09:51:01Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"bf7bb4adc6e0755e61a552d18557c7367543c93b8a2028771dab1c0cbdc6971c","abstract_canon_sha256":"077417cf3a1379a4db5b010616f6570a7541ea2fb595a6c176e7eca0db372d44"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:50:12.459985Z","signature_b64":"bGszNtjWIICA3b/5Dax8bVWwUAqhsjjodlkbd0aLspg2IsCFxepLWboCe9a36Iznx1Xzk68equ27BAotsbNvCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0dcee79d8121b4361230da55bc7c77ec61fac7aa234ec3979938f2e79c2fb7ff","last_reissued_at":"2026-07-05T05:50:12.459647Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:50:12.459647Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Confusion noise from Galactic binaries for Taiji","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Chang Liu, Wen-Hong Ruan, Zong-Kuan Guo","submitted_at":"2023-01-07T09:51:01Z","abstract_excerpt":"Gravitational waves (GWs) from tens of millions of compact binaries in our Milky Way enter the milli-Hertz band of space-based detection. The majority of them cannot be resolved individually, resulting in a foreground confusion noise for Laser Interferometer Space Antenna (LISA). The concept of Taiji mission is similar to LISA's with slightly better sensitivity, which means that the galactic GW signals will also affect the detection with Taiji. Here we generate the GW signals from 29.8 million galactic binaries for Taiji and subtract the `resolvable' sources. The confusion noise is estimated a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.02821","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/2301.02821/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":"2301.02821","created_at":"2026-07-05T05:50:12.459702+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.02821v2","created_at":"2026-07-05T05:50:12.459702+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.02821","created_at":"2026-07-05T05:50:12.459702+00:00"},{"alias_kind":"pith_short_12","alias_value":"BXHOPHMBEG2D","created_at":"2026-07-05T05:50:12.459702+00:00"},{"alias_kind":"pith_short_16","alias_value":"BXHOPHMBEG2DMERQ","created_at":"2026-07-05T05:50:12.459702+00:00"},{"alias_kind":"pith_short_8","alias_value":"BXHOPHMB","created_at":"2026-07-05T05:50:12.459702+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09713","citing_title":"PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2411.08691","citing_title":"Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term","ref_index":83,"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":94,"is_internal_anchor":false},{"citing_arxiv_id":"2601.00169","citing_title":"Isotropic stochastic gravitational wave background reconstruction for Taiji constellation","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":111,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13564","citing_title":"Topologically equivalent yet radiatively distinct orbits in EMRI system","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R","json":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R.json","graph_json":"https://pith.science/api/pith-number/BXHOPHMBEG2DMERQ3JK3Y7DX5R/graph.json","events_json":"https://pith.science/api/pith-number/BXHOPHMBEG2DMERQ3JK3Y7DX5R/events.json","paper":"https://pith.science/paper/BXHOPHMB"},"agent_actions":{"view_html":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R","download_json":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R.json","view_paper":"https://pith.science/paper/BXHOPHMB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.02821&json=true","fetch_graph":"https://pith.science/api/pith-number/BXHOPHMBEG2DMERQ3JK3Y7DX5R/graph.json","fetch_events":"https://pith.science/api/pith-number/BXHOPHMBEG2DMERQ3JK3Y7DX5R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R/action/storage_attestation","attest_author":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R/action/author_attestation","sign_citation":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R/action/citation_signature","submit_replication":"https://pith.science/pith/BXHOPHMBEG2DMERQ3JK3Y7DX5R/action/replication_record"}},"created_at":"2026-07-05T05:50:12.459702+00:00","updated_at":"2026-07-05T05:50:12.459702+00:00"}