{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:CKVO6VDN2MUOWW4WF7XMQSXLJ2","short_pith_number":"pith:CKVO6VDN","schema_version":"1.0","canonical_sha256":"12aaef546dd328eb5b962feec84aeb4eae318577bb013de2a3158bcd1027e406","source":{"kind":"arxiv","id":"2306.02636","version":1},"attestation_state":"computed","paper":{"title":"Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Changshuo Yan, Wei-Tou Ni, Youjun Lu, Yuetong Zhao, Zhiwei Chen","submitted_at":"2023-06-05T07:11:36Z","abstract_excerpt":"The ground-based gravitational wave (GW) observatories discover a population of merging stellar binary black holes (BBHs), which are promising targets for multiband observations by the low-, middle-, and high-frequency GW detectors. In this paper, we investigate the multiband GW detections of BBHs and demonstrate the advantages of such observations in improving the localization and parameter estimates of the sources. We generate mock samples of BBHs by considering different formation models as well as the merger rate density constrained by the current observations (GWTC-3). We specifically con"},"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":"2306.02636","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-06-05T07:11:36Z","cross_cats_sorted":[],"title_canon_sha256":"166b541cda92bcd4b7cbda813624adf58dead477090b172650807bfd0c429f8d","abstract_canon_sha256":"756f00ddf51464421abf9cfff4e5840c7ca4e9b0b52279cfe57b760e4b838c91"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:17:20.009757Z","signature_b64":"NLaZziIwWpQIGsg/WktwsCeIwELNFgNPOgB1rsynlrn+hpQJ1Hj33AzGPrBoJfp2jLchULsKwjcLdeyTjRhLBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"12aaef546dd328eb5b962feec84aeb4eae318577bb013de2a3158bcd1027e406","last_reissued_at":"2026-07-05T06:17:20.009310Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:17:20.009310Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Changshuo Yan, Wei-Tou Ni, Youjun Lu, Yuetong Zhao, Zhiwei Chen","submitted_at":"2023-06-05T07:11:36Z","abstract_excerpt":"The ground-based gravitational wave (GW) observatories discover a population of merging stellar binary black holes (BBHs), which are promising targets for multiband observations by the low-, middle-, and high-frequency GW detectors. In this paper, we investigate the multiband GW detections of BBHs and demonstrate the advantages of such observations in improving the localization and parameter estimates of the sources. We generate mock samples of BBHs by considering different formation models as well as the merger rate density constrained by the current observations (GWTC-3). We specifically con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.02636","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2306.02636/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":"2306.02636","created_at":"2026-07-05T06:17:20.009374+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.02636v1","created_at":"2026-07-05T06:17:20.009374+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.02636","created_at":"2026-07-05T06:17:20.009374+00:00"},{"alias_kind":"pith_short_12","alias_value":"CKVO6VDN2MUO","created_at":"2026-07-05T06:17:20.009374+00:00"},{"alias_kind":"pith_short_16","alias_value":"CKVO6VDN2MUOWW4W","created_at":"2026-07-05T06:17:20.009374+00:00"},{"alias_kind":"pith_short_8","alias_value":"CKVO6VDN","created_at":"2026-07-05T06:17:20.009374+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07120","citing_title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","ref_index":199,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2","json":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2.json","graph_json":"https://pith.science/api/pith-number/CKVO6VDN2MUOWW4WF7XMQSXLJ2/graph.json","events_json":"https://pith.science/api/pith-number/CKVO6VDN2MUOWW4WF7XMQSXLJ2/events.json","paper":"https://pith.science/paper/CKVO6VDN"},"agent_actions":{"view_html":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2","download_json":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2.json","view_paper":"https://pith.science/paper/CKVO6VDN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.02636&json=true","fetch_graph":"https://pith.science/api/pith-number/CKVO6VDN2MUOWW4WF7XMQSXLJ2/graph.json","fetch_events":"https://pith.science/api/pith-number/CKVO6VDN2MUOWW4WF7XMQSXLJ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2/action/storage_attestation","attest_author":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2/action/author_attestation","sign_citation":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2/action/citation_signature","submit_replication":"https://pith.science/pith/CKVO6VDN2MUOWW4WF7XMQSXLJ2/action/replication_record"}},"created_at":"2026-07-05T06:17:20.009374+00:00","updated_at":"2026-07-05T06:17:20.009374+00:00"}