{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:EPG4CHZR5RYOHSXJQPX2B5P4CV","short_pith_number":"pith:EPG4CHZR","schema_version":"1.0","canonical_sha256":"23cdc11f31ec70e3cae983efa0f5fc1577576552cd9e8f21ac3aad3620c10268","source":{"kind":"arxiv","id":"2407.17052","version":1},"attestation_state":"computed","paper":{"title":"Method to search for inspiraling planetary-mass ultra-compact binaries using the generalized frequency-Hough transform in LIGO O3a data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Andrew L. Miller, Cristiano Palomba, Federico De Lillo, Lorenzo Pierini, Nancy Aggarwal, Ornella J. Piccinni, Pia Astone, Sebastien Clesse, Surabhi Sachdev","submitted_at":"2024-07-24T07:25:19Z","abstract_excerpt":"Gravitational waves from sub-solar mass primordial black holes could be detected in LIGO, Virgo and KAGRA data. Here, we apply a method originally designed to look for rapidly spinning-down neutron stars, the generalized frequency-Hough transform, to search for planetary-mass primordial black holes using data from the first half of the third observing run of advanced LIGO. In this companion paper to arXiv:2402.19468, in which the main results of our search are presented, we delve into the details of the search methodology, the choices we have made regarding the parameter space to explore, the "},"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":"2407.17052","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2024-07-24T07:25:19Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"b20d9aff91feeb99f2c4c60d13dfd84b4dc420c4565aa3ca50eac4605c400227","abstract_canon_sha256":"8e9c8e017cf0e13a2961bf52a669947980b683f82db8dace8f14b57f01971f7a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:18:28.871948Z","signature_b64":"gUOXOo56t5qws7u/+Lh1HEu5ccvFNJKQhBgg02qLl77G67PeOMP1PhYaXP3flhz4SEyb6pokYycq6zdMczynCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23cdc11f31ec70e3cae983efa0f5fc1577576552cd9e8f21ac3aad3620c10268","last_reissued_at":"2026-07-05T09:18:28.871460Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:18:28.871460Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Method to search for inspiraling planetary-mass ultra-compact binaries using the generalized frequency-Hough transform in LIGO O3a data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Andrew L. Miller, Cristiano Palomba, Federico De Lillo, Lorenzo Pierini, Nancy Aggarwal, Ornella J. Piccinni, Pia Astone, Sebastien Clesse, Surabhi Sachdev","submitted_at":"2024-07-24T07:25:19Z","abstract_excerpt":"Gravitational waves from sub-solar mass primordial black holes could be detected in LIGO, Virgo and KAGRA data. Here, we apply a method originally designed to look for rapidly spinning-down neutron stars, the generalized frequency-Hough transform, to search for planetary-mass primordial black holes using data from the first half of the third observing run of advanced LIGO. In this companion paper to arXiv:2402.19468, in which the main results of our search are presented, we delve into the details of the search methodology, the choices we have made regarding the parameter space to explore, the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.17052","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/2407.17052/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":"2407.17052","created_at":"2026-07-05T09:18:28.871514+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.17052v1","created_at":"2026-07-05T09:18:28.871514+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.17052","created_at":"2026-07-05T09:18:28.871514+00:00"},{"alias_kind":"pith_short_12","alias_value":"EPG4CHZR5RYO","created_at":"2026-07-05T09:18:28.871514+00:00"},{"alias_kind":"pith_short_16","alias_value":"EPG4CHZR5RYOHSXJ","created_at":"2026-07-05T09:18:28.871514+00:00"},{"alias_kind":"pith_short_8","alias_value":"EPG4CHZR","created_at":"2026-07-05T09:18:28.871514+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.15749","citing_title":"Constraints on primordial black holes from the first part of LIGO-Virgo-KAGRA fourth observing run","ref_index":59,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV","json":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV.json","graph_json":"https://pith.science/api/pith-number/EPG4CHZR5RYOHSXJQPX2B5P4CV/graph.json","events_json":"https://pith.science/api/pith-number/EPG4CHZR5RYOHSXJQPX2B5P4CV/events.json","paper":"https://pith.science/paper/EPG4CHZR"},"agent_actions":{"view_html":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV","download_json":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV.json","view_paper":"https://pith.science/paper/EPG4CHZR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.17052&json=true","fetch_graph":"https://pith.science/api/pith-number/EPG4CHZR5RYOHSXJQPX2B5P4CV/graph.json","fetch_events":"https://pith.science/api/pith-number/EPG4CHZR5RYOHSXJQPX2B5P4CV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV/action/storage_attestation","attest_author":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV/action/author_attestation","sign_citation":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV/action/citation_signature","submit_replication":"https://pith.science/pith/EPG4CHZR5RYOHSXJQPX2B5P4CV/action/replication_record"}},"created_at":"2026-07-05T09:18:28.871514+00:00","updated_at":"2026-07-05T09:18:28.871514+00:00"}